<?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.2014.59089</article-id><article-id pub-id-type="publisher-id">JMP-47115</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>Emission of Thermal Photon in Heavy-Ion Collisions</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Poonam</surname><given-names>Jain</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>Yogesh</surname><given-names>Kumar</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>Deepak</surname><given-names>Kumar</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Department of Physics, Shyam Lal College, University of Delhi, New Delhi, India</addr-line></aff><aff id="aff1"><addr-line>Department of Physics, Sri Aurobindo College, University of Delhi, New Delhi, India</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>poonam.jn1@gmail.com(PJ)</email>;<email>yogesh.du81@gmail.com(YK)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>19</day><month>06</month><year>2014</year></pub-date><volume>05</volume><issue>09</issue><fpage>792</fpage><lpage>799</lpage><history><date date-type="received"><day>1</day>	<month>April</month>	<year>2014</year></date><date date-type="rev-recd"><day>3</day>	<month>May</month>	<year>2014</year>	</date><date date-type="accepted"><day>1</day>	<month>June</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>
	We study
the leading order processes for photon production using a phenomenological
model of quark-gluon plasma (QGP) in relativistic heavy-ion collisions
incorporating the parametrization factors in thermal dependent quark mass. The
measurement of photon emission provides valuable insights into the early
conditions of QGP. The production rate is observed in the low and intermediate
range of energy and transverse momentum. The photon yield is found to increase
marginally with the effect of thermal dependent quark mass. The results are
little enhanced and in good agreement with other work. 
</p></abstract><kwd-group><kwd>Photons</kwd><kwd> Quark-Gluon Plasma</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Many interesting outcomes have been observed at RHIC and LHC where a hot and dense matter is expected to be created. From low to high energy experiments, extensive effort have been made to probe the properties of the quark-gluon plasma (QGP), which has become a new worth of quantum cromo-dynamics (QCD) matter in the study of relativistic heavy-ion collisions [<xref ref-type="bibr" rid="scirp.47115-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref29">29</xref>] . First possibility for the discovery of the QGP in these ex- periments have been reported [<xref ref-type="bibr" rid="scirp.47115-ref30">30</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref32">32</xref>] . Photons and leptons are electromagnetic probes which are created during the evolution of a nuclear collision. In heavy-ion collisions, photons are taken as good messenger to in- vestigate properties of the matter since they leave the medium without a strong interaction once they are pro- duced.</p><p>The study of photon is especially interesting because they emit in the course of a heavy-ion reaction which is considered as a good observable for the space-time evolution of the colliding system. The photons are emitted from every stage of the collisions, and their transverse momentum are characterized by their origins. Especially, the low and intermediate transverse momentum region is considered as a suitable window for measuring the medium-induced direct photons. The high-energy photons are sensitive observables to the dynamics of the deconfined phase. Since long, Shuryak proposed photons as a promising direct probe [<xref ref-type="bibr" rid="scirp.47115-ref33">33</xref>] and other groups con- tinue to be actively investigated [<xref ref-type="bibr" rid="scirp.47115-ref34">34</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref53">53</xref>] . Unfortunately, most of the photons measured in heavy-ion collisions come from hadronic decays. The experimental challenge of obtaining spectra of direct photons has been gone through by several experiments; WA98 at SPS/CERN [<xref ref-type="bibr" rid="scirp.47115-ref54">54</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref56">56</xref>] and PHENIX at RHIC/BNL [<xref ref-type="bibr" rid="scirp.47115-ref57">57</xref>] [<xref ref-type="bibr" rid="scirp.47115-ref58">58</xref>] to analyze the explicit data points for direct photons and provided the most interesting results. Hence, electromagnetic probes are considered to be ideal probes for the detection and study of subsequent evolution of QGP.