<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OJG</journal-id><journal-title-group><journal-title>Open Journal of Geology</journal-title></journal-title-group><issn pub-type="epub">2161-7570</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojg.2015.55032</article-id><article-id pub-id-type="publisher-id">OJG-56667</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Earth&amp;Environmental Sciences</subject></subj-group></article-categories><title-group><article-title>
 
 
  Slope Year for the U-Pb Dating Method and Its Applications
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ie</surname><given-names>Yuan</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Science, Beijing, China</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>yuanjie@mail.iggcas.ac.cn</email></corresp></author-notes><pub-date pub-type="epub"><day>06</day><month>05</month><year>2015</year></pub-date><volume>05</volume><issue>05</issue><fpage>351</fpage><lpage>366</lpage><history><date date-type="received"><day>30</day>	<month>April</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>23</month>	<year>May</year>	</date><date date-type="accepted"><day>26</day>	<month>May</month>	<year>2015</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p><html>
 <head></head>
 
  The slope year
   
  t<sub>slope</sub> 
  for the U-Pb dating method is given as
   <img src="Edit_a586057a-4114-4846-95e0-635925d09e5e.bmp" alt="" />
  ,
   
  where λ<sub>238</sub> and λ<sub>235</sub> are the decay constants for <sup>238</sup>U and <sup>235</sup>U, respectively, and k is the slope of the tangent line at a point on either the Concordia or Discordia line. These two lines are determined by the initial <sup>206(7)</sup>Pb<sub>i</sub> concentrations in minerals. If <img src="Edit_1e65e700-58d6-4f66-b763-fb73e6c96874.bmp" width="0" height="0" alt="" /><img src="Edit_6d75aaf8-b9e1-4ace-a59c-b260328e1d43.bmp" alt="" />, the line is the Concordia. However, if<img src="Edit_067e558b-46c3-463f-8f70-18dc7cf7b981.bmp" alt="" />  (∧ is the logical operator “and”, also known as the logical conjunction), <img src="Edit_d59e7b82-c7bf-4977-a157-a6babbb86816.bmp" alt="" /> or <img src="Edit_c5656093-1cb8-41e5-b2a2-de8ad6de7d53.bmp" alt="" />, the line is Discordia. The Concordia line is of the form <img src="Edit_2314ee0c-5657-4641-9119-46bbf305f1df.bmp" alt="" /> (where p stands for the present), while the Discordia line has the form <img src="Edit_0312d7c9-57a9-4b34-ad73-767b0e204fcb.bmp" alt="" /> (where k and b are the slope and intercept of the straight line, respectively).
 
</html></p></abstract><kwd-group><kwd>Slope Year</kwd><kwd> U-Pb Dating</kwd><kwd> Zircon</kwd><kwd> Mass Spectrum</kwd><kwd> Isotope</kwd><kwd> Initial Pb Isotope Concentration</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In nature, uranium has three radioactive isotopes: <sup>238</sup>U(99.2743%), <sup>235</sup>U(0.7200%) and <sup>234</sup>U(0.0057%) [<xref ref-type="bibr" rid="scirp.56667-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.56667-ref2">2</xref>] . The former two isotopes decay in the forms:</p><disp-formula id="scirp.56667-formula390"><graphic  xlink:href="http://html.scirp.org/file/12-1210330x13.png"  xlink:type="simple"/></disp-formula><p>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x14.png" xlink:type="simple"/></inline-formula>,</p><p>where Q is the heat, β denotes the beta decay and He stands for the element Helium. The decay constants λ for <sup>238</sup>U and <sup>235</sup>U are <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x15.png" xlink:type="simple"/></inline-formula> a<sup>−1</sup> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x16.png" xlink:type="simple"/></inline-formula> a<sup>−1</sup>, respectively [<xref ref-type="bibr" rid="scirp.56667-ref2">2</xref>] -[<xref ref-type="bibr" rid="scirp.56667-ref4">4</xref>] .</p><p>These nuclear reactions occur in host minerals, such as zircon (ZrSiO<sub>4</sub>), and are the basis of the U-Pb dating method in geology [<xref ref-type="bibr" rid="scirp.56667-ref5">5</xref>] -[<xref ref-type="bibr" rid="scirp.56667-ref8">8</xref>] . In a mineral, Pb and U isotopes obey the exponential decay law:</p><disp-formula id="scirp.56667-formula391"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x17.png"  xlink:type="simple"/></disp-formula><p>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x18.png" xlink:type="simple"/></inline-formula>, (2)</p><p>where the subscripts i and p represent the initial measurement time and the present, respectively, and t is the age of the mineral [<xref ref-type="bibr" rid="scirp.56667-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.56667-ref6">6</xref>] .</p><p>The coordinates n(<sup>206</sup>Pb<sub>p</sub>)/n(<sup>238</sup>U<sub>p</sub>) (n, the number of isotopes in the bracket) as the ordinate and n(<sup>207</sup>Pb<sub>p</sub>)/ n(<sup>235</sup>U<sub>p</sub>) ratios as the abscissa form the Pb/U ratio diagram (<xref ref-type="fig" rid="fig1">Figure 1</xref>). Samples formed t years ago plot on either the Concordia or Discordia lines [<xref ref-type="bibr" rid="scirp.56667-ref9">9</xref>] -[<xref ref-type="bibr" rid="scirp.56667-ref12">12</xref>] . For instance, the classical Discordia line was discovered by Ahrens (1955) in Zimbabwe. Equation (1) divided by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x19.png" xlink:type="simple"/></inline-formula> is n(<sup>206</sup>Pb<sub>p</sub>)/n(<sup>238</sup>U<sub>p</sub>):</p><disp-formula id="scirp.56667-formula392"><label>. (3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x20.png"  xlink:type="simple"/></disp-formula><p>Similarly for n(<sup>207</sup>Pb<sub>p</sub>)/n(<sup>235</sup>U<sub>p</sub>), we have</p><disp-formula id="scirp.56667-formula393"><label>, (4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x21.png"  xlink:type="simple"/></disp-formula><p>from Equation (2).</p><p>To interpret the Discordia line, conventional theories have proposed: 1) this line was caused by Pb loss or U gain after formation of the host mineral [<xref ref-type="bibr" rid="scirp.56667-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.56667-ref11">11</xref>] -[<xref ref-type="bibr" rid="scirp.56667-ref17">17</xref>] , 2) the upper intersection of the Discordia and Concordia lines represents the crystallization age of the mineral [<xref ref-type="bibr" rid="scirp.56667-ref12">12</xref>] and 3) the lower intersection of the Discordia and Concordia lines represents the metamorphic age of the mineral [<xref ref-type="bibr" rid="scirp.56667-ref14">14</xref>] .</p><p>However, previous theories are not tenable when used in the following cases:</p><p>1) the lower intercept point is negative or</p><p>2) no upper intercept point exists.</p><p>For instance, in Zheng et al. (2012) (<xref ref-type="fig" rid="fig1">Figure 1</xref>), all zircons in YX1 from Yingxian lamproites were found to be discordant and yielded a lower intercept age of −370 &#177; 690 Ma. According to conventional theories, this age indicates that the samples will experience a metamorphic process in a distant age. In addition, in Zheng et al. (2012), all zircons in HBxa from Hebi basalt are also discordant, but yield no upper intercept age. According to conventional theories, these data indicate that the samples did not crystallize until the present. Apparently, the explanations do not conform to the objective facts: the samples are in front of scientists now. New studies should thus focus on resolving these discrepancies.</p><p>Herein, the slope years t<sub>slope</sub>s for the U-Pb dating method for the Concordia and Discordia lines are presented, and a method for estimating values for t<sub>slope</sub> from the experimental data is proposed. In addition, four examples are presented to illustrate the application of the proposed method.