<?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">WJCMP</journal-id><journal-title-group><journal-title>World Journal of Condensed Matter Physics</journal-title></journal-title-group><issn pub-type="epub">2160-6919</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/wjcmp.2015.52008</article-id><article-id pub-id-type="publisher-id">WJCMP-55287</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Violating of the Essam-Fisher and Rushbrooke Relationships at Low Temperatures
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ladimir</surname><given-names>Udodov</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>Department of Theoretical Physics, Katanov Khakas State University, Abakan, Russia</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>udododvv@hotmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>01</day><month>04</month><year>2015</year></pub-date><volume>05</volume><issue>02</issue><fpage>55</fpage><lpage>59</lpage><history><date date-type="received"><day>4</day>	<month>January</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>30</month>	<year>March</year>	</date><date date-type="accepted"><day>1</day>	<month>April</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>
 
 
  The Essam-Fisher and Rushbrooke relationships (1963) that connect the equilibrium critical exponents of susceptibility, specific heat and order parameter (and some other relations that follow from the scaling hypothesis) are shown to be valid only if the critical temperature 
  T<sub>С</sub> &gt; 0 and 
  T → 
  T<sub>C</sub>. For phase transitions (PT’s) with 
  T<sub>C</sub> = 0 K
   these relations are proved to be of different form. This fact has been actually observed experimentally, but the reasons were not quite clear. A general formula containing the classical results as a special case is proposed. This formula is applicable to all equilibrium PT’s of any space dimension for both 
  T<sub>C</sub> = 0 and 
  T<sub>C</sub> &gt; 0. The predictions of the theory are consistent with the available experimental data and do not cast any doubts upon the scaling hypothesis.
 
</p></abstract><kwd-group><kwd>Essam-Fisher and Rushbrooke Relationships</kwd><kwd> The Equilibrium Critical Exponents</kwd><kwd> The Scaling Hypothesis</kwd><kwd> Low Temperatures</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The critical exponents and scaling hypothesis (Patashinsky and Pokrovsky (1964); Widom (1965); Domb and Hunter (1965); Kadanoff (1966)) underlying the theory of critical phenomena [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.55287-ref5">5</xref>] . Essam and Fisher equality [<xref ref-type="bibr" rid="scirp.55287-ref6">6</xref>] and Rushbrooke inequality [<xref ref-type="bibr" rid="scirp.55287-ref7">7</xref>] (as the most famous inequality between critical exponents) were discovered 52 years ago and everyone believed that the relations are performed. These relations are connected with the critical exponents of the specific heat (α, α'), susceptibility (γ, γ') and the order parameter β (determining of the critical exponents see below) [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.55287-ref7">7</xref>] . In 1965-1966, it was shown that under the scaling hypothesis the Essam and Fisher equality are fulfilled and the Rushbrooke inequality <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x5.png" xlink:type="simple"/></inline-formula> reduces to equality [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>]</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x6.png" xlink:type="simple"/></inline-formula>.)</p><p>These results were obtained under the assumption that the critical temperature is finite T<sub>С</sub> &gt; 0 and T→T<sub>C</sub>. However, recently quantum phase transitions (PT’s) have inspired a new interest in low-temperature thermodynamics and statistical physics [<xref ref-type="bibr" rid="scirp.55287-ref8">8</xref>] - [<xref ref-type="bibr" rid="scirp.55287-ref10">10</xref>] . For quantum PT’s the temperature of phase transition T<sub>C</sub> is zero. In this paper we show that if T<sub>С</sub> = 0 K, the classical Essam-Fisher equation and Rushbrooke inequality changes: the right-hand side equal to two, is replaced by one. Change as well, and some other equations for the critical exponents resulting from the scaling hypothesis. In this paper, we propose a general interpolation formula (generalized Essam-Fisher equality), the right side of which ranges from 2 to 1. This general formula is valid for both finite critical temperature and for the case of T<sub>С</sub> = 0 K. In the experimental measurements of the critical exponents for the PT's at low temperatures (T → 0) we can expect that the right side of these relations will be less than 2 [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] . The proposed theory can be tested for any quantum phase transitions [<xref ref-type="bibr" rid="scirp.55287-ref8">8</xref>] -[<xref ref-type="bibr" rid="scirp.55287-ref11">11</xref>] .