</p><p>The earlier observations of photon production from quark-gluon plasma at finite temperature have been performed in Ref. [<xref ref-type="bibr" rid="scirp.47115-ref59">59</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref63">63</xref>] . In 1-loop approximation, the photon emission rate from annihilation and Compton processes has been calculated by Ref. [<xref ref-type="bibr" rid="scirp.47115-ref3">3</xref>] . Further, Aurenche et al. [<xref ref-type="bibr" rid="scirp.47115-ref64">64</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref66">66</xref>] has shown photon production rate in the QGP upto 2-loop level and found that emission rate are considerably same size or larger than the earlier lowest order results. A new annihilation with scattering (aws), higher order process was found to dominate the photon production rate from quark matter at high photon energies. With these informations, we focus on the measurement of photon emission which provide a good opportunity to study the early evolution of fireball.</p><p>In this work, we use the thermal mass formalism and the corresponding thermal Hamiltonian in the literature leading to the following choice for the confining/de-confining potential [<xref ref-type="bibr" rid="scirp.47115-ref67">67</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref69">69</xref>] . The phenomenological model is used as quasiparticle in which mass is dependent on temperature and parametrization factors [<xref ref-type="bibr" rid="scirp.47115-ref70">70</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref72">72</xref>] . This effective mass generated due to thermal interactions between quarks and gluons and shows well behaviour above and around critical temperature. The “Thermal-Hamiltonian” for the QGP is given as:</p><disp-formula id="scirp.47115-formula1678"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\bfe99bcb-f6de-458e-9a64-414f4a98e38d.png"/></disp-formula><p>The above result is taken in the large <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\c0ac3c3d-a2f4-461b-b943-7abe731c4c9b.png" xlink:type="simple"/></inline-formula> limit or expressed as,</p><disp-formula id="scirp.47115-formula1679"><label>(1)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\3b25cb53-57c4-462f-8c20-9eaa27ee7e3e.png"/></disp-formula><p>where,</p><disp-formula id="scirp.47115-formula1680"><label>(2)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\7d1cac50-3d18-4e33-825f-e1b20f5e61d9.png"/></disp-formula><p>with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\cab723b2-9b08-4c08-8566-4d95bcb96673.png" xlink:type="simple"/></inline-formula> is the quarks (gluons) momentum, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\ce115d66-9a37-4a2c-914e-27e0f8d22347.png" xlink:type="simple"/></inline-formula>is the rest mass of the quark, T is the temperature and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\cc8aa19d-d184-4371-9e49-878de03ef7e4.png" xlink:type="simple"/></inline-formula></p><p>is first order QCD running coupling constant. <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\68426a60-4e1c-4cbd-baff-88111fbcd6e8.png" xlink:type="simple"/></inline-formula>is the phenomenological parameter used to take care the</p><p>hydrodynamical aspects of the hot QGP droplet. We fix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\513ff3e5-85ed-42e7-bdf6-24d89e08bbde.png" xlink:type="simple"/></inline-formula> or <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\a80041af-1ec4-4d8b-a9dc-9637bed2dded.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\b271bb02-3751-4e2c-9dbd-5c26e4372f4c.png" xlink:type="simple"/></inline-formula>. All parameter values are taken by Ref. [<xref ref-type="bibr" rid="scirp.47115-ref73">73</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref75">75</xref>] in our calculation,</p><disp-formula id="scirp.47115-formula1681"><label>(3)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\e45fc372-0151-4233-bd7c-f3b363f815be.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\83ce6809-5b35-4d61-945a-91aad2868fc2.png" xlink:type="simple"/></inline-formula> is the QCD scale taken to be 150 MeV, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\abea9cc6-9739-4114-9dac-8cce3b7d4763.png" xlink:type="simple"/></inline-formula>is the number of flavor. Finally, we obtain the finite quark mass defined as [<xref ref-type="bibr" rid="scirp.47115-ref73">73</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref75">75</xref>] :</p><disp-formula id="scirp.47115-formula1682"><label>(4)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\4d2e3892-5dd1-4112-bd6c-915c06844aa3.