</p></sec><sec id="s2"><title>2. Methodology</title><sec id="s2_1"><title>2.1. Basic Assumptions</title><p>In this study, the basic assumptions for the U-Pb dating method included the following:</p><p>a) The decay constants λ<sub>238</sub> and λ<sub>235</sub> are precisely determined. For instance, the decay constants in Jaffey et al. (1971) are of good quality and widely accepted. The number of citations of this paper is greater than 1200 (data from Web of Science);</p><p>b) Host minerals are not influenced by chemical reactions after formation. The minerals included apatite [<xref ref-type="bibr" rid="scirp.56667-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.56667-ref19">19</xref>] , baddeleyite [<xref ref-type="bibr" rid="scirp.56667-ref20">20</xref>] -[<xref ref-type="bibr" rid="scirp.56667-ref25">25</xref>] , monazite [<xref ref-type="bibr" rid="scirp.56667-ref26">26</xref>] -[<xref ref-type="bibr" rid="scirp.56667-ref33">33</xref>] , tantalite [<xref ref-type="bibr" rid="scirp.56667-ref34">34</xref>] -[<xref ref-type="bibr" rid="scirp.56667-ref38">38</xref>] , titanite [<xref ref-type="bibr" rid="scirp.56667-ref39">39</xref>] -[<xref ref-type="bibr" rid="scirp.56667-ref41">41</xref>] , uraninite [<xref ref-type="bibr" rid="scirp.56667-ref42">42</xref>] [<xref ref-type="bibr" rid="scirp.56667-ref43">43</xref>] and zircon [<xref ref-type="bibr" rid="scirp.56667-ref44">44</xref>] [<xref ref-type="bibr" rid="scirp.56667-ref45">45</xref>] , etc.;</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Pb/U ratio diagram. This diagram shows the predicament for conventional theories. The Concordia (blue, colour for online version) and classical Discordia (black) for Zimbabwe samples (black diamond points) (Ahrens, 1955) are illustrated. This Discordia and Concordia intercept at A and B, for which the meanings in conventional theories are shown in the lower-right corner. Two counter-examples to traditional theories are also shown: HBxa (hexagon points and red Discordia, Zheng et al. (2012)) and YX1 (right triangle points and green Discordia, Zheng et al. (2012)). See discussions in text</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-1210330x22.png"/></fig><p>c) Present <sup>206(7)</sup>Pb<sub>p</sub> and <sup>235(8)</sup>U<sub>p</sub> isotope concentrations in host minerals can be precisely measured using mass spectrometry (MS). Such MS instruments include sensitive high mass-resolution ion microprobe (SHRIMP) [<xref ref-type="bibr" rid="scirp.56667-ref46">46</xref>] [<xref ref-type="bibr" rid="scirp.56667-ref47">47</xref>] , LaserProbe-inductively coupled plasma mass spectrometry (LP-ICPMS) [<xref ref-type="bibr" rid="scirp.56667-ref48">48</xref>] and Cameca IMS-series [<xref ref-type="bibr" rid="scirp.56667-ref44">44</xref>] [<xref ref-type="bibr" rid="scirp.56667-ref49">49</xref>] , etc.</p></sec><sec id="s2_2"><title>2.2. Slope k and Slope Year Tslope</title><p>In mathematics, the variance on the ordinate is a function of the variance on the abscissa [<xref ref-type="bibr" rid="scirp.56667-ref50">50</xref>] . Therefore, n(<sup>206</sup>Pb<sub>p</sub>)/n(<sup>238</sup>U<sub>p</sub>) is a function of n(<sup>207</sup>Pb<sub>p</sub>)/n(<sup>235</sup>U<sub>p</sub>) in the Pb/U diagram (<xref ref-type="fig" rid="fig2">Figure 2</xref>):</p><disp-formula id="scirp.56667-formula394"><label>. (5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x23.png"  xlink:type="simple"/></disp-formula><p>The theoretical expressions for this function under different conditions are given in Section 2.4.</p><p>Next, the slope k of the tangent line at point A on the general curve of Equation (5) was determined. The partial derivative of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x24.png" xlink:type="simple"/></inline-formula> (Equation (3)) with respect to t is</p><disp-formula id="scirp.56667-formula395"><label>. (6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x25.png"  xlink:type="simple"/></disp-formula><p>Similarly, we have</p><disp-formula id="scirp.56667-formula396"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x26.png"  xlink:type="simple"/></disp-formula><p>from Equation (4). Equation (6) divided by Equation (7) gives</p><disp-formula id="scirp.56667-formula397"><label>. (8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x27.png"  xlink:type="simple"/></disp-formula><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Pb/U ratio diagram. The general curve (in blue) for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x29.png" xlink:type="simple"/></inline-formula> and tangent line at point A on this curve are shown. The definition of the slope at this point is also given</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-1210330x28.png"/></fig><p>In this equation, the second part is the definition of the slope of the tangent line [<xref ref-type="bibr" rid="scirp.56667-ref50">50</xref>] :</p><disp-formula id="scirp.56667-formula398"><label>. (9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x30.png"  xlink:type="simple"/></disp-formula><p>This equation indicates that if t is determined, the value of k is a constant (<xref ref-type="table" rid="table1">Table 1</xref>) since t ≥ 0, 0 &lt; k ≤ 0.1575. In addition, the slope monotonically decreases with increasing time t (<xref ref-type="fig" rid="fig3">Figure 3</xref>).</p><p>If k is determined (see Section 2.6), the slope year is given by rewriting Equation (9):</p><disp-formula id="scirp.56667-formula399"><label>. (10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x31.png"  xlink:type="simple"/></disp-formula></sec><sec id="s2_3"><title>2.3. Initial <sup>206(7)</sup>Pb<sub>i</sub> Concentrations in Minerals</title><p>If the values for t<sub>slope</sub>, <sup>206(7)</sup>Pb<sub>p</sub> and <sup>235(8)</sup>U<sub>p</sub> are known, the initial <sup>206(7)</sup>Pb<sub>i</sub> concentrations in minerals can be determined using the following:</p><disp-formula id="scirp.56667-formula400"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x32.png"  xlink:type="simple"/></disp-formula><p>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x33.png" xlink:type="simple"/></inline-formula>, (12)</p><p>which are derived from Equations (1) and (2). Clearly, the concentrations are greater than or equal to zero:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x34.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s2_4"><title>2.4. Mathematical Expressions for the Concordia and Discordia Lines</title><p>The initial <sup>206(7)</sup>Pb<sub>i</sub> isotope concentrations determine the mathematical expressions for the general graph in <xref ref-type="fig" rid="fig2">Figure 2</xref>. This relationship can be demonstrated using assumed samples formed at the same time t with specific initial conditions. Assume there are three samples (1, 2 and 3, <xref ref-type="fig" rid="fig4">Figure 4</xref>(a)) with</p><disp-formula id="scirp.56667-formula401"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x35.png"  xlink:type="simple"/></disp-formula><p>and an additional three samples (4, 5 and 6, <xref ref-type="fig" rid="fig4">Figure 4</xref>(b)) with</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Plot of the slope k versus time t</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-1210330x36.png"/></fig><fig-group id="fig4"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Histories of Pb/U ratios (blue circle) for different samples on (a) Concordia and (b) Discordia. The red arrows indicate the direction of the evolution of each ratio.</title></caption><fig id ="fig4_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-1210330x37.png"/></fig><fig id ="fig4_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-1210330x38.png"/></fig></fig-group><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Values of the slope for specific years</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >t(Ma)</th><th align="center" valign="middle" >0</th><th align="center" valign="middle" >100</th><th align="center" valign="middle" >1000</th><th align="center" valign="middle" >2000</th><th align="center" valign="middle" >3000</th><th align="center" valign="middle" >4000</th><th align="center" valign="middle" >5000</th></tr></thead><tr><td align="center" valign="middle" >k<sup>a</sup></td><td align="center" valign="middle" >0.15751</td><td align="center" valign="middle" >0.14497</td><td align="center" valign="middle" >0.06870</td><td align="center" valign="middle" >0.02997</td><td align="center" valign="middle" >0.01307</td><td align="center" valign="middle" >0.00570</td><td align="center" valign="middle" >0.00249</td></tr></tbody></table></table-wrap><p>a, calculated from Equation (9)</p><disp-formula id="scirp.56667-formula402"><label>. (14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x39.png"  xlink:type="simple"/></disp-formula><p>The mathematical expressions are given by solving the first-order differential Equation (9) using Equations (3) and (4):</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x40.png" xlink:type="simple"/></inline-formula>. (15).</p><p>The solution to this equation is different for each set of samples.</p><p>a) For samples 1, 2 and 3, rewriting Equation (15) using Equation (13) gives</p><disp-formula id="scirp.56667-formula403"><label>. (16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x41.png"  xlink:type="simple"/></disp-formula><p>The general solution of Equation (16) is</p><disp-formula id="scirp.56667-formula404"><label>. (17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x42.png"  xlink:type="simple"/></disp-formula><p>Since the concentrations of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x43.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x44.png" xlink:type="simple"/></inline-formula> are both zero at t = 0, the result is 0 = 0 + C; thus, C = 0. Therefore,</p><disp-formula id="scirp.56667-formula405"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x45.png"  xlink:type="simple"/></disp-formula><p>or</p><disp-formula id="scirp.56667-formula406"><label>, (19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x46.png"  xlink:type="simple"/></disp-formula><p>which is the expression for the Concordia line.