<?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">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2014.518209</article-id><article-id pub-id-type="publisher-id">JMP-52749</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>
 
 
  A Possible Role of the Gailitis Resonance in Muon Catalyzed Fusion
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>hi</surname><given-names>Yu Hu</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>David</surname><given-names>Caballero</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Claremont Graduate University, Claremont, USA</addr-line></aff><aff id="aff1"><addr-line>Department of Physics and Astronomy, California State University, Long Beach, USA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>Chiyu.hu@CSULB.Edu(HYH)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>04</day><month>12</month><year>2014</year></pub-date><volume>05</volume><issue>18</issue><fpage>2142</fpage><lpage>2148</lpage><history><date date-type="received"><day>1</day>	<month>October</month>	<year>2014</year></date><date date-type="rev-recd"><day>26</day>	<month>October</month>	<year>2014</year>	</date><date date-type="accepted"><day>15</day>	<month>November</month>	<year>2014</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>
 
 
  In a previous JMP article published May 2013, a comprehensive calculation was presented for all properties of a number of long-life s-state Gailitis resonances lying just above the PS(
  n = 2) formation threshold in a positron-Hydrogen scattering system. The six open-channel calculation was carried out by solving a set of four hundred thousand coupled linear equations. The modified Faddeev equation was used to obtain the wave-amplitude for each of the six open channels. Details can be found in reference 
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  . This note presents some qualitative properties of Gailitis resonances in the scattering systems of d + tu just above the thresholds of the opening of a new channel of the muonic atoms tu(n) or du(n), n &gt; 2 is the principal quantum number. u is a negatively charged muon, d and t are the nuclei of the two isotopes of the Hydrogen atom with one and two neutrons in the nucleus respectively. We study the possible decay channels of some of the long-life Gailitis resonances. Of particular interest is a transition directly from a Gailitis (3-body) resonance to the bound states dtu molecular ions via a radiative emission of a photon or an external auger ejection of a nearby electron. Possible experimental evidence will be presented.
 
</p></abstract><kwd-group><kwd>Faddeev</kwd><kwd> Resonance</kwd><kwd> Cross Section</kwd><kwd> 3-Body Scattering</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Muon catalyzed fusion has had a long and exciting history since the discovery of the Vesman resonance formation mechanism [<xref ref-type="bibr" rid="scirp.52749-ref2">2</xref>] . For a comprehensive review of this subject and numerous references see refs. [<xref ref-type="bibr" rid="scirp.52749-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.52749-ref4">4</xref>] .</p><p>The Vesman resonance is a six-body system. A typical process is</p><disp-formula id="scirp.52749-formula595"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x5.png"  xlink:type="simple"/></disp-formula><p>D<sub>2</sub> is the molecule of heavy Hydrogen (deuteron atom). <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x6.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x7.png" xlink:type="simple"/></inline-formula> are the rovibrational quantum numbers of D<sub>2</sub>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x8.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x9.png" xlink:type="simple"/></inline-formula> are the rovibrational quantum numbers of the complex molecule on the right hand side of Equation (1).</p><p>This process is accomplished after the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x10.png" xlink:type="simple"/></inline-formula> + d sub-system on the left hand side resonantly transfers 0.66 eV of energy to the rovibrational energy of the large complex molecule and becomes a weakly bounded small molecular ion<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x11.png" xlink:type="simple"/></inline-formula>.</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x12.png" xlink:type="simple"/></inline-formula>lies only 0.66 eV below the muonic atom <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x13.png" xlink:type="simple"/></inline-formula> ground state.</p><p>Subsequent radiative decays lead to the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x14.png" xlink:type="simple"/></inline-formula> three-body ground state at 319.13 eV below <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x15.png" xlink:type="simple"/></inline-formula> threshold. The nuclear fusion takes place at a rate ~10<sup>8</sup>/s.</p><disp-formula id="scirp.52749-formula596"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x16.png"  xlink:type="simple"/></disp-formula><p>W. Beunlich et al. [<xref ref-type="bibr" rid="scirp.52749-ref5">5</xref>] measured the fusion time spectra in 1984. All of their measurements display a sharp transient structure with initial time peak much larger than 10<sup>8</sup>/s.