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\379f372f-9b82-44ce-9da2-334c0e83f230.png" xlink:type="simple"/></inline-formula> known as minimum momentum cut off with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\56832d06-3010-4320-8067-18f84a5d8cad.png" xlink:type="simple"/></inline-formula> and flow parameter</p><p>is taken as<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\67923413-558d-4b61-b66c-6830c7b58f3b.png" xlink:type="simple"/></inline-formula>. The finite value of quark mass also removes the infrared divergence produced in</p><p>photons production [<xref ref-type="bibr" rid="scirp.47115-ref76">76</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref78">78</xref>] . We compute the thermal photon emission from quark-gluon plasma of complete</p><p>leading order (LO) results at temperatures <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\a651276f-6045-4c19-b2ec-fe4aefc8358b.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\23fbdf7f-dd6d-4307-8b57-402eabb5fd20.png" xlink:type="simple"/></inline-formula> with parametrization factor for</p><p>flavor 2 and 3 and compare the results with other work.</p><p>The paper is organized as follows. In Section 2 we outline the LO processes for photon spectra in QGP. Results are presented in Section 3. Finally in Section 4 we give the conclusion.</p></sec><sec id="s2"><title>2. Emission of Thermal Photon from QGP</title><p>Various theoretical predictions have been proved, some of the surprises have been found in experimental results and indicate that RHIC and LHC is, indeed, probing a new development in the field of high energy physics. One loop and two loop order for complete calculation of photon production rate from QGP to order <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\d35dfb11-addb-4da8-a314-4ce4f96da9f4.png" xlink:type="simple"/></inline-formula> have been considered in the Ref. [<xref ref-type="bibr" rid="scirp.47115-ref59">59</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref61">61</xref>] [<xref ref-type="bibr" rid="scirp.47115-ref64">64</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref66">66</xref>] [<xref ref-type="bibr" rid="scirp.47115-ref79">79</xref>] [<xref ref-type="bibr" rid="scirp.47115-ref80">80</xref>] . The relevant LO processes include different channels. For the present calculation, we use the parametrization of the rate given in Ref. [<xref ref-type="bibr" rid="scirp.47115-ref80">80</xref>] .</p><p>The rate for photons of momentum <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\9466d18f-eaaf-44e6-8f66-7e1e21d7735c.png" xlink:type="simple"/></inline-formula> is given by the expression [<xref ref-type="bibr" rid="scirp.47115-ref80">80</xref>] [<xref ref-type="bibr" rid="scirp.47115-ref81">81</xref>]</p><disp-formula id="scirp.47115-formula1683"><label>(5)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\d2e63a09-dbec-439a-a284-0b3bab526909.png"/></disp-formula><p>with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\3fe0a518-cf9a-49a9-b72f-eb57ae7416ab.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\f994357d-344e-4c7c-a205-a05e81a4b096.png" xlink:type="simple"/></inline-formula> is the leading order large momentum limit of the thermal quark mass. The leading-</p><p>log coefficient <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\2d5b06ee-de9b-4944-bf7f-5c7128a027fd.png" xlink:type="simple"/></inline-formula> is given as</p><disp-formula id="scirp.47115-formula1684"><label>(6)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\4de39b6a-47a2-4fe9-adbd-34ecdeff6358.png"/></disp-formula><p>The summation is over the number of quark flavors and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\17a4f44c-542e-4e8b-9774-6e918bd0a99f.png" xlink:type="simple"/></inline-formula> is their electric charge, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\584a9411-bd57-4e42-9d2d-78bacef000fe.png" xlink:type="simple"/></inline-formula>is the electromag-</p><p>netic constant and mass of quark are taken by Ref. [<xref ref-type="bibr" rid="scirp.47115-ref73">73</xref>] -[<xref ref-type="bibr" rid="scirp.47115-ref75">75</xref>] . <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\d63a6458-3171-4f2d-b3e8-a3c2ddca9da2.png" xlink:type="simple"/></inline-formula>is the fermi distribution function. The</p><p>dependence on the specific photon production process is written in the term<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\fc3af655-d85e-40c3-94e7-6cc2b45c3f80.