</p><p>b) For samples 4, 5 and 6, because of the existence of the variances in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x47.png" xlink:type="simple"/></inline-formula> and/or <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x48.png" xlink:type="simple"/></inline-formula> (Equation (14)), Equation (15) is not an elementary function and the solution to it cannot be obtained using elementary integral calculus.</p><p>This difficulty can be overcome in the following manner. Consider a geological body (containing samples 4, 5 and 6) with continuous <sup>206</sup>Pb<sub>i</sub>, <sup>207</sup>Pb<sub>i</sub>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x49.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x50.png" xlink:type="simple"/></inline-formula> distributions. Then <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x51.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x52.png" xlink:type="simple"/></inline-formula> in the system are continuous variables [<xref ref-type="bibr" rid="scirp.56667-ref50">50</xref>] . Looking back to the original differential Equation (9):</p><disp-formula id="scirp.56667-formula407"><label>. (20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x53.png"  xlink:type="simple"/></disp-formula><p>Since k is a constant when t is given (<xref ref-type="table" rid="table1">Table 1</xref>), the solution to this equation is</p><disp-formula id="scirp.56667-formula408"><label>, (21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x54.png"  xlink:type="simple"/></disp-formula><p>where k and b are the slope and intercept of the line, respectively. This equation shows that the general curve in <xref ref-type="fig" rid="fig2">Figure 2</xref> is a straight line, i.e. the Discordia line.</p><p>Equation (21) is consistent with the initial condition (Equation (14)). If k = 0.15751 (at t = 0) is applied:</p><disp-formula id="scirp.56667-formula409"><label>. (22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x55.png"  xlink:type="simple"/></disp-formula><p>This equation indicates that 1) in the geological system, <sup>206</sup>Pb<sub>i</sub>/<sup>238</sup>U<sub>i</sub> monotonically increases with increasing <sup>207</sup>Pb<sub>i</sub>/<sup>235</sup>U<sub>i</sub> from samples 4 to 5 to 6 (<xref ref-type="fig" rid="fig4">Figure 4</xref>(b)) and 2) these two ratios for the three samples cannot simultaneously be zero.</p></sec><sec id="s2_5"><title>2.5. Histories of Pb/U Ratios on the Concordia and Discordia Lines</title><p>The <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x56.png" xlink:type="simple"/></inline-formula> also determines the histories of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x57.png" xlink:type="simple"/></inline-formula> data points on the Concordia and Discordia lines. In <xref ref-type="fig" rid="fig4">Figure 4</xref>, the histories are shown for</p><p>a) samples 1, 2 and 3 (<xref ref-type="fig" rid="fig4">Figure 4</xref>(a)), for which when t = 0, the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x58.png" xlink:type="simple"/></inline-formula> points plot on the origin (0, 0) where the Concordia line begins (Equation (19)). As time increases, the slope of the curve decreases from 0.15751 (0 Ma) to 0.06870 (1000 Ma) to 0.02997 (2000 Ma) and finally to 0.01307 (3000 Ma) (<xref ref-type="table" rid="table1">Table 1</xref>) and</p><p>b) samples 4, 5 and 6 (<xref ref-type="fig" rid="fig4">Figure 4</xref>(b)), for which when t = 0 the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x59.png" xlink:type="simple"/></inline-formula> points plot on a straight line with slope 0.15751 (Equation (22)). As time increases, the three <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x60.png" xlink:type="simple"/></inline-formula> points plot on discordant lines with different slopes, and the slope of each line decreases from 0.15751 (0 Ma) to 0.06870 (1000 Ma) to 0.02997 (2000 Ma) and finally to 0.01307 (3000 Ma) (<xref ref-type="table" rid="table1">Table 1</xref>).</p></sec><sec id="s2_6"><title>2.6. Methods for Determining k from Experimental Data</title><p>For n <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x61.png" xlink:type="simple"/></inline-formula> <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x62.png" xlink:type="simple"/></inline-formula> data points obtained from a mass spectrum, the k values are given as follows.</p><p>a) If the n data points plot on the Concordia line (<xref ref-type="fig" rid="fig4">Figure 4</xref>(a)), using Equation (19), the slope of the ith data point is</p><disp-formula id="scirp.56667-formula410"><label>, (23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x63.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x64.png" xlink:type="simple"/></inline-formula>. The mean slope for all the n points is then</p><disp-formula id="scirp.56667-formula411"><label>. (24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x65.png"  xlink:type="simple"/></disp-formula><p>b) If the n data points plot on the Discordia line (<xref ref-type="fig" rid="fig4">Figure 4</xref>(b)), the slope can be determined using the least squares method [<xref ref-type="bibr" rid="scirp.56667-ref51">51</xref>] . This method gives a linear function for the points:</p><disp-formula id="scirp.56667-formula412"><label>, (25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x66.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.56667-formula413"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x67.png"  xlink:type="simple"/></disp-formula><p>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x68.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x69.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x70.png" xlink:type="simple"/></inline-formula>. See proofs for k<sub>Discordia</sub> in Appendix A.</p></sec><sec id="s2_7"><title>2.7. Error Propagation</title><p>For a function<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x71.png" xlink:type="simple"/></inline-formula>, where x, y and z are independent variables, the error (1σ) is given by</p><disp-formula id="scirp.56667-formula414"><label>, (27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x72.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x73.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x74.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x75.png" xlink:type="simple"/></inline-formula> are the standard errors for x, y and z, respectively [<xref ref-type="bibr" rid="scirp.56667-ref51">51</xref>] .</p><p>According to Equation (27), the standard error for t<sub>slope</sub> (Equation (10)) is</p><disp-formula id="scirp.56667-formula415"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x76.png"  xlink:type="simple"/></disp-formula><p>or</p><disp-formula id="scirp.56667-formula416"><label>, (29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x77.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x78.png" xlink:type="simple"/></inline-formula> a<sup>−1</sup> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x79.png" xlink:type="simple"/></inline-formula> a<sup>−1</sup> [<xref ref-type="bibr" rid="scirp.56667-ref3">3</xref>] and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x80.png" xlink:type="simple"/></inline-formula> is the standard error of the slope. Then the values for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x81.png" xlink:type="simple"/></inline-formula> are given as follows.</p><p>a) For concordant data, the standard error of the ith slope (Equation (23)) is</p><disp-formula id="scirp.56667-formula417"><label>, (30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x82.png"  xlink:type="simple"/></disp-formula><p>and the standard error of the mean slope (Equation (24)) is</p><disp-formula id="scirp.56667-formula418"><label>. (31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x83.png"  xlink:type="simple"/></disp-formula><p>b) For discordant data, the standard error of k in Equation (26) is</p><disp-formula id="scirp.56667-formula419"><label>. (32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x84.png"  xlink:type="simple"/></disp-formula><p>See proofs of this equation in Appendix A.</p><p>According to Equation (27), the standard error for <sup>206(207)</sup>Pb<sub>i</sub> (Equations (11) and (12)) is</p><disp-formula id="scirp.56667-formula420"><label>(33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x85.png"  xlink:type="simple"/></disp-formula><p>where m and n stand for 206(7) and 235(8) respectively, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x86.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x87.png" xlink:type="simple"/></inline-formula> are taken from experimental data, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x88.png" xlink:type="simple"/></inline-formula>is obtained using Equation (28) and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x89.png" xlink:type="simple"/></inline-formula> a<sup>−1</sup> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x90.png" xlink:type="simple"/></inline-formula> a<sup>−1</sup> [<xref ref-type="bibr" rid="scirp.56667-ref3">3</xref>] .