</p><p>This large transient fusion rate is attributed to the epithermal energy collision in Equation (1) [<xref ref-type="bibr" rid="scirp.52749-ref6">6</xref>] . In this note, an argument will be presented for possible Gailitis resonance contribution to this initial transient fusion phenomenon. Section 2 will review [<xref ref-type="bibr" rid="scirp.52749-ref1">1</xref>] some properties of the Gailitis resonance [<xref ref-type="bibr" rid="scirp.52749-ref7">7</xref>] . Section 3 provides upper bounds for the life-time of the Gailitis resonances just above the thresholds of the new channels involving du(n) or <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x17.png" xlink:type="simple"/></inline-formula> for a number of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x18.png" xlink:type="simple"/></inline-formula>. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x19.png" xlink:type="simple"/></inline-formula>is the principal quantum number of the muonic atoms. Section 4 presents a simple model calculation to estimate the lower bound of the rate of radiative transition from a Gailitis resonance located just above the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x20.png" xlink:type="simple"/></inline-formula> energy level to a bound dtu molecular ion. This calculation is needed to support the discussion in section 5. Section 5 will discuss the possibility that the Gailitis resonance may have contributed to the unique experimental phenomenon, the appearance of large initial transient fusion peaks in muon catalyzed fusion experiments [<xref ref-type="bibr" rid="scirp.52749-ref5">5</xref>] .</p></sec><sec id="s2"><title>2. The Gailitis Resonance</title><p>The first indication of the existence of the Gailitis resonance was provided by Gailitis and Damburg in their calculation of the electron-Hydrogen scattering system [<xref ref-type="bibr" rid="scirp.52749-ref7">7</xref>] . The resonances become obsolescence, mainly due to a lack of interest. It was difficult to study it using conventional methods until recently [<xref ref-type="bibr" rid="scirp.52749-ref1">1</xref>] . They have much smaller energy widths compared to Feshbach resonances [<xref ref-type="bibr" rid="scirp.52749-ref1">1</xref>] and occupy much larger configuration space compared to the size of the atoms. That means the calculation must have small enough energy grids and large enough effective cut-off distances. Reference [<xref ref-type="bibr" rid="scirp.52749-ref1">1</xref>] provides such a calculation using the modified Faddeev equation. This calculation solved a six-open channel system from first principles without intermediate approximations of any kind.</p><p>A complete set of the properties of the resonances are calculated directly including their wave functions. As a result, it becomes possible to identify the simple physical mechanism responsible for these resonances. Namely, it is a “dynamic” Stark effect [<xref ref-type="bibr" rid="scirp.52749-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.52749-ref7">7</xref>] -[<xref ref-type="bibr" rid="scirp.52749-ref9">9</xref>] . While an atom with Coulomb degeneracy acquires a dipole moment in the field of colliding charged particles, this field also splits some of the Coulomb degeneracy into separate Stark energy levels. If the energy of the incoming particle matches the Stark energy split at certain distances from the target atom resonance occurs. The energy is transferred to the atom via the exchange of a photon. During the life-time of the resonance the incoming particle remains a wave packet centered at a distance <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x21.png" xlink:type="simple"/></inline-formula> from the atom that satisfies the following conditions, for more details see reference [<xref ref-type="bibr" rid="scirp.52749-ref1">1</xref>] :</p><disp-formula id="scirp.52749-formula597"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x22.png"  xlink:type="simple"/></disp-formula><p>or</p><disp-formula id="scirp.52749-formula598"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x23.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x24.png" xlink:type="simple"/></inline-formula>is the quantum number of the Gailitis resonances. The resonant energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x25.png" xlink:type="simple"/></inline-formula> is in atomic energy units.</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x26.png" xlink:type="simple"/></inline-formula>is calculated in mass-normalized Jacobian coordinates, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x27.png" xlink:type="simple"/></inline-formula>is the location of the center of the</p><p>wave packet in Jacobian coordinates. The atom is initially in an excited state with principal quantum number<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x28.png" xlink:type="simple"/></inline-formula>. Its energy levels depend only on <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x29.png" xlink:type="simple"/></inline-formula> (the Coulomb degeneracy).</p><p>Initially, the wave packet has a width equal to the DeBroglie wavelength of the incoming charged particle,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x30.png" xlink:type="simple"/></inline-formula>. