<?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.2014.511104</article-id><article-id pub-id-type="publisher-id">JMP-47490</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>Investigation on Virtual State Contribution to Gauge Invariant Cross Section of e<sup>+</sup>e<sup>-</sup>→J/ψ+η<sub>c</sub> in Bethe-Salpeter Framework</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Shashank</surname><given-names>Bhatnagar</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ming</surname><given-names>Li</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Shiyuan</surname><given-names>Li</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Physics, Addis Ababa University, Addis Ababa, Ethiopia</addr-line></aff><aff id="aff2"><addr-line>School of Physics, Shandong University, Jinan, China</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>lishy@sdu.edu.cn(SL)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>30</day><month>06</month><year>2014</year></pub-date><volume>05</volume><issue>11</issue><fpage>1027</fpage><lpage>1035</lpage><history><date date-type="received"><day>14</day>	<month>January</month>	<year>2014</year></date><date date-type="rev-recd"><day>12</day>	<month>February</month>	<year>2014</year>	</date><date date-type="accepted"><day>8</day>	<month>March</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>
	It is
shown that the virtual states and relative momentum of the constituents of the
bound states are very important for the cross section of the process <!--[if gte vml 1]><v:shapetype id="_x0000_t75" coordsize="21600,21600" o:spt="75" o:preferrelative="t" path="m@4@5l@4@11@9@11@9@5xe" filled="f" stroked="f">
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</v:shape><![endif]--><!--[if !vml]-->e<sup>+</sup>e<sup>-</sup>→J/ψ+η<sub>c</sub><!--[endif]--><!--[if gte mso 9]><xml>
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</xml><![endif]--> with the help of the Bethe-Salpeter wave
function description of the bound states. The gauge invariance of the cross
section is demonstrated. The numerical results can explain the experimental
data. 
</p></abstract><kwd-group><kwd>Bethe-Salpeter Wave Function</kwd><kwd> Virtual States</kwd><kwd> Relative Momentum</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Heavy quarkonium physics has been the traditional arena of Quantum Chromodynamics (QCD) since <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\aeec94c4-5a45-443d-895f-51362fb60c31.png" xlink:type="simple"/></inline-formula> was discovered, in both perturbative (PT) and non-perturbative (NPT) aspects. The heavy quark mass provides a hard scale for PT QCD calculations. The mass term of fermions in the QCD Lagrangian is irrelevant to the colour symmetry, so that the confinement and NPT QCD mechanism for heavy and light quarks could be similar. These facts make the heavy quark a good tool in investigating the unsolved NPT QCD. A simplification is expected from the large mass of the heavy quark, so that it may be non-relativistic (NR) in the bound states. As a matter of fact, not only the relative momentum between heavy quarks in the bound states are considered small, but also these quarks are treated as almost on mass shell. The off shell states and the creation/annihilation of the heavy quarks are not taken into account in the description of the static bound state. This is justified for the rest quarkonia, as investigating their decay widths. In these processes, the largest energy scale is the quarkonium mass<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\d3682bec-3d31-43ca-9732-52445695d64d.png" xlink:type="simple"/></inline-formula>. However, in the hard production processes of heavy quarkonium at high energies, the hard scales like the transverse momentum are much larger than<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\6bae1c72-1a83-4ed9-8238-9ec56d1668cb.png" xlink:type="simple"/></inline-formula>. If there is no well justified factorization formula<sup>1</sup> for a certain process, the NR description of the bound states could not be straightforward applicable. In this case, more general framework, which is relativistic and robust to introduce enough number of parameters to describe the bound system, especially the off shell states of the heavy quarks, is needed. The Bethe-Salpeter (BS) wave function framework is one of the good choices. If various relativistic effects are found to be small or could be factorized from the static bound state, the BS framework will naturally leads to the NR descriptions.</p><p>In this paper, the cross section of the exclusive production process <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\d18054fe-bcad-47d8-817a-09d333034676.png" xlink:type="simple"/></inline-formula> at B factories [<xref ref-type="bibr" rid="scirp.47490-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref3">3</xref>] is studied in the BS framework. It has been found that the relativistic effects are necessary for explaining the large cross section of this process. We show that both the off-shell heavy quark states as well as the large relative momentum are important in the BS framework.