</p></sec></sec><sec id="s3"><title>3. Applications</title><p>To demonstrate the validity of our work, four examples are illustrated (<xref ref-type="table" rid="table2">Table 2</xref> and <xref ref-type="fig" rid="fig5">Figure 5</xref>). <xref ref-type="table" rid="table2">Table 2</xref> includes original Pb/U isotope ratios from the published literature along with the slope years (i.e. U-Pb ages) when the samples were formed.</p><p>The first example comes from Qinghu granite in the Nanling Range, South China [<xref ref-type="bibr" rid="scirp.56667-ref44">44</xref>] . The Pb/U ratios in this granite are the concordant type (<xref ref-type="fig" rid="fig5">Figure 5</xref>(a)) [<xref ref-type="bibr" rid="scirp.56667-ref44">44</xref>] . The slope and slope year were calculated using Equations (24) and (10), respectively, and found to be k<sub>Concordia</sub> = 0.13792 &#177; 0.00025 and t<sub>slope</sub> = 160 &#177; 2 Ma (<xref ref-type="table" rid="table2">Table 2</xref>), which are in good agreement with values reported by Li et al., 2009.</p><fig-group id="fig5"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Present slope years (with 1σ error) for (a) Qinghu granite, (b) a Zimbabwe uranium deposit, (c) Yingxian amphibolites and (d) Hebi amphibolites. All data points except Zimbabwe are plotted with 1σ error bars. The norms of the residuals (R<sup>2</sup>) for the least squares fits are illustrated, and the slopes (with 1σ errors) are given. In (a), the red diamond indicates the mean value for all the measured data and the tangent line at this point coincides with the Concordia line.</title></caption><fig id ="fig5_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-1210330x91.png"/></fig><fig id ="fig5_2"><label>(c)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-1210330x92.png"/></fig><fig id ="fig5_3"><label> (d)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-1210330x93.png"/></fig><fig id ="fig5_4"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-1210330x94.png"/></fig></fig-group><p>The k and t<sub>slope</sub> values for the three discordant examples described in the introduction were also calculated using Equations (26) and (10), respectively. For the Zimbabwe uranium deposit (<xref ref-type="fig" rid="fig5">Figure 5</xref>(b)), the slope was k<sub>Discordia</sub> = 0.03950 &#177; 0.00178 and slope year was t<sub>slope</sub> = 1668 &#177; 55 Ma. For amphibolites in the Yingxian lamproite (YX1, <xref ref-type="fig" rid="fig5">Figure 5</xref>(c)), the slope was k<sub>Discordia</sub> = 0.06779 &#177; 0.00564 and slope year was t<sub>slope</sub> = 1016 &#177; 100 Ma. For Hebi amphibolites (HBxa, <xref ref-type="fig" rid="fig5">Figure 5</xref>(d)), the slope was k<sub>Discordia</sub> = 0.010734 &#177; 0.00196 and slope year was t<sub>slope</sub> = 3237 &#177; 220 Ma.</p></sec><sec id="s4"><title>4. Conclusion</title><p>A method for determining the slope year for the U-Pb dating method and initial <sup>206(7)</sup>Pb concentrations in samples was described. It was also found that if no <sup>206(7)</sup>Pb isotopes are initially present in minerals, the Pb/U ratios plot on the Concordia line. On the other hand, if <sup>206(7)</sup>Pb isotopes are initially present in minerals, the Pb/U ratios plot on the Discordia line. Therefore, the Discordia line is not the result of Pb loss or U gain. Furthermore, methods for determining the slope year using experimental data were also proposed and applied to data on four samples previously described in the literature. These results demonstrate that our approach is useful for geological research.</p><table-wrap-group id="2"><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Values for <sup>206</sup>Pb/<sup>238</sup>U, <sup>207</sup>Pb/<sup>235</sup>U, the slope (k) and the slope year (t<sub>slope</sub>) of zircons in different geological bodies. The Pb/U isotope ratios in the Qinghu granite (07QH-1), a Zimbabwe uranium deposit, Yingxian amphibolites (YX1) and Hebi amphibolites (HBxa) are taken from Li et al. (2009), Ahrens, (1955), Zheng et al. (2012) and Zheng et al. (2012), respectively</title></caption><table-wrap id="2_1"><table><tbody><thead><tr><th align="center" valign="middle"  rowspan="2"  >Type</th><th align="center" valign="middle"  colspan="6"  >Experiments</th><th align="center" valign="middle"  colspan="3"  >Present Results</th></tr></thead><tr><td align="center" valign="middle" >Locations</td><td align="center" valign="middle" >Samples</td><td align="center" valign="middle" ><sup>206</sup>Pb/<sup>238</sup>U</td><td align="center" valign="middle" >1σ</td><td align="center" valign="middle" ><sup>207</sup>Pb/<sup>235</sup>U</td><td align="center" valign="middle" >1σ</td><td align="center" valign="middle" >Item</td><td align="center" valign="middle" >Value</td><td align="center" valign="middle" >1σ</td></tr><tr><td align="center" valign="middle" >Concordia</td><td align="center" valign="middle" >07QH-1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >0.0250</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.171</td><td align="center" valign="middle" >0.003</td><td align="center" valign="middle" >k</td><td align="center" valign="middle" >0.13792</td><td align="center" valign="middle" >0.00025</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >0.0253</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.172</td><td align="center" valign="middle" >0.002</td><td align="center" valign="middle" >t<sub>slope </sub></td><td align="center" valign="middle" >160</td><td align="center" valign="middle" >2 Ma</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >3</td><td align="center" valign="middle" >0.0252</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.172</td><td align="center" valign="middle" >0.003</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >0.0250</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.170</td><td align="center" valign="middle" >0.003</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >0.0252</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.172</td><td align="center" valign="middle" >0.002</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >0.0249</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.171</td><td align="center" valign="middle" >0.003</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >7</td><td align="center" valign="middle" >0.0251</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.173</td><td align="center" valign="middle" >0.002</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >8</td><td align="center" valign="middle" >0.0251</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.168</td><td align="center" valign="middle" >0.003</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >9</td><td align="center" valign="middle" >0.0251</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.176</td><td align="center" valign="middle" >0.003</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >10</td><td align="center" valign="middle" >0.0251</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.170</td><td align="center" valign="middle" >0.003</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >11</td><td align="center" valign="middle" >0.0251</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.172</td><td align="center" valign="middle" >0.002</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >12</td><td align="center" valign="middle" >0.0248</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.169</td><td align="center" valign="middle" >0.003</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >13</td><td align="center" valign="middle" >0.0251</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.172</td><td align="center" valign="middle" >0.003</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >14</td><td align="center" valign="middle" >0.0250</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.170</td><td align="center" valign="middle" >0.002</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >15</td><td align="center" valign="middle" >0.0250</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.169</td><td align="center" valign="middle" >0.002</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >16</td><td align="center" valign="middle" >0.0249</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.166</td><td align="center" valign="middle" >0.002</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >17</td><td align="center" valign="middle" >0.0250</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.171</td><td align="center" valign="middle" >0.002</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >18</td><td align="center" valign="middle" >0.0249</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.170</td><td align="center" valign="middle" >0.002</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >19</td><td align="center" valign="middle" >0.0249</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.168</td><td align="center" valign="middle" >0.002</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >20</td><td align="center" valign="middle" >0.0252</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.174</td><td align="center" valign="middle" >0.002</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Mean</td><td align="center" valign="middle" >0.0250</td><td