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x31.png" xlink:type="simple"/></inline-formula>is of the order of magnitude as the fine structure energies or other non-Coulombic corrections which removes the Coulomb degeneracy.</p><p>Thus <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x32.png" xlink:type="simple"/></inline-formula> can be very small and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x33.png" xlink:type="simple"/></inline-formula> can be very long, usually more than 3-orders of magnitude larger than the size of the atom.</p><p>The life-time of the resonances (or the wave packet) can be determined using the uncertainty principle [<xref ref-type="bibr" rid="scirp.52749-ref9">9</xref>] , such that</p><disp-formula id="scirp.52749-formula599"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x34.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.52749-formula600"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x35.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.52749-formula601"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x36.png"  xlink:type="simple"/></disp-formula><p>The small energy width <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x37.png" xlink:type="simple"/></inline-formula> results in a long life-time for the Gailitis resonances.</p><p>Some useful information of the Gailitis resonance can be seen from <xref ref-type="fig" rid="fig1">Figure 1</xref>, taking from Ref. [<xref ref-type="bibr" rid="scirp.52749-ref1">1</xref>] , which illustrates its unique singular behavior in the resonant channels 5 and 6. Taking from the six open channel K-matrix [<xref ref-type="bibr" rid="scirp.52749-ref1">1</xref>] , the diagonal matrix elements of channels 5 and 6 are plotted as function of collision energies. The matrix elements and their corresponding phase-shifts cross the zero axis between adjacent singularities. They remain small and negative on the lower energy side of the resonances. But the phase-shifts moves rapidly towards 90 degree approaching the resonant energies, these repulsive behaviors [<xref ref-type="bibr" rid="scirp.52749-ref8">8</xref>] provide rapid deceleration forcing the incoming charged particle to deliver all of its energy to excite the Stark energy levels of the target at the speed of light via a Bremsstrahlung photon while the incoming particle wave packet remains far from the target Equation (3). The phase shift jumps from <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x38.png" xlink:type="simple"/></inline-formula> to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x39.png" xlink:type="simple"/></inline-formula> separated by a narrow energy gap. Near the end of the resonance, the phase shift drops rapidly from <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x40.png" xlink:type="simple"/></inline-formula> toward the next crossing of the zero’s. This indicates a strong attraction [<xref ref-type="bibr" rid="scirp.52749-ref8">8</xref>] between the atom and the incoming “particle” near the end of the resonance. This property could facilitate the collective radiation of the 3-body system as a whole among many other possibilities. Section 4 will provide more support for this conjecture.</p></sec><sec id="s3"><title>3. Lower Bounds of the Gailitis Resonant Energies in d + tu(n), t + du(n) Scattering with n ≥ 2</title><p>In principle, the calculation of ref. [<xref ref-type="bibr" rid="scirp.52749-ref1">1</xref>] for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x41.png" xlink:type="simple"/></inline-formula> can be extended to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x42.png" xlink:type="simple"/></inline-formula>. That is not practical at the present</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> The diagonal matrix elements <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x44.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x45.png" xlink:type="simple"/></inline-formula> are plotted against<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x46.png" xlink:type="simple"/></inline-formula>, the energy of channel (1). Singularities occur between <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x47.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x48.png" xlink:type="simple"/></inline-formula> for both <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x50.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x52.png" xlink:type="simple"/></inline-formula> respectively. 5 and 6 are the two resonant channels</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/16-7501989x43.png"/></fig><p>time, especially when the current interest for these systems involves <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x53.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.52749-ref10">10</xref>] , sufficient physics can be obtained with qualitative calculations. According to [<xref ref-type="bibr" rid="scirp.52749-ref10">10</xref>] , the muon replaces an electron in the ground state of the atom and becomes a muonic atom with principal quantum number<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x54.png" xlink:type="simple"/></inline-formula>.