</p><p>The double charm pair production process in B factory energies is of special significance. These four (anti)charms can be respectively grouped into two colour-singlet pairs, hence the colour-octet mechanism never plays important role because of the relatively much smaller colour-octet matrix elements. One can then concentrate on the effects of relative movement and heavy quark off shell states. It has been found that the decay width, as well as the energy distribution of the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\81618ea3-a236-4d12-9b80-f8aed099228f.png" xlink:type="simple"/></inline-formula> in <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\24bb7ccc-53ad-40c6-a6ec-4e34838c878e.png" xlink:type="simple"/></inline-formula> process [<xref ref-type="bibr" rid="scirp.47490-ref4">4</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref6">6</xref>] can be easily understood by considering such kind of process [<xref ref-type="bibr" rid="scirp.47490-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.47490-ref8">8</xref>] . It has also been suggested [<xref ref-type="bibr" rid="scirp.47490-ref9">9</xref>] double charm pair production is helpful to analyze the Tevatron polarization ’paradox’, which is refreshed by Tevatron RUNII [<xref ref-type="bibr" rid="scirp.47490-ref10">10</xref>] as well as LHC recently. When the discrepancy between the data [<xref ref-type="bibr" rid="scirp.47490-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref3">3</xref>] and the lowest order NRQCD calculation [<xref ref-type="bibr" rid="scirp.47490-ref11">11</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref13">13</xref>] for the exclusive process <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\0c4c3ba8-09a1-4291-b988-1aa0e45c68b8.png" xlink:type="simple"/></inline-formula> was presented, Many groups recognized and have shown the importance of the relativistic corrections, besides the higher order PT QCD corrections. It has been generally adopted that exclusive process could be more sensitive to the inner movements and more difficult to factorize.</p><p>The ways of incorporating the relativistic corrections can be grouped into two: One is in the NRQCD framework, the other is to employ various relativistic wave functions of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\8d03c0eb-55b1-4ed7-b2fe-079a2b8d902d.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\f2cb5e83-168a-43b5-8101-9866654499f1.png" xlink:type="simple"/></inline-formula>. Works in the NRQCD frameworks [<xref ref-type="bibr" rid="scirp.47490-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.47490-ref15">15</xref>] show that the relativistic correction is important, at the same time the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\01fc0e73-58a1-45d9-860d-07135ad476f7.png" xlink:type="simple"/></inline-formula> PQCD corrections are found also very large. The large higher order corrections [<xref ref-type="bibr" rid="scirp.47490-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.47490-ref17">17</xref>] indicate the requirement of all order summations. For the to-date review of works in this framework, one refers to [<xref ref-type="bibr" rid="scirp.47490-ref18">18</xref>] . Works in the framework of light-cone wave functions [<xref ref-type="bibr" rid="scirp.47490-ref19">19</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref23">23</xref>] , or other relativistic quark wave function [<xref ref-type="bibr" rid="scirp.47490-ref24">24</xref>] employ the same hard partonic process as the lowest order NRQCD approach. When the scale parameter in the wave function is large, the momentum fraction difference <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\d022bc88-37d6-4dc7-9d87-1eba7c560428.png" xlink:type="simple"/></inline-formula> is of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\1f9e2277-8e64-442c-a8de-65b4df568534.png" xlink:type="simple"/></inline-formula>, and this approach can explain the data well. In both the above frameworks, the charm quarks in the bound states are treated as almost on shell, i.e., factorization is assumed.</p><p>On the other hand, the bound states can be described by BS wave functions [<xref ref-type="bibr" rid="scirp.47490-ref25">25</xref>] [<xref ref-type="bibr" rid="scirp.47490-ref26">26</xref>] . The results [<xref ref-type="bibr" rid="scirp.47490-ref25">25</xref>] [<xref ref-type="bibr" rid="scirp.47490-ref26">26</xref>] with the heavy quark limit (HQL) employed and the partonic process the same as that of the lowest order NRQCD approach are consistent with data, i.e., much larger than that of the lowest order NRQCD. However, the HQL generally is considered as to make NR description of the quarks in the bound states valid. This fact implies that different approaches for “NR limit” (HQL vs. NRQCD) could lead to completely different results. There could be effects of the full BS approach not incorporated in the NRQCD framework (but kept in HQL) which enhance the cross section. Such experiences have been seen in history. For the electron in the hydrogen atom, the most important “relativistic effect” comes from the generators of the little group of the Lorentz group (SO(3)), i.e., spin. Such a quantum number can only be naturally deduced from the relativistic wave function/equation of the electron, i.e., the Dirac spinor/equation. The Sommerfeld relativistic corrections to the Bohr theory can never incorporate this.