</p><p>Even now there is evidence that these relations are broken. For example, for the magnetic transition in nickel we have [<xref ref-type="bibr" rid="scirp.55287-ref12">12</xref>] (within the framework of the scaling hypothesis γ = γ')</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x7.png" xlink:type="simple"/></inline-formula>.</p><p>For the critical point in CO<sub>2</sub> [<xref ref-type="bibr" rid="scirp.55287-ref12">12</xref>] , for example,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x8.png" xlink:type="simple"/></inline-formula>.</p><p>Explanations of these violations were absent apart from possible measurement errors, but everyone believed that the formulas are correct, since derived from thermodynamics. The situation is complicated by the fact that a breach of these relationships speaks about the disturbance of the scaling hypothesis [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.55287-ref5">5</xref>] . Though the apparent violations of the scaling hypothesis are discussed by Aharony and Ahlers [<xref ref-type="bibr" rid="scirp.55287-ref13">13</xref>] , they did not consider the case of zero critical temperature.</p><p>It turns out, if T<sub>С</sub> = 0, the classic relationships [<xref ref-type="bibr" rid="scirp.55287-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.55287-ref7">7</xref>] have the different form and this may be explains the apparent violations and it can save the scaling hypothesis.</p></sec><sec id="s2"><title>2. The Essam and Fisher Equality</title><p>First, we recall the usual derived Essam-Fisher equality. The order parameter in a weak field (or lack thereof) is proportional to [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>]</p><disp-formula id="scirp.55287-formula85"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x9.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x10.png" xlink:type="simple"/></inline-formula>, β is order parameter critical exponent. On the other hand in a weak field h, the order parameter is [<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>]</p><disp-formula id="scirp.55287-formula86"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x11.png"  xlink:type="simple"/></disp-formula><p>where χ?susceptibility, the critical exponent is determined by the ratio (in a weak field) [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>]</p><disp-formula id="scirp.55287-formula87"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x12.png"  xlink:type="simple"/></disp-formula><p>γ?the critical exponent of the susceptibility. In the field PT becomes fuzzy. If we substitute Equations (1) and (3) in Equation (2), we find blur for temperature interval of PT [<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>]</p><disp-formula id="scirp.55287-formula88"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x13.png"  xlink:type="simple"/></disp-formula><p>from which we obtain</p><disp-formula id="scirp.55287-formula89"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x14.png"  xlink:type="simple"/></disp-formula><p>The same interval of blur can be found from the requirement that a field term of potential G<sub>h</sub> is equal to a heat term G<sub>T</sub> [<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>] (G?the Gibbs potential [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>] )</p><disp-formula id="scirp.55287-formula90"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x15.png"  xlink:type="simple"/></disp-formula><p>where С<sub>р</sub>?heat capacity, for which the formula is valid in weak field [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>]</p><disp-formula id="scirp.55287-formula91"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x16.png"  xlink:type="simple"/></disp-formula><p>α, α'?the heat capacity critical exponents, within the framework of the scaling hypothesis α = α' [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] . Substituting Equations (5) and (7) into Equation (6) this gives</p><disp-formula id="scirp.55287-formula92"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x17.png"  xlink:type="simple"/></disp-formula><p>or</p><disp-formula id="scirp.55287-formula93"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x18.png"  xlink:type="simple"/></disp-formula><p>it is Essam and Fisher equality [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.55287-ref6">6</xref>] .</p><p>Longer arguments prove Rushbrooke inequality [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.55287-ref7">7</xref>] , which is true for the stable states</p><disp-formula id="scirp.55287-formula94"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x19.png"  xlink:type="simple"/></disp-formula><p>where the primed symbols correspond to the region below the PT point (at temperature<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x20.png" xlink:type="simple"/></inline-formula>), the order parameter critical exponent β is defined only in this area [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>] . In rare cases, the asymmetric phase can be high-temperature phase [<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>] , then the exponent β is determined for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x21.