</p><p>The resonant series in Equation (3) must be truncated when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x55.png" xlink:type="simple"/></inline-formula> approaches the fine structure energy or the vacuum polarization energy splits such that it removes the Coulomb degeneracy of the atomic energy levels. Even though the latter effect can be larger than the former in muonic atoms, the former is very convenient to calculate for all principal quantum numbers n of a muonic atom.</p><p>For the purpose of estimating the lower bounds, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x56.png" xlink:type="simple"/></inline-formula>, and upper bounds<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x57.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x58.png" xlink:type="simple"/></inline-formula>at any<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x59.png" xlink:type="simple"/></inline-formula>, the fine structure energies are used. The fine structure of Coulomb energy levels can be found in any quantum mechanics textbook [<xref ref-type="bibr" rid="scirp.52749-ref8">8</xref>] . In general for any principal quantum number n and orbital angular momentum<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x60.png" xlink:type="simple"/></inline-formula>, the fine structure energy is:</p><disp-formula id="scirp.52749-formula602"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x61.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x62.png" xlink:type="simple"/></inline-formula>is the degenerate energy level of a Coulombic atom, α is the find structure constant.</p><p>In the following, a special case of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x63.png" xlink:type="simple"/></inline-formula> will be presented. It follows for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x64.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.52749-formula603"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x65.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.52749-formula604"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x66.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.52749-formula605"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x67.png"  xlink:type="simple"/></disp-formula><p>Equation (4), gives</p><disp-formula id="scirp.52749-formula606"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x68.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.52749-formula607"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x69.png"  xlink:type="simple"/></disp-formula><p>The wave length is in muonic Bohr radius au.</p><p>A similar table for t + du should have a difference of only ~1% from the numbers in <xref ref-type="table" rid="table1">Table 1</xref>. Please note, this table gives only the respective bounds of the Gailitis resonances. The properties of the resonance themselves can only be determined by the dynamic of the three-body systems, such as that carried out in reference [<xref ref-type="bibr" rid="scirp.52749-ref1">1</xref>] .</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Summarized bounds In d + tu(n)</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >n</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x70.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x71.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x72.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x73.png" xlink:type="simple"/></inline-formula>(sec)</th></tr></thead><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >5.408 (−6)</td><td align="center" valign="middle" >2.702 (3)</td><td align="center" valign="middle" >1.370 (−7)</td><td align="center" valign="middle" >0.8861 (−12)</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >5.125 (−8)</td><td align="center" valign="middle" >2.776 (4)</td><td align="center" valign="middle" >1.298 (−9)</td><td align="center" valign="middle" >0.9351 (−10)</td></tr><tr><td align="center" valign="middle" >20</td><td align="center" valign="middle" >6.531 (−9)</td><td align="center" valign="middle" >7.779 (4)</td><td align="center" valign="middle" >1.654 (−10)</td><td align="center" valign="middle" >0.7345 (−9)</td></tr><tr><td align="center" valign="middle" >30</td><td align="center" valign="middle" >1.9475 (−9)</td><td align="center" valign="middle" >1.4238 (5)</td><td align="center" valign="middle" >4.933 (−11)</td><td align="center" valign="middle" >0.2461 (−8)</td></tr><tr><td align="center" valign="middle" >40</td><td align="center" valign="middle" >0.8242 (−9)</td><td align="center" valign="middle" >2.1890 (5)</td><td align="center" valign="middle" >2.0869 (−11)</td><td align="center" valign="middle" >0.5816 (−8)</td></tr><tr><td align="center" valign="middle" >50</td><td align="center" valign="middle" >0.42278 (−9)</td><td align="center" valign="middle" >3.0565 (5)</td><td align="center" valign="middle" >1.0709 (−11)</td><td align="center" valign="middle" >1.1334 (−8)</td></tr></tbody></table></table-wrap><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x74.png" xlink:type="simple"/></inline-formula>. 1 a.u. = 5422.50 eV, a.u. is the muon atomic unit, all lengths are in au, au is the muonic Bohr radius, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x75.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x76.