</p><p>Of course by the mention of this history we do not imply NRQCD cannot properly incorporate the spin effect of the bound state, but want to point out that it could be better to start from the completely relativistic framework, i.e., the full BS wave function without HQL, to investigate all the relativistic effects in the bound state, namely the off-shell states and the large relative movement of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\d8e038a6-a2bc-4ecc-8492-0bf7978ca25e.png" xlink:type="simple"/></inline-formula>. The off-shell states have never been (and can never) covered in all the above approaches, but once they are taken into account, the Feynman diagrams in <xref ref-type="fig" rid="fig1">Figure 1</xref> <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\551a5644-a02f-4f5a-b7b1-85e00e23e838.png" xlink:type="simple"/></inline-formula> naturally comes up. These three charm quark lines can never be all on shell at the same time that the four-momenta are all conserved for the two quark-hadron vertices (which requiring at least one of the charm</p><fig id="fig1"><label>Figure 1</label><caption><p> The momentum of each line is explicitly written. <img src="htmlimages\4-7501703x\999fc71c-604a-4ce5-b0f1-80687b5ffedf.png" width="56.25" height="28.75" />are colour indices for the quark line. There is another diagram with all the arrows of three loop fermion propagators backward</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\08b2f892-bb33-4ef5-b9b5-e16aee950743.png"/></fig><p>propagators off-shell at the order of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\91f3c6a5-1d27-4c12-8347-813314b9a98a.png" xlink:type="simple"/></inline-formula>). Hence all the above mentioned approaches, which neglect the consideration of off-shell states of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\e1cebac8-f6e7-450b-bffd-2a05c47716da.png" xlink:type="simple"/></inline-formula>, set these diagrams to be zero by hand. On the contrary, taking into account the the off-shell states and the large relative movement of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\538acbf3-3611-462b-bb04-e78ee4a05345.png" xlink:type="simple"/></inline-formula> in a self-consistent BS wave function framework, one has to make clear the contribution of these diagrams. Their contribution is not necessarily the leading, but depending on how large the effects of the off-shell states and relative movements, which need the concrete calculations to clarify.</p><p>Next section will be the introduction of the BS framework we employ, then followed by Section 3 for describing the calculation details. Here we do the loop integral directly in the momentum space rather than employing the Feynman parameters because of the complex form of the BS vertex. Such a method is quite general and can be applied to the calculation of much more complex production processes in the BS framework. We conclude and discuss at Section 4.</p></sec><sec id="s2"><title>2. The Bethe-Salpeter Framework for the Calculation</title><p>In quantum field theory, the BS wave function of a quarkonium is</p><disp-formula id="scirp.47490-formula1873"><label>(1)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\3cadf7d6-db24-4215-9dc6-ffa23a75e6b3.png"/></disp-formula><disp-formula id="scirp.47490-formula1874"><label>(2)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\2836e3a3-3dcd-402e-9419-1d85ffbfe757.png"/></disp-formula><p>where</p><disp-formula id="scirp.47490-formula1875"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\0bf57923-f759-4a3a-b883-2562dcf628ab.png"/></disp-formula><disp-formula id="scirp.47490-formula1876"><label>(3)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\c7bceee4-cb31-495d-928d-22a978621f81.png"/></disp-formula><p>for equal mass quark pair. <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\3374bccb-d7af-46bf-a0a6-c03cb6dd3c9d.png" xlink:type="simple"/></inline-formula>denotes the quark propagator with momentum<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\b8494761-16e6-40ea-88f3-02ad2b05c8dc.png" xlink:type="simple"/></inline-formula>. Equation (2) defines the BS vertex for the coupling of the bound state particle with the composite particles. One simple way to under-</p><p>stand this point is that one can get the coordinate space BS wave function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\883c0d8a-cef6-4126-a371-ae4967978389.png" xlink:type="simple"/></inline-formula> from the Green function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\6d3aca49-1fb2-4ad3-84ab-6ad9fffb6998.png" xlink:type="simple"/></inline-formula> employing the reduction formula. Here <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\6988410a-cefc-4a9a-9824-a8389c2d90f0.png" xlink:type="simple"/></inline-formula> is the field for the bound state particle B. So this <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\f7ac244a-8831-47b9-be4f-36bcabfc895e.png" xlink:type="simple"/></inline-formula> is just the coupling vertex which is the Green function without the ex-</p><p>ternal legs. Of course from such an observation we can only obtain the coupling vertex