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s3"><title>3. The Case of Zero Critical Temperature</title><p>Note that the heat term has the form (6) only if T<sub>С</sub> &gt; 0. In fact, let</p><disp-formula id="scirp.55287-formula95"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x22.png"  xlink:type="simple"/></disp-formula><p>We show that the heat term G<sub>T</sub> in the form shown in Equation (6) leads to incorrect results. From Equation (11) it follows that</p><disp-formula id="scirp.55287-formula96"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x23.png"  xlink:type="simple"/></disp-formula><p>The thermal term becomes in the form (within the framework of the scaling hypothesis<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x24.png" xlink:type="simple"/></inline-formula>)</p><disp-formula id="scirp.55287-formula97"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x25.png"  xlink:type="simple"/></disp-formula><p>We find the entropy</p><disp-formula id="scirp.55287-formula98"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x26.png"  xlink:type="simple"/></disp-formula><p>and heat capacity (using Equations (12) and (14))</p><disp-formula id="scirp.55287-formula99"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x27.png"  xlink:type="simple"/></disp-formula><p>which contradicts Equation (7).</p><p>Let us find the right formula. Let heat term has the form <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x28.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.55287-formula100"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x29.png"  xlink:type="simple"/></disp-formula><p>We now find b. Heat capacity is</p><disp-formula id="scirp.55287-formula101"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x30.png"  xlink:type="simple"/></disp-formula><p>hence we have</p><disp-formula id="scirp.55287-formula102"><graphic  xlink:href="http://html.scirp.org/file/1-4800279x31.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.55287-formula103"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x32.png"  xlink:type="simple"/></disp-formula><p>Essam and Fisher equality will take the form [<xref ref-type="bibr" rid="scirp.55287-ref14">14</xref>]</p><disp-formula id="scirp.55287-formula104"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x33.png"  xlink:type="simple"/></disp-formula><p>which differs from the standard formula (9) [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.55287-ref6">6</xref>] .</p></sec><sec id="s4"><title>4. The General Case</title><p>In the general case may be offered the following interpolation formula (generalized Essam-Fisher equality)</p><disp-formula id="scirp.55287-formula105"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x34.png"  xlink:type="simple"/></disp-formula><p>where S-function is [<xref ref-type="bibr" rid="scirp.55287-ref14">14</xref>]</p><disp-formula id="scirp.55287-formula106"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x35.png"  xlink:type="simple"/></disp-formula><p>where positive constant n can be found either from the comparison with experiment, or from the microscopic theory. Indeed, if the T<sub>C</sub> = 0 (T &gt; 0), then we arrive at the formula (19). If T<sub>C</sub><sup> </sup>&gt; 0 and T → T<sub>C</sub>, we get a classical Essam and Fisher equality (9).</p><p>Turns out, if the number n is fraction, then S-function is a nonanalitic function at a point<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x36.png" xlink:type="simple"/></inline-formula>. For example, if<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x37.png" xlink:type="simple"/></inline-formula>, then the first derivative tends to infinity<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x38.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x39.png" xlink:type="simple"/></inline-formula>. If n is an integer, then the function <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x40.png" xlink:type="simple"/></inline-formula> can be decomposed into a series of x. For<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x41.png" xlink:type="simple"/></inline-formula>, we get decomposition into a series accurate within quadratic term</p><disp-formula id="scirp.55287-formula107"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x42.png"  xlink:type="simple"/></disp-formula><p>Now consider the case<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x43.png" xlink:type="simple"/></inline-formula>. S-function is rewritten as</p><disp-formula id="scirp.55287-formula108"><graphic  xlink:href="http://html.scirp.org/file/1-4800279x44.