align="center" valign="middle" >0.0003</td><td align="center" valign="middle" >0.171</td><td align="center" valign="middle" >0.0025</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Discordia</td><td align="center" valign="middle" >Zimbabwe</td><td align="center" valign="middle" >Monazite(Manitoba)</td><td align="center" valign="middle" >0.634</td><td align="center" valign="middle" >0.000</td><td align="center" valign="middle" >14.75</td><td align="center" valign="middle" >0.00</td><td align="center" valign="middle" >k</td><td align="center" valign="middle" >0.03950</td><td align="center" valign="middle" >0.00178</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Monazite(Ebonite)</td><td align="center" valign="middle" >0.507</td><td align="center" valign="middle" >0.000</td><td align="center" valign="middle" >12.45</td><td align="center" valign="middle" >0.00</td><td align="center" valign="middle" >t<sub>slope</sub></td><td align="center" valign="middle" >1667</td><td align="center" valign="middle" >55 Ma</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Monazite(Jack Tin)</td><td align="center" valign="middle" >0.420</td><td align="center" valign="middle" >0.000</td><td align="center" valign="middle" >10.10</td><td align="center" valign="middle" >0.00</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Monazite(Irumi)</td><td align="center" valign="middle" >0.383</td><td align="center" valign="middle" >0.000</td><td align="center" valign="middle" >9.02</td><td align="center" valign="middle" >0.00</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Uraainite(Manitoba)</td><td align="center" valign="middle" >0.270</td><td align="center" valign="middle" >0.000</td><td align="center" valign="middle" >5.85</td><td align="center" valign="middle" >0.00</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Monazite(Antsirabe)</td><td align="center" valign="middle" >0.241</td><td align="center" valign="middle" >0.000</td><td align="center" valign="middle" >5.16</td><td align="center" valign="middle" >0.00</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Discordia</td><td align="center" valign="middle" >YX1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >0.33464</td><td align="center" valign="middle" >0.00363</td><td align="center" valign="middle" >5.22129</td><td align="center" valign="middle" >0.06472</td><td align="center" valign="middle" >k</td><td align="center" valign="middle" >0.06779</td><td align="center" valign="middle" >0.00564</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >0.34491</td><td align="center" valign="middle" >0.00368</td><td align="center" valign="middle" >5.52554</td><td align="center" valign="middle" >0.06520</td><td align="center" valign="middle" >t<sub>slope</sub></td><td align="center" valign="middle" >1016</td><td align="center" valign="middle" >100 Ma</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >3</td><td align="center" valign="middle" >0.33249</td><td align="center" valign="middle" >0.00385</td><td align="center" valign="middle" >5.12718</td><td align="center" valign="middle" >0.07519</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >0.33347</td><td align="center" valign="middle" >0.00352</td><td align="center" valign="middle" >5.19461</td><td align="center" valign="middle" >0.05960</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >0.21231</td><td align="center" valign="middle" >0.00226</td><td align="center" valign="middle" >3.66393</td><td align="center" valign="middle" >0.04298</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >0.33912</td><td align="center" valign="middle" >0.00358</td><td align="center" valign="middle" >5.34786</td><td align="center" valign="middle" >0.06130</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr></tbody></table></table-wrap><table-wrap id="2_2"><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" ></th><th align="center" valign="middle" >7</th><th align="center" valign="middle" >0.33246</th><th align="center" valign="middle" >0.00353</th><th align="center" valign="middle" >5.22593</th><th align="center" valign="middle" >0.06103</th><th align="center" valign="middle" ></th><th align="center" valign="middle" ></th><th align="center" valign="middle" ></th></tr></thead><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >8</td><td align="center" valign="middle" >0.24655</td><td align="center" valign="middle" >0.00268</td><td align="center" valign="middle" >3.94621</td><td align="center" valign="middle" >0.04940</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >9</td><td align="center" valign="middle" >0.30931</td><td align="center" valign="middle" >0.00328</td><td align="center" valign="middle" >5.33072</td><td align="center" valign="middle" >0.06161</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >10</td><td align="center" valign="middle" >0.26968</td><td align="center" valign="middle" >0.00309</td><td align="center" valign="middle" >4.22308</td><td align="center" valign="middle" >0.05705</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >11</td><td align="center" valign="middle" >0.34094</td><td align="center" valign="middle" >0.00374</td><td align="center" valign="middle" >5.29417</td><td align="center" valign="middle" >0.06276</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Discordia</td><td align="center" valign="middle" >Hbxa</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >0.31857</td><td align="center" valign="middle" >0.00389</td><td align="center" valign="middle" >6.52978</td><td align="center" valign="middle" >0.08636</td><td align="center" valign="middle" >k</td><td align="center" valign="middle" >0.010734</td><td align="center" valign="middle" >0.001956</td><td align="center" valign="middle"  rowspan="15"  ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >2c</td><td align="center" valign="middle" >0.37868</td><td align="center" valign="middle" >0.00542</td><td align="center" valign="middle" >11.83149</td><td align="center" valign="middle" >0.19556</td><td align="center" valign="middle" >t<sub>slope</sub></td><td align="center" valign="middle" >3237</td><td align="center" valign="middle" >220 Ma</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >2r</td><td align="center" valign="middle" >0.35917</td><td align="center" valign="middle" >0.00452</td><td align="center" valign="middle" >9.43864</td><td align="center" valign="middle" >0.13599</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >3c</td><td align="center" valign="middle" >0.32201</td><td align="center" valign="middle" >0.00375</td><td align="center" valign="middle" >6.60397</td><td align="center" valign="middle" >0.08699</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >3r</td><td align="center" valign="middle" >0.32726</td><td align="center" valign="middle" >0.00388</td><td align="center" valign="middle" >6.39918</td><td align="center" valign="middle" >0.08482</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >0.35923</td><td align="center" valign="middle" >0.00457</td><td align="center" valign="middle" >10.94269</td><td align="center" valign="middle" >0.15946</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >0.33858</td><td align="center" valign="middle" >0.00402</td><td align="center" valign="middle" >8.05032</td><td align="center" valign="middle" >0.10509</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >0.32256</td><td align="center" valign="middle" >0.00368</td><td align="center" valign="middle" >6.04709</td><td align="center" valign="middle" >0.07394</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >7</td><td align="center" valign="middle" >0.32507</td><td align="center" valign="middle" >0.00396</td><td align="center" valign="middle" >6.51079</td><td align="center" valign="middle" >0.08888</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >8</td><td align="center" valign="middle" >0.29783</td><td align="center" valign="middle" >0.00355</td><td align="center" valign="middle" >6.74590</td><td align="center" valign="middle" >0.09045</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >9</td><td align="center" valign="middle" >0.32970</td><td align="center" valign="middle" >0.00477</td><td align="center" valign="middle" >7.19338</td><td align="center" valign="middle" >0.12913</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >10</td><td align="center" valign="middle" >0.34275</td><td align="center" valign="middle" >0.00486</td><td align="center" valign="middle" >8.54210</td><td align="center" valign="middle" >0.14216</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >11</td><td align="center" valign="middle" >0.31630</td><td align="center" valign="middle" >0.00412</td><td align="center" valign="middle" >7.75610</td><td align="center" valign="middle" >0.12353</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >12</td><td align="center" valign="middle" >0.30213</td><td align="center" valign="middle" >0.00442</td><td align="center" valign="middle" >7.02483</td><td align="center" valign="middle" >0.12968</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >13</td><td align="center" valign="middle" >0.31948</td><td align="center" valign="middle" >0.00461</td><td align="center" valign="middle" >6.22754</td><td align="center" valign="middle" >0.13341</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr></tbody></table></table-wrap></table-wrap-group></sec><sec id="s5"><title>Acknowledgements</title><p>This work was supported by the National Natural Science Foundation of China (Grant Nos. 41303047, 90914010 and 41020134003).