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s4"><title>4. Gailitis Resonances and Bound State dtu Molecular Ions</title><p>Can a photon or an auger electron carry away the excess energy between a Gailitis resonance and its bound state 3-body molecular ions, such as dtu in a d + tu scattering system?</p><p>The only satisfactory answer must be the precise solution of a time dependent multichannel 3-body quantum equation that is not possible at this time. Nevertheless, it is possible to find experimental evidence using the vast volume of experimental data on muon catalyzed fusion research [<xref ref-type="bibr" rid="scirp.52749-ref3">3</xref>] , and its plausible theoretical interpretation from presently available theoretical calculations [<xref ref-type="bibr" rid="scirp.52749-ref11">11</xref>] - [<xref ref-type="bibr" rid="scirp.52749-ref13">13</xref>] .</p><p>We use the perturbative formula of photon emission by a muonic atom (or one electron atom) [<xref ref-type="bibr" rid="scirp.52749-ref13">13</xref>] derived from the Golden Rule, the transition probability per unit time, P<sub>2</sub>, is</p><disp-formula id="scirp.52749-formula608"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x77.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x78.png" xlink:type="simple"/></inline-formula>is the photon energy, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x79.png" xlink:type="simple"/></inline-formula>is the fine structure constant, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x80.png" xlink:type="simple"/></inline-formula>is the initial atomic state, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x81.png" xlink:type="simple"/></inline-formula>is the final atomic state, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x82.png" xlink:type="simple"/></inline-formula>is the coordinate of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x83.png" xlink:type="simple"/></inline-formula> measured from the center of mass of the two body system and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x83.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x84.png" xlink:type="simple"/></inline-formula> is the radiative decay life-time of the excited state atom.</p><p>According to reference [<xref ref-type="bibr" rid="scirp.52749-ref11">11</xref>] , for the muonic atom pμ</p><disp-formula id="scirp.52749-formula609"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x85.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.52749-formula610"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x86.png"  xlink:type="simple"/></disp-formula><p>We have:</p><disp-formula id="scirp.52749-formula611"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x87.png"  xlink:type="simple"/></disp-formula><p>For the purpose of providing a lower bound, we propose a very simple model for the dipole matrix element in Equation (7).</p><disp-formula id="scirp.52749-formula612"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x88.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x89.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x90.png" xlink:type="simple"/></inline-formula>are the “size” of the initial and final state of the radiative decay respectively. Using this model, the transitions from <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x91.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x92.png" xlink:type="simple"/></inline-formula> are:</p><disp-formula id="scirp.52749-formula613"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x93.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.52749-formula614"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x94.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.52749-formula615"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x95.png"  xlink:type="simple"/></disp-formula><p>This is less than that of Equation (8), but is of the same order of magnitude.</p><p>This simple model can be used to provide a lower bound for the three body radiative decay.</p><p>Equation (7) must be modified for three-body bound state transitions:</p><disp-formula id="scirp.52749-formula616"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x96.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x97.png" xlink:type="simple"/></inline-formula>is measured from charged particle <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x97.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x98.png" xlink:type="simple"/></inline-formula> (including sign of the charge) to the center of mass of the three- body system. In the d-t-u system the center of mass is near the line joining d and t and inversely proportional to the masses from each of them respectively.</p><p>Consider the case when the initial state is a time dependent Gailitis resonance. As qualitatively described in Section 2 from the behavior of the phase shift, it is clear the perturbative formula (11) cannot be applied near the singular point which can be excluded from the following average over the life time of the resonance<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x99.png" xlink:type="simple"/></inline-formula>. Hence, during the life-time of the resonance, it can be assumed that the Gailitis resonance is normalized as a three body bound state. It follows:</p><disp-formula id="scirp.52749-formula617"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x100.png"  xlink:type="simple"/></disp-formula><p>From the qualitative behavior of the Gailitis resonance described in Section 2 the major contribution to the integral must come near the end of life of the resonance. It is possible to provide a lower bound to this integral using the model provided by the two-body radiative decay, Equation (9). The <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x101.png" xlink:type="simple"/></inline-formula> of Equation (3) is measured from d to the center of mass of tμ. Thus <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x102.png" xlink:type="simple"/></inline-formula> is the initial “radius” of the Gailitis resonance.