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.47115-formula1685"><label>(7)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\df1bff32-26fb-40c6-8a2a-8e93ae83522d.png"/></disp-formula><p>The non-logarithmic two-to-two contribution <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\d744e129-6e08-4316-ab57-7bc105493c2b.png" xlink:type="simple"/></inline-formula> for general E/T and the rate of photon production by</p><p>bremsstrahlung and annihilation with scattering are computed. This requires solving a non-trivial integral equation to determine this rate. The thermal corrections to the dispersion relations for incoming or outgoing</p><p>particles can no longer be neglected in these <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\c1a45d93-3aed-4b7c-9337-0ca6543ac26c.png" xlink:type="simple"/></inline-formula> processes. The <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\54041bcf-7e25-4b26-8efb-2c72d0df1fca.png" xlink:type="simple"/></inline-formula> is the non-trivial function that</p><p>can only be solved numerically. All results for <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\2802eddd-acdf-4fe0-9991-183b82e57189.png" xlink:type="simple"/></inline-formula> are evaluated by Ref. [<xref ref-type="bibr" rid="scirp.47115-ref80">80</xref>] [<xref ref-type="bibr" rid="scirp.47115-ref81">81</xref>] .</p><p>Then we study the total photon spectrum above critical temperature by integrating the total rate over the space-time history of the collision for all the LO processes after getting the temperature of the evolution from the model. We integrate rates at preferential temperatures, which are considered as temperature of transition to be completely hot phase. It is expressed as [<xref ref-type="bibr" rid="scirp.47115-ref75">75</xref>] [<xref ref-type="bibr" rid="scirp.47115-ref81">81</xref>] :</p><disp-formula id="scirp.47115-formula1686"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\e27a89f1-89d2-4a83-96da-aaa5c3297d7f.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\b2fad58e-57a3-4354-8a31-532b4d3fd01f.png" xlink:type="simple"/></inline-formula> is time evolution determined with the temperature from initial to final state with the rapidity <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\0a7ea779-613f-4cf7-b95d-b46c6066fe5f.png" xlink:type="simple"/></inline-formula> corresponding to RHIC energy. <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\506dfa09-d2fe-44fd-b356-1e2361598501.png" xlink:type="simple"/></inline-formula>is transverse cross section and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\73f94228-f9e4-44e6-86cf-ba6c563979fa.png" xlink:type="simple"/></inline-formula> is the photon transverse momentum. The quantity on the extreme R.H.S. is defined in the centre-of-mass system with the</p><p>photon energy<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\1b6070af-451b-4200-b158-3ede148fc10e.png" xlink:type="simple"/></inline-formula>. Thus, with the values of rapidity and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\386fda2a-0b1f-4576-ad81-033d74e236c9.png" xlink:type="simple"/></inline-formula>, we get the total photon spec-</p><p>trum of LO processes.</p></sec><sec id="s3"><title>3. Results</title><p>The results are important concerning photon production as a signature for the creation of a quark-gluon plasma. We perform the calculation of LO processes for photon emission in the QGP which consist QCD Compton Scattering, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\c17ef693-8eab-4b5f-a6bb-f0c9c79b2e61.png" xlink:type="simple"/></inline-formula>annihilation, Bremsstrahlung (brems), and annihilation with scattering (aws) with suitable choice of parametrization factors in the quark mass at hot phase of QGP evolution with temperature <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\bd1a4820-6e85-4e16-a358-349a868f55f8.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\9dee4a0b-1626-44a0-85e7-8f223b8dec68.png" xlink:type="simple"/></inline-formula> for flavor <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\3abb5f02-6a19-48a0-b0c3-c130514c923a.png" xlink:type="simple"/></inline-formula> and 3.</p><p>In <xref ref-type="fig" rid="fig1">Figure 1</xref>, we plot LO processes for photon emission rate at fixed temperature <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\2e294e77-abe0-4f25-9ebc-f9bf8c912efe.png" xlink:type="simple"/></inline-formula> for flavor <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\9cd15988-83e2-466b-90b6-5ce82016c339.png" xlink:type="simple"/></inline-formula> and 3 with the effect of finite value of quark mass with the variation of the photon energy. At closer inspection, it turns out that the model calculation in the relevant range give the significant contribution and dominate over the results of Renk et al. [<xref ref-type="bibr" rid="scirp.47115-ref81">81</xref>] . The results show visible increment at temperature <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\57f3872e-899a-4ad0-8637-7993d725eb88.png" xlink:type="simple"/></inline-formula> of the QGP fireball for flavor<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\c3bfa3c9-10df-4db6-afcf-26ae68509232.png" xlink:type="simple"/></inline-formula>. We also show the result for flavor 3 and found that the strength of photon emission is enhanced for the large flavor numbers. The larger number of anticipating quarks bring more interactions, resulting in the enhancement of production rate. So with introducing the strange mass, photon emis- sion increases. The increase in the emission rate is highly effected by temperature of the system, and it seems to be large near creation of quark matter that is considered to be exist at very hot temperature. We compare the outputs between our result and the standard result of Ref. [<xref ref-type="bibr" rid="scirp.47115-ref81">81</xref>] . Our results has visible incremental amount in LO production rate over the result of Ref. [<xref ref-type="bibr" rid="scirp.47115-ref81">81</xref>] .