</p></sec><sec id="s6"><title>Appendix A: Standard Error (1σ) for the Slope Using the Least Squares Method</title><p>The least squares method is described in textbooks on probability statistics [<xref ref-type="bibr" rid="scirp.56667-ref51">51</xref>] [<xref ref-type="bibr" rid="scirp.56667-ref52">52</xref>]. For a measured set of values (x<sub>1</sub>, y<sub>1</sub>,) … (x<sub>n</sub><sub>,</sub>y<sub>n</sub>), there is a line:</p><disp-formula id="scirp.56667-formula421"><label>(A.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x95.png"  xlink:type="simple"/></disp-formula><p>that best fits the data. The quality of this line is determined by</p><disp-formula id="scirp.56667-formula422"><label>. (A.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x96.png"  xlink:type="simple"/></disp-formula><p>When <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x97.png" xlink:type="simple"/></inline-formula> is at its minimum value, the estimation (Equation (A.1)) is the “best” fitting of the measured data. This approach is referred to as the method of linear-least-squares.</p><p>To find the minimum value for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x98.png" xlink:type="simple"/></inline-formula>, the following equation must be solved:</p><disp-formula id="scirp.56667-formula423"><label>(A.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x99.png"  xlink:type="simple"/></disp-formula><p>giving</p><disp-formula id="scirp.56667-formula424"><label>, (A.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x100.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x101.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x102.png" xlink:type="simple"/></inline-formula>. Then Equation (A.1) becomes</p><disp-formula id="scirp.56667-formula425"><label>. (A.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x103.png"  xlink:type="simple"/></disp-formula><p>The variance of a new predicted <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x104.png" xlink:type="simple"/></inline-formula> then follows:</p><disp-formula id="scirp.56667-formula426"><label>, (A.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x105.png"  xlink:type="simple"/></disp-formula><p>where σ is the standard error of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-1210330x106.png" xlink:type="simple"/></inline-formula> or</p><disp-formula id="scirp.56667-formula427"><label>, (A.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x107.png"  xlink:type="simple"/></disp-formula><p>if n is very small. Because k follows a Gaussian distribution, its variance is</p><disp-formula id="scirp.56667-formula428"><label>(A.8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-1210330x108.png"  xlink:type="simple"/></disp-formula><p>The square root of this equation is the 1σ error of k.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.56667-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Rutherford, E. and Soddy, F. (1903) The Radioactivity of Uranium. Philosophical Magazine, 5, 25-30, 441-445.</mixed-citation></ref><ref id="scirp.56667-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Audi, G., Bersillon, O., Blachot, J. and Wapstra, A.H. (2003) The Nubase Evaluation of Nuclear and Decay Properties. Nuclear Physics A, 729, 3-128. http://dx.doi.org/10.1016/j.nuclphysa.2003.11.001</mixed-citation></ref><ref id="scirp.56667-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Jaffey, A.H., Flynn, K.F., Glendenin, L.E., Bentley, W.C. and Essling, A.M. (1971) Precision Measurement of Half-Lives and Specific Activities of 235U and 238U. Physical Review C, 4, 1889-1906.  
http://dx.doi.org/10.1103/PhysRevC.4.1889</mixed-citation></ref><ref id="scirp.56667-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Pomme, S., Garcia-Torano, E., Sibbens, G., Richter, S., Wellum, R., Stolarz, A., et al. (2008) U-234/U-235 Activity Ratios as a Probe for the U-238/U-235 Half-Life Ratio. Journal of Radioanalytical and Nuclear Chemistry, 277, 207-210. http://dx.doi.org/10.1007/s10967-008-0731-6</mixed-citation></ref><ref id="scirp.56667-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Baker, T., Perkins, C., Blake, K.L. and Williams, P.J. (2001) Radiogenic and Stable Isotope Constraints on the Genesis of the Eloise Cu-Au Deposits, Cloncurry District, Northwest Queensland. Economic Geology, 96, 723-742.  
http://dx.doi.org/10.2113/96.4.723</mixed-citation></ref><ref id="scirp.56667-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Muller, R. (1996) Radiogenic Isotope Geology. Physics Today, 49, 60. http://dx.doi.org/10.1063/1.2807660</mixed-citation></ref><ref id="scirp.56667-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Panneerselvam, K., Macfarlane, A.W. and Salters, V.J.M. (2012) Reconnaissance Lead Isotope Characteristics of the Blackbird Deposit: Implications for the Age and Origin of Cobalt-Copper Mineralization in the Idaho Cobalt Belt, United States. Economic Geology, 107, 1177-1188. http://dx.doi.org/10.2113/econgeo.107.6.1177</mixed-citation></ref><ref id="scirp.56667-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Solomon, M., Gemmell, J.B. and Zaw, K. (2004) Nature and Origin of the Fluids Responsible for Forming the Hellyer Zn-Pb-Cu, Volcanic-Hosted Massive Sulphide Deposit, Tasmania, Using Fluid Inclusions, and Stable and Radiogenic Isotopes. Ore Geology Reviews, 25, 89-124. http://dx.doi.org/10.1016/j.oregeorev.2003.11.001</mixed-citation></ref><ref id="scirp.56667-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Ahrens, L.H. (1955) Implications of the Rhodesia Age Pattern. Geochimica et Cosmochimica Acta, 8, 1-15.  
http://dx.doi.org/10.1016/0016-7037(55)90013-2</mixed-citation></ref><ref id="scirp.56667-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Mezger, K. and Krogstad, E.J. (1997) Interpretation of Discordant U-Pb Zircon Ages: An Evaluation. Journal of Metamorphic Geology, 15, 127-140. http://dx.doi.org/10.1111/j.1525-1314.1997.00008.x</mixed-citation></ref><ref id="scirp.56667-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">Tilton, G.R. (1960) Volume Diffusion as a Mechanism for Discordant Lead Ages. Journal of Geophysical Research, 65, 2933-2945. http://dx.doi.org/10.1029/JZ065i009p02933</mixed-citation></ref><ref id="scirp.56667-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">Wetherill, G.W. (1956) An Interpretation of the Rhodesia and Witwatersrand Age Patterns. Geochimica et Cosmochimica Acta, 9, 290-292. http://dx.doi.org/10.1016/0016-7037(56)90029-1</mixed-citation></ref><ref id="scirp.56667-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">Goldich, S.S. and Fischer, L.B. (1986) Air-Abrasion Experiments in U-Pb Dating of Zircon. Chemical Geology, 58, 195-215. http://dx.doi.org/10.1016/0168-9622(86)90010-2</mixed-citation></ref><ref id="scirp.56667-ref14"><label>14</label><mixed-citation publication-type="book" xlink:type="simple">Goldrich, S.S. and Mudrey, M.G. (1972) Dilatancy Model for Discordant U-Pb Zircon Ages. In: Tugarinov, A.I., Ed., Contributions to Recent Geochemistry and Analytical Chemistry, Nauka Publishing Office, Moscow, 415-418.</mixed-citation></ref><ref id="scirp.56667-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">Holmes, A. (1954) The Oldest Dated Minerals of the Rhodesian Shield. Nature, 173, 612-614. 
http://dx.doi.org/10.1038/173612a0</mixed-citation></ref><ref id="scirp.56667-ref16"><label>16</label><mixed-citation publication-type="other" xlink:type="simple">Silver, L.T. and Deutsch, S. (1961) Uranium-Lead Method on Zircons. Annals of the New York Academy of Sciences, 91, 279-283.</mixed-citation></ref><ref id="scirp.56667-ref17"><label>17</label><mixed-citation publication-type="journal" xlink:type="simple"><name name-style="western"><surname>Wasserburg</surname><given-names> G.J. </given-names></name>,<etal>et al</etal>. (<year>1963</year>)<article-title>Diffusion Processes in Lead-Uranium Systems</article-title><source> Journal of Geophysical Research</source><volume> 68</volume>,<fpage> 4823</fpage>-<lpage>4846</lpage>.<pub-id pub-id-type="doi"></pub-id></mixed-citation></ref><ref id="scirp.56667-ref18"><label>18</label><mixed-citation publication-type="other" xlink:type="simple">Chew, D.M., Sylvester, P.J. and Tubrett, M.N. (2011) U-Pb and Th-Pb Dating of Apatite by LA-ICPMS. Chemical Geology, 280, 200-216. http://dx.doi.org/10.1016/j.chemgeo.2010.11.010</mixed-citation></ref><ref id="scirp.56667-ref19"><label>19</label><mixed-citation publication-type="other" xlink:type="simple">Thomson, S.N., Gehrels, G.E., Ruiz, J. and Buchwaldt, R. (2012) Routine Low-Damage Apatite U-Pb Dating Using Laser Ablation-Multicollector-ICPMS. Geochemistry, Geophysics, Geosystems, 13, 1. 