</p><disp-formula id="scirp.52749-formula618"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x103.png"  xlink:type="simple"/></disp-formula><p>We are interested in the principle quantum number<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x104.png" xlink:type="simple"/></inline-formula>.</p><disp-formula id="scirp.52749-formula619"><graphic  xlink:href="http://html.scirp.org/file/16-7501989x105.png"  xlink:type="simple"/></disp-formula><p>thus the “size” of the initial state is of the order of the resonant wavelength, the final state is one of the bound states of the dtu molecular ions. Their “size” ranges from 3 au to 10 au (from unpublished calculations).</p><p>Consider the “size” of the final state<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x106.png" xlink:type="simple"/></inline-formula>. At<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x106.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x107.png" xlink:type="simple"/></inline-formula>, <xref ref-type="table" rid="table1">Table 1</xref> shows<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x106.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x107.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x108.png" xlink:type="simple"/></inline-formula>. Since the wave functions involved in Equation (12) cannot change appreciably during the short radiative life time<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x106.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x107.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x108.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x109.png" xlink:type="simple"/></inline-formula>, the time integral in Equation (12) can be replaced as follows</p><disp-formula id="scirp.52749-formula620"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x110.png"  xlink:type="simple"/></disp-formula><p>Equation (12) becomes</p><disp-formula id="scirp.52749-formula621"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x111.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x112.png" xlink:type="simple"/></inline-formula>from the transition of a Gailitis resonance just above the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x113.png" xlink:type="simple"/></inline-formula> muonic atom to one of the bound muonic molecules. Equation (14) gives</p><disp-formula id="scirp.52749-formula622"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/16-7501989x114.png"  xlink:type="simple"/></disp-formula><p>This value is comparable to that of Equation (8), thus supporting the possibility of dtu molecular formation via the Gailitis resonances.</p></sec><sec id="s5"><title>5. Discussion and Conclusions</title><p>Muon catalyzed fusion utilizing the six-body resonance Equation (1) is carried out in various mixtures of molecules of heavy Hydrogen and their nuclei, such as D<sub>2</sub>, DT and t. According to cascade models [<xref ref-type="bibr" rid="scirp.52749-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.52749-ref11">11</xref>] , when the negative muon is first introduced into such mixtures, it displaces a ground state electron from a D atom and forms an excited state muonic atom<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x115.png" xlink:type="simple"/></inline-formula>, with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x116.png" xlink:type="simple"/></inline-formula>. Ref. [<xref ref-type="bibr" rid="scirp.52749-ref11">11</xref>] shows that the Stark effect is by far the fastest process of all cascade processes. Before the cascade begins, <xref ref-type="table" rid="table1">Table 1</xref> suggests that the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x116.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x117.png" xlink:type="simple"/></inline-formula> atom can find a t nuclei with the appropriate energy Equation (3) from the vast volume of space tens and thousands of muonic Bohr radius around it. Thus Gailitis resonances are produced ahead of other cascade processes.</p><p>From <xref ref-type="table" rid="table1">Table 1</xref>, the lifetime of these resonances is of the order of 10<sup>−9</sup> sec. It is stable against all other pro- cesses [<xref ref-type="bibr" rid="scirp.52749-ref1">1</xref>] and comparable to radiative decay of muonic atoms with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x118.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.52749-ref11">11</xref>] . In case of Gailitis resonances, the 3-body correlation is very strong near the end of its life, the possibility exists that a photon or an Auger electron can carry away the extra energy of some ~3 kev and becomes one of the bound state dtu molecular ions.