</p><p>Now, we study the total photon spectrum over the space-time evolution of QGP. The results are shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>. With the similar line of parameters, we show total emission rate as a function of transverse mo- mentum at temperature <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\48981355-015c-41f0-aadc-f00e2c8ff059.png" xlink:type="simple"/></inline-formula> and compare the results produced by Ref. [<xref ref-type="bibr" rid="scirp.47115-ref81">81</xref>] . In the yield rate of two different quark flavors, the higher value of quark flavor <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\333f37a0-b68c-4a48-97c5-c86d4039a09c.png" xlink:type="simple"/></inline-formula> has larger yield than lower value. It is due to the more interaction among the large number of constituent quarks. In the comparison, we find that the photon spectra of our model for quark flavor <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\bcc6d075-50ec-4b0f-a551-e34ee04a600a.png" xlink:type="simple"/></inline-formula> has visible improvement, indeed, enhacement over theoretical result of Ref. [<xref ref-type="bibr" rid="scirp.47115-ref81">81</xref>] . Thus, the consideration of thermal dependent quark mass has an important role in LO processes for photon measurements and does not invalidate the results of high energy heavy-ion collisions. This simple phenomenological model shows little improved result over the results of Ref. [<xref ref-type="bibr" rid="scirp.47115-ref81">81</xref>] . The figure also shows that production rate as function of transverse momentum have much enhancement over the production rate as function of photon energy.</p></sec><sec id="s4"><title>4. Conclusion</title><p>The measurement of leading order processes for photon production in the QGP which consist QCD Compton Scattering, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\9666413f-e32f-456a-abe2-c72f7e48e81b.png" xlink:type="simple"/></inline-formula>annihilation, Bremsstrahlung, and annihilation with scattering provides a good opportunity to study the evolution of fireball in high-energy heavy-ion collisions. We have used the leading order photon</p><fig id="fig1"><label>Figure 1</label><caption><p> The photon spectra at thermal temperature <img src="htmlimages\7-7501842x\ea4b8c99-3d0c-4c96-a7a5-7d74b20e640e.png" width="133.75" height="28.75" /> for <img src="htmlimages\7-7501842x\81909d21-dd21-472a-86b6-17e7469e3b54.png" width="63.75" height="37.5" /> and 3 and compared with other work</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\911c0ddc-de61-41a1-b8bc-e3b1db0dbc1f.png"/></fig><fig id="fig2"><label>Figure 2</label><caption><p> The total photon rate at thermal temperature <img src="htmlimages\7-7501842x\70a0d768-abc8-4eb5-b702-e785c5edb18f.png" width="133.75" height="28.75" /> for <img src="htmlimages\7-7501842x\3178ecb2-3420-4568-bce0-c0a5f7a5d5dd.png" width="63.75" height="37.5" /> and 3 and compared with other work</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\7-7501842x\05325ed8-b44c-4597-8edc-3b49ab6eb76d.png"/></fig><p>emission rate from QGP, along with the estimates of the impact of our phenomenological model on this rate, in a simple model for the fireball evolution to calculate the resulting photon spectrum. The work on LO processes for thermal photons have discussed within a model with various sets of initial condition. This implies that the consideration of thermal dependent quark mass has important role in the photon measurements of the high- energy heavy-ion collisions. The QGP fireball with the model of parametrization factor give a significant contribution and improved the calculation of photon radiation for 2 and 3 flavor in high-energy heavy-ion col- lisions.</p></sec><sec id="s5"><title>Acknowledgements</title><p>We thank V. Kumar for suggestions and discussions in preparing the manuscript.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.47115-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">HUNG, C.M. AND SHURYAK, E. (1998) PHYSICS REVIEW C, 57, 1891. 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