http://dx.doi.org/10.1029/2011GC003928</mixed-citation></ref><ref id="scirp.56667-ref20"><label>20</label><mixed-citation publication-type="other" xlink:type="simple">Allibon, J., Ovtcharova, M., Bussy, F., Cosca, M., Schaltegger, U., Bussien, D., et al. (2011) Lifetime of an Ocean Island Volcano Feeder Zone: Constraints from U-Pb Dating on Coexisting Zircon and Baddeleyite, and 40AR/39AR Age Determinations, Fuerteventura, Canary Islandssp. Canadian Journal of Earth Sciences, 48, 567-592. 
http://dx.doi.org/10.1139/E10-032</mixed-citation></ref><ref id="scirp.56667-ref21"><label>21</label><mixed-citation publication-type="other" xlink:type="simple">Bayanova, T.B. and Yakovenchuk, V.N. (1994) U-Pb Dating of Baddeleyite and Zircon from Imandrites on the Kola Peninsula. Doklady Earth science sections, 323, 147-150.</mixed-citation></ref><ref id="scirp.56667-ref22"><label>22</label><mixed-citation publication-type="other" xlink:type="simple">de Assis Janasi, V., de Freitas, V.A. and Heaman, L.H. (2011) The Onset of Flood Basalt Volcanism, Northern Parana Basin, Brazil: A Precise U-Pb Baddeleyite/Zircon Age for a Chapeco-Type Dacite. Earth and Planetary Science Letters, 302, 147-153. http://dx.doi.org/10.1016/j.epsl.2010.12.005</mixed-citation></ref><ref id="scirp.56667-ref23"><label>23</label><mixed-citation publication-type="other" xlink:type="simple">Li, Q.-L., Li, X.-H., Liu, Y., Tang, G.-Q., Yang, J.-H. and Zhu, W.-G. (2010) Precise U-Pb and Pb-Pb Dating of Phanerozoic Baddeleyite by SIMS with Oxygen Flooding Technique. Journal of Analytical Atomic Spectrometry, 25, 1107-1113. http://dx.doi.org/10.1039/b923444f</mixed-citation></ref><ref id="scirp.56667-ref24"><label>24</label><mixed-citation publication-type="other" xlink:type="simple">Soderlund, U. (2006) U-Pb Baddeleyite Ages of Meso- and Neoproterozoic Dykes and Sills in Central Fennoscandia: A Review. 5th International Dyke Conference: Dyke Swarms—Time Markers of Crustal Evolution, IDC-5. Rovaniemi, 31 July 2005-3 August 2005, 75-84.</mixed-citation></ref><ref id="scirp.56667-ref25"><label>25</label><mixed-citation publication-type="other" xlink:type="simple">Wahlgren, C.H., Heaman, L.M., Kamo, S. and Ingvald, E. (1996) U-Pb Baddeleyite Dating of Dolerite Dykes in the Eastern Part of the Sveconorwegian Orogen, South-Central Sweden. Precambrian Research, 79, 227-237. 
http://dx.doi.org/10.1016/0301-9268(95)00094-1</mixed-citation></ref><ref id="scirp.56667-ref26"><label>26</label><mixed-citation publication-type="other" xlink:type="simple">Aleinikoff, J.N., Lack, J.F.S., Lund, K., Evans, K.V., Fanning, C.M., Mazdab, F.K., et al. (2012) Constraints on the Timing of Co-Cu Au Mineralization in the Blackbird District, Idaho, Using SHRIMP U-Pb Ages of Monazite and Xenotime Plus Zircon Ages of Related Mesoproterozoic Orthogneisses and Metasedimentary Rocks. Economic Geology, 107, 1143-1175. http://dx.doi.org/10.2113/econgeo.107.6.1143</mixed-citation></ref><ref id="scirp.56667-ref27"><label>27</label><mixed-citation publication-type="other" xlink:type="simple">Baltybaev, S.K., Levchenkov, O.A., Glebovitskii, V.A., Rizvanova, N.G., Yakubovich, O.V. and Fedoseenko, A.M. (2010) Timing of the Regional Postmigmatitic K-Feldspar Mineralization on the Base of U-Pb Dating of Monazite (Metamorphic Complex of the Northern Ladoga Region). Doklady Earth Sciences, 430, 186-189. 
http://dx.doi.org/10.1134/S1028334X1002008X</mixed-citation></ref><ref id="scirp.56667-ref28"><label>28</label><mixed-citation publication-type="other" xlink:type="simple">Bose, S., Dunkley, D.J., Dasgupta, S., Das, K. and Arima, M. (2011) India-Antarctica-Australia-Laurentia Connection in the Paleoproterozoic-Mesoproterozoic Revisited: Evidence from New Zircon U-Pb and Monazite Chemical Age Data from the Eastern Ghats Belt, India. Bulletin of the Geological Society of America, 123, 2031-2049. 
http://dx.doi.org/10.1130/B30336.1</mixed-citation></ref><ref id="scirp.56667-ref29"><label>29</label><mixed-citation publication-type="other" xlink:type="simple">Dunning, G.R., Macdonald, A.S. and Barr, S.M. (1995) Zircon and Monazite U-Pb Dating of the Doi Inthanon Core Complex, Northern Thailand: Implications for Extension within the Indosinian Orogen. Tectonophysics, 251, 197. 
http://dx.doi.org/10.1016/0040-1951(95)00037-2</mixed-citation></ref><ref id="scirp.56667-ref30"><label>30</label><mixed-citation publication-type="other" xlink:type="simple">Evans, J. and Zalasiewicz, J. (1996) U-Pb, Pb-Pb and Sm-Nd Dating of Authigenic Monazite: Implications for the Diagenetic Evolution of the Welsh Basin. Earth and Planetary Science Letters, 144, 421. 
http://dx.doi.org/10.1016/S0012-821X(96)00177-X</mixed-citation></ref><ref id="scirp.56667-ref31"><label>31</label><mixed-citation publication-type="other" xlink:type="simple">Peterman, E.M., Mattinson, J.M. and Hacker, B.R. (2012) Multi-Step TIMS and CA-TIMS Monazite U-Pb Geochronoogy. Chemical Geology, 312-313, 58-73. http://dx.doi.org/10.1016/j.chemgeo.2012.04.006</mixed-citation></ref><ref id="scirp.56667-ref32"><label>32</label><mixed-citation publication-type="other" xlink:type="simple">Rasmussen, B., Fletcher, I.R. and McNaughton, N.J. (2001) Dating Low-Grade Metamorphic Events by SHRIMP U-Pb Analysis of Monazite in Shales. Geology, 29, 963-966. 
http://dx.doi.org/10.1130/0091-7613(2001)029&lt;0963:DLGMEB&gt;2.0.CO;2</mixed-citation></ref><ref id="scirp.56667-ref33"><label>33</label><mixed-citation publication-type="other" xlink:type="simple">Rasmussen, B., Fletcher, I.R., Muhling, J.R., Mueller, A.G. and Hall, G.C. (2007) Bushveld-Aged Fluid Flow, Peak Metamorphism, and Gold Mobilization in the Witwatersrand Basin, South Africa: Constraints from in Situ SHRIMP U-Pb Dating of Monazite and Xenotime. Geology, 35, 931-934. http://dx.doi.org/10.1130/G23588A.1</mixed-citation></ref><ref id="scirp.56667-ref34"><label>34</label><mixed-citation publication-type="other" xlink:type="simple">Baumgartner, R., Romer, R.L., Moritz, R., Sallet, R. and Chiaradia, M. (2006) Columbite-Tantalite-Bearing Granitic Pegmatites from the Serido Belt, Northeastern Brazil: Genetic Constraints from U-Pb Dating and Pb Isotopes. Canadian Mineralogist, 44, 69-86. http://dx.doi.org/10.2113/gscanmin.44.1.69</mixed-citation></ref><ref id="scirp.56667-ref35"><label>35</label><mixed-citation publication-type="other" xlink:type="simple">Camacho, A., Baadsgaard, H., Davis, D.W. and Cerny, P. (2012) Radiogenic Isotope Systematics of the Tanco and Silverleaf Granitic Pegmatites, Winnipeg River Pegmatite District, Manitoba. Canadian Mineralogist, 50, 1775-1792. 