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.55287-formula109"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x45.png"  xlink:type="simple"/></disp-formula><p>Now the S-function is analytic function at a point<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x46.png" xlink:type="simple"/></inline-formula>. The decomposition into a series is</p><disp-formula id="scirp.55287-formula110"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x47.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x48.png" xlink:type="simple"/></inline-formula>. Note that formulas (23) and (24) it is also true if Т<sub>С</sub> → 0, however τ → 0, it follows from this Т → 0. Rushbrooke inequality in the general case is given by</p><disp-formula id="scirp.55287-formula111"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x49.png"  xlink:type="simple"/></disp-formula><p>that is, the right-hand side of equality (25) can be less than 2. We obtained a principal result: the right side of the classic relationships is not a constant, but rather a function that depends on the temperature and takes the values from 1 to 2.</p><p>Finally, two equalities which follow from the scaling hypothesis [<xref ref-type="bibr" rid="scirp.55287-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>]</p><disp-formula id="scirp.55287-formula112"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x50.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.55287-formula113"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x51.png"  xlink:type="simple"/></disp-formula><p>alter their appearance (d?the space dimension, ν?critical exponent of the correlation length). ε?critical exponent for strong field [<xref ref-type="bibr" rid="scirp.55287-ref3">3</xref>]</p><disp-formula id="scirp.55287-formula114"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x52.png"  xlink:type="simple"/></disp-formula><p>Scaling relations now take the form</p><disp-formula id="scirp.55287-formula115"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x53.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.55287-formula116"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800279x54.png"  xlink:type="simple"/></disp-formula><p>r?phase transition order in the sense of Baxter R. [<xref ref-type="bibr" rid="scirp.55287-ref2">2</xref>] , we believe that the scaling hypothesis is performed.</p><p>It should be noted that the S-function expresses the degree of “classical” behavior. Thus, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x55.png" xlink:type="simple"/></inline-formula>for the non-classical behavior and T<sub>С</sub> = 0 and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800279x56.png" xlink:type="simple"/></inline-formula> corresponds to the known regime [<xref ref-type="bibr" rid="scirp.55287-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.55287-ref7">7</xref>] .</p></sec><sec id="s5"><title>5. Conclusions</title><p>Thus showed that the classical Essam and Fisher equation and Rushbrooke inequality are only valid if the critical temperature T<sub>C</sub> is finite and T → T<sub>C</sub>. If the critical temperature is zero, the classic relationships change its form: on the right side instead of the deuce will be unit. Because at change of parameters critical temperature tends to zero for many quantum phase transitions, the right-hand side of these relations should be continuously varied from 2 to 1 [<xref ref-type="bibr" rid="scirp.55287-ref14">14</xref>] .</p><p>The real test of the results is possible for any quantum phase transitions [<xref ref-type="bibr" rid="scirp.55287-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.55287-ref10">10</xref>] as T → 0, for example for ferromagnetic Ce<sub>2.15</sub>Pd<sub>1.95</sub>In<sub>0.9</sub> [<xref ref-type="bibr" rid="scirp.55287-ref11">11</xref>] , for heavy-fermions systems [<xref ref-type="bibr" rid="scirp.55287-ref15">15</xref>] or for superconductors [<xref ref-type="bibr" rid="scirp.55287-ref10">10</xref>] .</p><p>We note that the relations (19), (20), (25) are equilibrium, which implies that the right side equal to one, is unlikely to be achieved because the relaxation time (the transition to the equilibrium state) at T → T<sub>C</sub> ~ 0 tends to infinity (critical slowing). In conclusion, it must be emphasized that the results can be observed at temperatures not very low (see [<xref ref-type="bibr" rid="scirp.55287-ref12">12</xref>] ).</p></sec><sec id="s6"><title>Acknowledgements</title><p>I thank S. Prosandeev and A. Levanyuk for discussions and I am grateful for discussions and the support to I. Naumov.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.55287-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Stanley, H.E. (1971) Introduction to Phase Transitions and Critical Phenomena. Physics Department Massachusetts Institute of Technology, Clarendon Press, Oxford.</mixed-citation></ref><ref id="scirp.55287-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Baxter, R.J. (1982) Exactly Solved Models in Statistical Mechanics. 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