</p><p>Sakamoto et al. [<xref ref-type="bibr" rid="scirp.52749-ref12">12</xref>] presented direct measurements of the energy spectra of prompt X-rays from ppu and ddu fusion experiments respectively. The large peaks of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x119.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x119.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x120.png" xlink:type="simple"/></inline-formula>rays are clearly displaced. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x119.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x120.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x121.png" xlink:type="simple"/></inline-formula>rays are not clearly resolved from the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x119.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x120.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x121.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x122.png" xlink:type="simple"/></inline-formula> rays. Ref. [<xref ref-type="bibr" rid="scirp.52749-ref12">12</xref>] showed small structures around the energy 3 kev. The energy of an np -&gt; 1s X-ray is less than 2.65 kev. The ~3 kev X-ray can only come from radiative decay of a Gailitis resonance. If this can be confirmed, the Gailitis resonance could indeed contribute to the initial transient fusion peaks of Ref. [<xref ref-type="bibr" rid="scirp.52749-ref5">5</xref>] .</p><p>Clearly the contribution is not significant in these experiments.</p><p>A deuteron beam of appropriate range of energies that covers the energy levels of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x123.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x123.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x124.png" xlink:type="simple"/></inline-formula>, from <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x123.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x125.png" xlink:type="simple"/></inline-formula> to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x123.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/16-7501989x126.png" xlink:type="simple"/></inline-formula> should provide a sufficient number of Gailitis resonances to make a significant contribution to the formation of dtu molecular ions.</p><p>The advantages of this approach are:</p><p>1) The experiment can be carried out in room temperature.</p><p>2) Such low energy deuteron beam can be produced easily.</p><p>3) If it becomes necessary, precision quantum three-body.</p><p>Scattering calculations for this system is possible.</p><p>In view of the long-term needs for dependable clean nuclear energy, this simple mechanism for muon catalyzed fusion must be given a chance to be tested!</p></sec></body><back><ref-list><title>References</title><ref id="scirp.52749-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Hu, C.Y. and Caballero, D. (2013) Journal of Modern Physics, 4, 622-627.</mixed-citation></ref><ref id="scirp.52749-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Vesman, E.A. (1967) Soviet Physics-JETP Letters, 5, 91.</mixed-citation></ref><ref id="scirp.52749-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Petitjean, C. (2007) International Conference on Muon Catalyzed Fusion (uCF-07), 82-87.</mixed-citation></ref><ref id="scirp.52749-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Ponomarev, L.I. (2007) International Conference on Muon Catalyzed Fusion (uCF-07), 405-410.</mixed-citation></ref><ref id="scirp.52749-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Breunlich, W., et al. (1984) Physical Review Letters, 53, 1137. http://dx.doi.org/10.1103/PhysRevLett.53.1137</mixed-citation></ref><ref id="scirp.52749-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Faifman, M.P. and Ponomerev, L.I. (1991) Physics Letters, B265, 201-206. http://dx.doi.org/10.1016/0370-2693(91)90041-N</mixed-citation></ref><ref id="scirp.52749-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Gailitis, M. and Damburg, R. (1963) Soviet Physics-JETP, 17, 1107.</mixed-citation></ref><ref id="scirp.52749-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Shiff, L.I. (1949) Quantum Mechanics. Landau and Lifshitz, Quantum Mechanics, Non-Relative Theory.</mixed-citation></ref><ref id="scirp.52749-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Gailitis, M. and Damburg, R. (1963) Proceedings of the Physical Society, 82, 192. http://dx.doi.org/10.1088/0370-1328/82/2/305</mixed-citation></ref><ref id="scirp.52749-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Cohen, J.S. and Leon, M. (1985) Physical Review Letters, 55, 52. http://dx.doi.org/10.1103/PhysRevLett.55.52</mixed-citation></ref><ref id="scirp.52749-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">Markushin, V.E. (1994) Physical Review A, 50, 1137. http://dx.doi.org/10.1103/PhysRevA.50.1137</mixed-citation></ref><ref id="scirp.52749-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">Sakamoto, S., Ishia, K., Matsuzaki, T. and Nagamine, K. (1999) Hyperfine Interaction, 119, 115-120. http://dx.doi.org/10.1023/A:1012618905252</mixed-citation></ref><ref id="scirp.52749-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">Merzbacher, E. (1970) Quantum Mechanics. 2nd Edition, John Wiley &amp; Son, Inc., New York, 563.</mixed-citation></ref></ref-list></back></article>