from the BS wave function in the special case that the B particle is on mass shell. However this is enough for our purpose since here we only study the case of the B particle production as the real physical particle. In the following concrete calculations, consistent with all the studies on the decay processes [<xref ref-type="bibr" rid="scirp.47490-ref27">27</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref29">29</xref>] , we take the quark propagator as the following form with an effective valence quark mass, i.e.,</p><disp-formula id="scirp.47490-formula1877"><label>(4)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\df2421c5-b8ef-45ed-8f52-f30ea1ec24ff.png"/></disp-formula><p>For incorporation of the inner information of the bound states obtained from their decay processes which we have investigated in the BS framework [<xref ref-type="bibr" rid="scirp.47490-ref27">27</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref29">29</xref>] , we here employ the Covariant Instantaneous Ansatz (CIA) for the BS wave function and BS equations same as [<xref ref-type="bibr" rid="scirp.47490-ref27">27</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref29">29</xref>] (and refs. therein) to do the calculations. In such a framework, the vertex is</p><disp-formula id="scirp.47490-formula1878"><label>(5)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\6b074b53-a16b-4ef5-a670-aeed2e3d0ecb.png"/></disp-formula><p>where</p><disp-formula id="scirp.47490-formula1879"><label>(6)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\0dcb4860-8ec7-4191-8227-8dc20069c617.png"/></disp-formula><disp-formula id="scirp.47490-formula1880"><label>(7)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\2eba4ba2-753e-44ae-9ce1-915052b8ec43.png"/></disp-formula><disp-formula id="scirp.47490-formula1881"><label>(8)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\ec9795e3-a082-4ca2-9e8f-a48e75b26fd3.png"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\a34fab5c-33df-4e78-999b-4cbb02d10f45.png" xlink:type="simple"/></inline-formula>is the normalization factor for the BS wave function. <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\b9383a83-7982-4bc4-acef-9fcca24d946c.png" xlink:type="simple"/></inline-formula>are the form obtained from Equation(4) with the momentum <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\f55bbca4-c9c8-4f7a-a344-55eaad7191ff.png" xlink:type="simple"/></inline-formula> replaced by<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\0ec807ee-5a7e-4d1a-8e06-b7a9adaeac7d.png" xlink:type="simple"/></inline-formula>, respectively. Equation (7) shows that the space component of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\cb4a5d83-a1b7-41d2-845d-7074c025b254.png" xlink:type="simple"/></inline-formula> is exactly the 3-dimension relative momentum between <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\67b7bae1-51d8-439c-a39c-cf966b400ef9.png" xlink:type="simple"/></inline-formula> in the quarkonium rest frame. <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\911df23a-766f-4ab4-8215-cc0821d52785.png" xlink:type="simple"/></inline-formula>contains the complete Dirac structures. Based on a simple power counting rule which has been investigated to NLO recently [<xref ref-type="bibr" rid="scirp.47490-ref27">27</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref29">29</xref>] , one can expand the structures as powers of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\e241ddd8-b082-4e90-ab30-d93255814022.png" xlink:type="simple"/></inline-formula>, and fit to the data to get the coefficients order by order. In this work we take the most simple and popular-used structure which belongs to the leading order. For vector meson <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\35ce1df5-4b61-490d-9345-1044598470eb.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.47490-formula1882"><label>(9)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\bdcab231-cf13-42fc-9c11-a9a7878045ef.png"/></disp-formula><p>For pseudo-scalar meson <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\97e52333-655a-4c69-8ad9-9b8ccb03c29f.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.47490-formula1883"><label>(10)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\439342fe-e895-4f69-b191-a0c1b37fa0cb.png"/></disp-formula><p>From comparing with the decay data, it has been found that the higher order Dirac structures do not contribute significantly to heavy quark bound states [<xref ref-type="bibr" rid="scirp.47490-ref27">27</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref29">29</xref>] . Only with more and more production processes are investigated within this BS framework and comparing with more and more precise data, it is possible to check how much other Dirac structures contribute in production processes.