http://dx.doi.org/10.3749/canmin.50.6.1775</mixed-citation></ref><ref id="scirp.56667-ref36"><label>36</label><mixed-citation publication-type="other" xlink:type="simple">Melcher, F., Graupner, T., Henjes-Kunst, F., Oberthur, T., Sitnikova, M., Gabler, E., et al. (2008) Analytical Fingerprint of Columbite-Tantalite (Coltan) Mineralisation in Pegmatites—Focus on Africa. 9th International Congress for Applied Mineralogy, ICAM 2008, 8-10 September 2008, Brisbane, 615-624.</mixed-citation></ref><ref id="scirp.56667-ref37"><label>37</label><mixed-citation publication-type="other" xlink:type="simple">Melleton, J., Gloaguen, E., Frei, D., Novak, M. and Breiter, K. (2012) How Are the Emplacement of Rare-Element Pegmatites, Regional Metamorphism and Magmatism Interrelated in the Moldanubian Domain of the Variscan Bohemian Massif, Czech Republic? Canadian Mineralogist, 50, 1751-1773. http://dx.doi.org/10.3749/canmin.50.6.1751</mixed-citation></ref><ref id="scirp.56667-ref38"><label>38</label><mixed-citation publication-type="other" xlink:type="simple">Schmitt, A.K. and Zack, T. (2012) High-Sensitivity U-Pb Rutile Dating by Secondary Ion Mass Spectrometry (SIMS) with an O2+ Primary Beam. Chemical Geology, 332-333, 65-73. http://dx.doi.org/10.1016/j.chemgeo.2012.09.023</mixed-citation></ref><ref id="scirp.56667-ref39"><label>39</label><mixed-citation publication-type="other" xlink:type="simple">Essex, R.M. and Gromet, L.P. (2000) U-Pb Dating of Prograde and Retrograde Titanite Growth during the Scandian Orogeny. Geology, 28, 419-422. http://dx.doi.org/10.1130/0091-7613(2000)28&lt;419:UDOPAR&gt;2.0.CO;2</mixed-citation></ref><ref id="scirp.56667-ref40"><label>40</label><mixed-citation publication-type="other" xlink:type="simple">Nesterova, N.S., Kirnozova, T.I. and Fugzan, M.M. (2011) New U-Pb Titanite Age Data on the Rocks from the Karelian Craton and the Belomorian Mobile Belt, Fennoscandian Shield. Geochemistry International, 49, 1161-1167.  
http://dx.doi.org/10.1134/S0016702911120081</mixed-citation></ref><ref id="scirp.56667-ref41"><label>41</label><mixed-citation publication-type="other" xlink:type="simple">Spencer, K.J., Hacker, B.R., Kylander-Clark, A.R.C., Andersen, T.B., Cottle, J.M., Stearns, M.A., et al. (2013) Campaign-Style Titanite U-Pb Dating by Laser-Ablation ICP: Implications for Crustal Flow, Phase Transformations and Titanite Closure. Chemical Geology, 341, 84-101. http://dx.doi.org/10.1016/j.chemgeo.2012.11.012</mixed-citation></ref><ref id="scirp.56667-ref42"><label>42</label><mixed-citation publication-type="other" xlink:type="simple">Richards, J.P., Cumming, G.L., Krstic, D., Wagner, P.A. and Spooner, E.T.C. (1988) Pb Isotope Constraints on the Age of Sulfide Ore Deposition and U-Pb Age of Late Uraninite Veining at the Musoshi Stratiform Copper Deposit, Central African Copper Belt, Zaire. Economic Geology, 83, 724-741. http://dx.doi.org/10.2113/gsecongeo.83.4.724</mixed-citation></ref><ref id="scirp.56667-ref43"><label>43</label><mixed-citation publication-type="other" xlink:type="simple">Votyakov, S.L., Ivanov, K.S., Khiller, V.V., Bochkarev, V.S. and Erokhin, Y.V. (2011) Chemical Microprobe Th-U-Pb Age Dating of Monazite and Uraninite Grains from Granites of the Yamal Crystalline Basement. Doklady Earth Sciences, 439, 994-997. http://dx.doi.org/10.1134/S1028334X1107018X</mixed-citation></ref><ref id="scirp.56667-ref44"><label>44</label><mixed-citation publication-type="other" xlink:type="simple">Li, X.-H., Li, W.-X., Wang, S.-C., Li, Q.-L., Liu, Y. and Tang, G.-J. (2009) Role of Mantle-Derived Magma in Genesis of Early Yanshanian Granites in the Nanling Range, South China: In Situ Zircon Hf-O Isotopic Constraints. Scientia Sinica Terrae, 39, 872-887. http://dx.doi.org/10.1007/s11430-009-0117-9</mixed-citation></ref><ref id="scirp.56667-ref45"><label>45</label><mixed-citation publication-type="other" xlink:type="simple">Zheng, J.P., Griffin, W.L., Ma, Q., O’Reilly, S.Y., Xiong, Q., Tang, H.Y., et al. (2012) Accretion and Reworking beneath the North China Craton. Lithos, 149, 61-78. http://dx.doi.org/10.1016/j.lithos.2012.04.025</mixed-citation></ref><ref id="scirp.56667-ref46"><label>46</label><mixed-citation publication-type="other" xlink:type="simple">Compston, W., Williams, I.S. and Clement, S.W. (1982) U-Pb Ages within Single Zircons Using a Sensitive High Mass-Resolution Ion Microprobe. The 30th Annual Conference on Mass Spectrometry and Allied Topics, Abstracts, Honolulu, 15 February 1984, B525-B534.</mixed-citation></ref><ref id="scirp.56667-ref47"><label>47</label><mixed-citation publication-type="other" xlink:type="simple">Compston, W., Williams, I.S. and Meyer, C. (1984) U-Pb Geochronology of Zircons from Lunar Breccia 73217 Using a Sensitive High Mass-Resolution Ion Microprobe. Journal of Geophysical Research, 89, 525-534. 
http://dx.doi.org/10.1029/JB089iS02p0B525</mixed-citation></ref><ref id="scirp.56667-ref48"><label>48</label><mixed-citation publication-type="other" xlink:type="simple">Feng, R., Machado, N. and Ludden, J. (1993) Lead Geochronology of Zircon by Laser Probe-Inductively Coupled Plasma Mass Spectrometry (LP-ICPMS). Geochimica et Cosmochimica Acta, 57, 3479-3486. 
http://dx.doi.org/10.1016/0016-7037(93)90553-9</mixed-citation></ref><ref id="scirp.56667-ref49"><label>49</label><mixed-citation publication-type="other" xlink:type="simple">Srinivasan, G., Whitehouse, M.J., Weber, I. and Yamaguchi, A. (2004) U-Pb and Hf-W Chronometry of Zircons from Eucrite A881467. The 35th Lunar and Planetary Science Conference, League City, TX, 19 March 2004, 1709.</mixed-citation></ref><ref id="scirp.56667-ref50"><label>50</label><mixed-citation publication-type="other" xlink:type="simple">Fong, C.F.C.M., Kee, D.D. and Kaloni, P.N. (2002) Advanced Mathematics for Engineering and Science. World Scientific Publishing Co. Pte. Ltd, Singapore.</mixed-citation></ref><ref id="scirp.56667-ref51"><label>51</label><mixed-citation publication-type="other" xlink:type="simple">Wang, J., Qian, Z., Qian, W., Zhuang, Y., He, Y. and Pan, C. (1999) Analysis of Regression and Variance, in Probability Statistics (Engineering Mathematics). Tongji University, Shanghai, 240-247. (In Chinese)</mixed-citation></ref><ref id="scirp.56667-ref52"><label>52</label><mixed-citation publication-type="other" xlink:type="simple">Bühlmann, P. and M?chler, M. (2008) Computational Statistics, 4-10.  
https://stat.ethz.ch/education/semesters/ss2012/CompStat/sk.pdf</mixed-citation></ref></ref-list></back></article>