</p><p>The ground state scalar wave function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\9023c3ca-ea75-42b0-a04e-17d5996d2a31.png" xlink:type="simple"/></inline-formula> takes the form</p><disp-formula id="scirp.47490-formula1884"><label>(11)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\e1aa0375-7f89-4d81-a240-41d3dcf0a21c.png"/></disp-formula><p>which leave only one parameter <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\358f058d-cf94-45b4-86ee-5f77b15f67af.png" xlink:type="simple"/></inline-formula> to be determined. It is clearly defined in [<xref ref-type="bibr" rid="scirp.47490-ref27">27</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref29">29</xref>] , and is dependent on the quark mass. In this paper we leave it as a free parameter to see the dependence of cross section on it. As can be seen from the scalar wave function, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\92e9054f-3af0-46af-be33-e62feefb2624.png" xlink:type="simple"/></inline-formula>characterizes the distribution width of the relative momentum between<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\05ef05a0-5695-4273-adf3-1694cd69cc59.png" xlink:type="simple"/></inline-formula>. This point will be further discussed in next section.</p></sec><sec id="s3"><title>3. The Calculation Procedure and the Results</title><p>The invariant amplitude for the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\cf41ed5e-97a6-4b94-b081-ef1f9bef398a.png" xlink:type="simple"/></inline-formula> process is<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\d5adf274-0e20-4230-ac1e-a517f75cfff3.png" xlink:type="simple"/></inline-formula>, corresponding to two Feynman diagrams. It is easy to show that<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\9dfb5527-96d4-42d8-8aea-d4b9b4a25e02.png" xlink:type="simple"/></inline-formula>, so <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\9b8b45b2-489a-4d1c-9990-4177741c293a.png" xlink:type="simple"/></inline-formula> is</p><disp-formula id="scirp.47490-formula1885"><label>(12)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\4fd47499-ddfb-4d9d-8cfc-4c1d0ff19ae2.png"/></disp-formula><p>with</p><disp-formula id="scirp.47490-formula1886"><label>(13)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\ab144af3-e2ea-4039-bf1d-21a81944f561.png"/></disp-formula><p>and</p><disp-formula id="scirp.47490-formula1887"><label>(14)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\b95d28d9-a18f-40fc-a3b0-17cc69a1a069.png"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\9f607e03-6ddf-47b1-ba39-006643082a3c.png" xlink:type="simple"/></inline-formula>are the normalization factor of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\f8017431-2181-47c2-922b-5d5d15cece6c.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\6a6c5ac1-e307-4ffc-a22d-767eb692017e.png" xlink:type="simple"/></inline-formula> BS wave functions, respectively. They can be found from [<xref ref-type="bibr" rid="scirp.47490-ref28">28</xref>] [<xref ref-type="bibr" rid="scirp.47490-ref29">29</xref>] , by only keeping the Dirac structures we take into account here. In the above equations, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\35407210-8ab8-4a53-a870-2dd76c096658.png" xlink:type="simple"/></inline-formula>are defined according to Equation (7) w.r.t.<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\28a16ff8-b5e5-4f8d-a7f0-519c6c0110b7.png" xlink:type="simple"/></inline-formula>, respectively. According to Equation (3),</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\669716fc-09df-495a-a116-5193067a0555.png" xlink:type="simple"/></inline-formula>. So all the variables above are functions of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\8c8332e7-783e-4f62-b2be-d7a1e97ae6fd.png" xlink:type="simple"/></inline-formula>.</p><p>The electromagnetic (U(1)) gauge invariance for this amplitude is explicit. When replacing the four-vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\349d12bf-9334-47ca-b1c3-e85f5b98fd3d.png" xlink:type="simple"/></inline-formula> by the total four-momentum of the virtual photon, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\5cb97116-d8ba-4a2e-8fe2-70f8475d3713.png" xlink:type="simple"/></inline-formula>, the above expression (12) is zero. The reason is</p><disp-formula id="scirp.47490-formula1888"><label>(15)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\dd0009f9-da3a-4267-9662-875a2284cce2.png"/></disp-formula><p>because the totally antisymmetric tensor in <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\c5597a55-f66d-4e6f-9207-2fe36ef06f63.png" xlink:type="simple"/></inline-formula> and totally only three independent 4-vectors in the product.</p><p>The key point in the calculation is the loop integral in Equation (12). In principle it is simple and straightforward, since there is no divergence so that no regularization and renormalization are needed. However, the complexity of the vertex function makes it difficult to employ the formal and conventional Feynman parameter formulations. it will be more difficult if one want to improve precision by employing a more general form of the vertex (more Dirac structures and more complex form of scalar function) rather than the simplified ones employed in this paper. Here we first integrate over the poles of the propagators and then do the numerical integral for the remaining 3-dimensional momentum. This method, though no help to give analytical results but gives a schematic way to do the calculation to obtain the numerical results for much more complex diagrams. As a matter of fact, one of the purposes for this paper is to explore a systematic and practical way to do calculations for production processes within the BS wave function framework, of which the complexity from the loop integrals is quite common.</p><p>Such a method is employed to calculate the high energy scattering amplitude with the help of the flow diagrams, which shows great advantage [<xref ref-type="bibr" rid="scirp.47490-ref30">30</xref>] . The key difference here is that the high energy approximation is not applicable hence not applied. As the consequence, no infrared cutoff caused by the approximation of [<xref ref-type="bibr" rid="scirp.47490-ref30">30</xref>] is needed, so no explicit <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\7a81212a-f0b3-49dc-88f9-5fdd2268be90.png" xlink:type="simple"/></inline-formula> dependence (s is the center of mass energy square) is obtained. As another consequence of not applying the high energy limit, there will be more integral regions of the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\50116f0c-4834-4599-b3da-a8966288100f.png" xlink:type="simple"/></inline-formula> contributing as can be seen in the following.</p><p>We denote the integral in Equation (12) as<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\5769bf7d-da2b-4121-9209-4e2f6b464963.png" xlink:type="simple"/></inline-formula>, and write the momenta in light cone coordinates, i.e. for any four momentum <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\bc6f2887-06f0-412e-ae61-50c9b56706ea.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.47490-formula1889"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\805ca37d-6119-4043-8651-2cc0d1ced293.png"/></disp-formula><disp-formula id="scirp.47490-formula1890"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\805ca37d-6119-4043-8651-2cc0d1ced293.png"/></disp-formula><disp-formula id="scirp.47490-formula1891"><label>(16)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\185c3c37-06c8-436d-b973-b4e268c907ae.png"/></disp-formula><p>Here <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\08f2509c-fb86-4008-9168-3073158fdc6a.png" xlink:type="simple"/></inline-formula> and in the concrete calculations we choose the direction of the 3-momentum of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\094cb58c-e92c-4e23-8342-db9433714dad.png" xlink:type="simple"/></inline-formula> as the z-axis positive direction. So the integral <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\eeaee675-56bc-4716-a229-7503093a1bdb.png" xlink:type="simple"/></inline-formula> can be written as</p><disp-formula id="scirp.47490-formula1892"><label>(17)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\58d68f6c-210d-4182-9169-5f8a74594f66.png"/></disp-formula><p>where</p><disp-formula id="scirp.47490-formula1893"><label>(18)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\d0b581a3-7b00-49f9-ac12-d3ec05d93935.png"/></disp-formula><p>We first integrate <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\e4e09f47-f29d-46f5-a334-ef5e93cf3039.png" xlink:type="simple"/></inline-formula> employing the residue theorem. As <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\d944fafc-90d0-4a71-93de-1d24a4f279f5.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\3353eb50-0e29-4084-984b-9a835c03b53a.png" xlink:type="simple"/></inline-formula>, all poles locate up or under the Real-axis of the complex <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\002d76ea-10b4-4774-a7b1-4c5f99aaa341.png" xlink:type="simple"/></inline-formula> plane, so the integral on <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\05e2ddde-d335-4986-968d-153aa5d4ef97.png" xlink:type="simple"/></inline-formula> is zero. Therefore, the contributing</p><p>integral interval of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\12cbe419-84c4-4b7b-9d9f-ee81db913c96.png" xlink:type="simple"/></inline-formula> should be <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\ec5bca0b-cdfa-47d7-b461-768bc792f647.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\b9a0f912-9486-46c8-bcdc-01e440741a89.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\fa3f6c1d-a20f-46eb-bcaf-3d872def8ebd.png" xlink:type="simple"/></inline-formula> is composed by two parts:</p><disp-formula id="scirp.47490-formula1894"><label>(19)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\9834e435-703b-4a68-b65d-7011d60f743b.png"/></disp-formula><p>Here</p><disp-formula id="scirp.47490-formula1895"><label>(20)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\87825c7d-42ba-4b34-a215-1fc89dfda4c4.png"/></disp-formula><p>with</p><disp-formula id="scirp.47490-formula1896"><label>(21)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\06bb0db1-a258-45ce-955c-e61ff00b1dee.png"/></disp-formula><p>and</p><disp-formula id="scirp.47490-formula1897"><label>(22)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\63f7d536-3cf3-4036-89ea-d15979d2892d.png"/></disp-formula><p>with</p><disp-formula id="scirp.47490-formula1898"><label>(23)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\5b2afe53-cb75-470d-8664-ac3616af3b24.png"/></disp-formula><p>The next step is the numerical integral of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\4245f544-9f8a-498e-b8bf-6be092dc1579.png" xlink:type="simple"/></inline-formula>, and the total cross section is straightforward:</p><disp-formula id="scirp.47490-formula1899"><label>(24)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\3e125872-0a08-4846-9796-24f818d1f626.png"/></disp-formula><disp-formula id="scirp.47490-formula1900"><label>(25)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\334c4512-bbb4-4e01-9b05-bfc2c7f69620.png"/></disp-formula><disp-formula id="scirp.47490-formula1901"><label>(26)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\2cbed1a6-7233-4f93-a65c-7c59430d7f50.png"/></disp-formula><p>The numerical results are listed in <xref ref-type="table" rid="table1">Table 1</xref>.</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\90a62d1c-d700-47a9-b3ae-ca5bfe110a52.png" xlink:type="simple"/></inline-formula>depends on the quark masses and it is around <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\2461ffac-f7d8-422a-bd05-d439cab8f485.png" xlink:type="simple"/></inline-formula> GeV [<xref ref-type="bibr" rid="scirp.47490-ref27">27</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref29">29</xref>] . Here all the quark masses are taken as half of the bound state masses. Since the masses are almost the same for <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\41cc9c86-3b18-46e1-8213-e3b971dacf9c.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\e3c34d61-c365-413a-b38f-5e161263285e.png" xlink:type="simple"/></inline-formula>, so we take the same <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\52b7b1dd-60c2-454f-a7b7-4bb53b990b35.png" xlink:type="simple"/></inline-formula> for them for simplicity. When taking this <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\93d9e505-854e-48f3-a815-a6d8b8d30db0.png" xlink:type="simple"/></inline-formula> value, the cross section is not very large but reaches the same order of magnitude as those in the lowest order NRQCD framework [<xref ref-type="bibr" rid="scirp.47490-ref11">11</xref>] -[<xref ref-type="bibr" rid="scirp.47490-ref13">13</xref>] . One can also observe from the table that though the production cross section is quite sensitive to small <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\fbeb1253-82dd-48fd-b56b-a57f0ca1aa34.png" xlink:type="simple"/></inline-formula> (the cross section should be vanishing for very small<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\5b9c795b-f736-46e1-af71-d1b74af9d44a.png" xlink:type="simple"/></inline-formula>, corresponding to the case of the NR limit), it is steady for large <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\82ffdde0-0fb6-4cdc-a668-1536c019068d.png" xlink:type="simple"/></inline-formula> value. For <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\92adc785-0f2b-45f0-a3e0-c4550d62bd86.png" xlink:type="simple"/></inline-formula> varies from</p><table-wrap id="table1"  position="float"><object-id pub-id-type="pii">Table 1</object-id><label>Table 1</label><caption><p>. The center of mass energy is taken to be 10.58 GeV</p></caption><table><thead><tr><th align="center" valign="middle" ><img src="htmlimages\4-7501703x\5527ccbd-b665-4a5f-a004-d9503cbe3d22.png" width="22.5" height="31.25" /> (GeV)</th><th align="center" valign="middle" ><img src="htmlimages\4-7501703x\8162f0d2-ed9d-474c-a661-a6dd8e51411b.png" width="62.5" height="37.5" /></th></tr></thead><tbody><tr><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></tr><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >0.9</td></tr><tr><td align="center" valign="middle" >1.15</td><td align="center" valign="middle" >1.5</td></tr><tr><td align="center" valign="middle" >1.3</td><td align="center" valign="middle" >6.6</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >5.0</td></tr><tr><td align="center" valign="middle" >1.5</td><td align="center" valign="middle" >1.6</td></tr><tr><td align="center" valign="middle" >1.6</td><td align="center" valign="middle" >2.2</td></tr><tr><td align="center" valign="middle" >1.7</td><td align="center" valign="middle" >3.1</td></tr><tr><td align="center" valign="middle" >1.8</td><td align="center" valign="middle" >4.7</td></tr><tr><td align="center" valign="middle" >1.9</td><td align="center" valign="middle" >8.1</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >12.2</td></tr><tr><td align="center" valign="middle" >2.1</td><td align="center" valign="middle" >74.6</td></tr><tr><td align="center" valign="middle" >2.25</td><td align="center" valign="middle" >8.2</td></tr><tr><td align="center" valign="middle" >2.5</td><td align="center" valign="middle" >1.5</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >0.4</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >0.05</td></tr></tbody></table></table-wrap><p>1 to 1.9, the cross section varies very slowly. It goes up for larger <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\4bf57a6d-29fc-4fc2-9ae2-87ab630e4cdf.png" xlink:type="simple"/></inline-formula> value but then decrease for too large (maybe unphysical) <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\83d41f31-1184-4c67-8a18-4b117803e6bd.png" xlink:type="simple"/></inline-formula>values. As a matter of fact, the decay constants for <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\fe09484a-a42b-4948-a40a-4f9cb4ec4b18.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\ea2981ab-7c34-495b-afb4-3368044f1380.png" xlink:type="simple"/></inline-formula> calculated in the BS framework is also not sensitive to the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\00c77e9a-a4a5-4215-8d90-c9714c9e45a3.png" xlink:type="simple"/></inline-formula> value. So one is even possible to take a larger <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\92e07990-9c09-4c47-b8b2-d2e6c287f1df.png" xlink:type="simple"/></inline-formula> value in calculating the production cross section, say, 2 GeV, to coincide the experimental data at the same time not to change the decay constant much. For this large <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\5581e001-69a0-4afe-ba75-7d2df2e60f69.png" xlink:type="simple"/></inline-formula> value, the half width of the energy fraction distribution of a quark in the rest frame of the quarkonium is about 0.3. There is no direct correspondence of this energy fraction to that in the light cone framework, but it is found that to explain the data, the light cone wave function must have a likely wide distribution. Here we will not sharpen the fact that one can explain the data by the lowest order diagrams considered in <xref ref-type="fig" rid="fig1">Figure 1</xref> by taking a large <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\974d0a0e-e056-4be8-ad30-2dd311260786.png" xlink:type="simple"/></inline-formula> value, but to emphasize the following points:</p><p>1. In the BS framework, when one takes into account the off shell states and large relative movement of the bound quarks, one can get a large contribution to the production cross section from the diagrams of <xref ref-type="fig" rid="fig1">Figure 1</xref>.</p><p>2. To get the best value of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\d53b3b25-ea88-4692-80ac-6478c2785a2c.png" xlink:type="simple"/></inline-formula> so to gain more definite information on the inner movements, it is better to employ more processes to make a global fit. One needs to fit more decay as well as production data. In other words, investigation on various production processes in the BS framework may help to get more precise information for the bound state rather than only consideration on its decay constant.</p></sec><sec id="s4"><title>4. Summary and Discussion</title><p>The BS wave function framework can naturally take into account the off shell states of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\747af742-72b6-4799-b613-720e3e6fdc5f.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\bf7b770e-2679-4bdb-8ba7-7e94f42ff590.png" xlink:type="simple"/></inline-formula> in the bound states, whose effects are ignored a priori in other frameworks. This framework also naturally takes into account the relative movement of the bound quarks at the same time. Our calculations show that the above effects can contribute significantly to the cross section of the production process<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\7944fdac-b3f6-41a8-a409-855df21170c3.png" xlink:type="simple"/></inline-formula>. One can even get the experimental data by adopting a larger value of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-7501703x\ea5a74b6-9b55-4b4c-8bc4-a37c867696cd.png" xlink:type="simple"/></inline-formula>, i.e., wider relative momentum distribution. The calculations are done with the method of direct integration in the momentum space rather than employing the Feynman parameters. Such a systematic method can be applied to more complex production and decay processes for investigation on the inner information of the bound states within the BS framework.</p><p>A question left is how to combine with the calculations in [<xref ref-type="bibr" rid="scirp.47490-ref25">25</xref>] [<xref ref-type="bibr" rid="scirp.47490-ref26">26</xref>] , which could be considered as ‘NNLO’ calculations at HQL of the BS framework. Higher order calculations are straightforward though a little more tedious. But the treating of the propagators and vertices need to be investigated to eliminate double counting. We leave this topic as later works.</p><p>There are two papers employing the diagrams like this paper. In [<xref ref-type="bibr" rid="scirp.47490-ref31">31</xref>] it is a hadronic level calculation. Because the quark states (especially when considering the concept of constituent quark) and the hadron states are not orthogonal to each other [<xref ref-type="bibr" rid="scirp.47490-ref32">32</xref>] , it is more interesting to discuss the possible overlap or relation between these two treatments, which could be helpful in clarifying the physical mechanism underlying the QCD bound states. In [<xref ref-type="bibr" rid="scirp.47490-ref33">33</xref>] , the authors employ the QCD sum rule to do the calculations, but it is not clear whether they take into account the off-shell states in their evaluation on the form factors.</p></sec><sec id="s5"><title>Acknowledgements</title><p>The authors thank Z.-G. Si for discussion. D. Soper and J.-X. Wang is also thanked for comments on the U(1) gauge invariance. This work is partially supported by NSFC, NSF of Shandong Province with Grant Nos. 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