Virtual Photon Emission from QuarkGluon Plasma
Abstract
We recently proposed an empirical approach for the LandauPomeranchukMigdal (LPM) effects in photon emission from the quark gluon plasma as a function of photon mass. This approach was based on Generalized Emission Functions (GEF) for photon emission, derived at a fixed temperature and strong coupling constant. In the present work, we have extended the LPM calculations for several temperatures and strong coupling strengths. The integral equations for () and () are solved by the iterations method for the variable set {}, considering bremsstrahlung and processes. We generalize the dynamical scaling variables, , , for bremsstrahlung and aws processes which are now functions of variables . The GEF introduced earlier, , , , , are also generalized for any temperatures and coupling strengths. From this, the imaginary part of the photon polarization tensor as a function of photon mass and energy can be calculated as a one dimensional integral over these GEF and parton distribution functions in the plasma. However, for phenomenological studies of experimental data, one needs a simple empirical formula without involving parton momentum integrations. Therefore, we present a phenomenological formula for imaginary photon polarization tensor as a function of {} that includes bremsstrahlung and mechanisms along with LPM effects.
pacs:
12.38.Mh ,13.85.Qk , 25.75.q , 24.85.+pIn this work, we present a study of LandauPomeranchukMigdal effects (1); (2) (LPM) in virtual photon emission from thermalized quark gluon plasma (QGP). The LPM effects on real photon emission from QGP have been reported (3); (4) and an empirical approach in (5). For the case of virtual photon emission in QGP, the processes that contribute at order (6) and the higher order corrections (7) and LPM effects (8) were well studied. In hard thermal loops (HTL) (9) method these processes occur at the one loop, two lop and higher loop levels represented by ladder diagrams. In the photon emission calculations, the quantity of interest is the the imaginary part of photon retarded polarization tensor (). The dilepton emission rates are estimated in terms of this , BoseEinstein factor and as given by Eq.1. The including LPM effects is determined in terms of a transverse function and a longitudinal part , as given by Eq.2 (8).
For the case of virtual photon emission having small virtuality, the transverse vector function is determined by the AMY equation (Eq.3) and the longitudinal function by AGMZ equation (Eq.4) (8). The energy transfer function is given in Eq.5. The tilde represents quantities in units of Debye mass, for details see (10).
(1)  
(2)  
(3)  
(4)  
(5) 
I Generalized Emission Functions for photon emission
In the present work, we solved these Eqs.(3,4) by iterations method at a fixed photon energy of /T=50. Alternatively, these equations can also be solved by variational approach (11). In the following calculations, we have used two flavors and three colors. Using the iterations method, we obtained distributions for different , plasma temperatures (T=1.0, 0.50, 0.25GeV) and strong coupling constants (=0.30, 0.10, 0.05). We integrate these distributions to derive as defined in the Eqs.6,7. The superscripts in these equations represent bremsstrahlung or processes depending on the value used. The subscripts represent contributions from transverse () or longitudinal parts. are the quantities required for calculating imaginary part of polarization tensor (see Eq.2). Therefore, in the following, we empiricize these .
(6)  
(7)  
(8)  
(9)  
(10)  
(11)  
(12)  
(13) 
In the remaining part of this work, we adopt the formulae and results of (10) presented at fixed T=1GeV, , by suitably redefining the quantities for all temperatures and strong coupling constants. In Eqs.8,9,10 we define four dimensionless variables. The factor in above equations is required to match the definitions in present work with those of (10). The variable is the real photon dynamical variable (5). For virtual photon emission from QGP, we define two more variables, given in Eqs.11,12. are in general functions of {} and when plotted versus any of these , they do not exhibit any simple trends. Following (10), we define the generalized emission functions (GEF) in Eq.13. The GEF are functions of only variables. These GEF () are obtained from corresponding values by multiplying with coefficient functions given in Eqs.1418. The variable in Eqs.1923 is for transverse part and for longitudinal parts. The quantities and in Eqs.1118 are found by search for dynamical variables hidden in the solutions of AMY and AGMZ equations.
(14)  
(15)  
(16)  
(17)  
(18) 
(19)  
(20)  
(21)  
(22)  
(23)  
Figure 1 shows the results for GEF for bremsstrahlung (Fig.1(a)).
The calculations are for a fixed photon energy (/T=50.)
but include six different cases of temperatures and coupling strengths mentioned
in figure labels. The solid curve in (a) is the empirical fit to this emission function, given by Eq.19
The emission function for high Q values () for transverse part of process is shown in Figure 2.
The and the emission function are given in Eqs.15,20. Similarly, Figures (3(a,b)
show the longitudinal components of GEF for bremsstrahlung (Fig.(a)) and (Fig.(b)).
The coeffiicient functions and GEF are given in Eqs.17,22,18,23.
These transformation functions are very complex.
Ii GEF and photon retarded polarization tensor
In the previous section, we used the results from the iterations methods to obtain the values by integrating the distributions. We transformed these into GEF () functions shown in Figs.13. We fitted these by empirical functions given in Eqs.1923. Using the empirical functions, for any values, we can generate the values, circumventing the need to solve the integral equations. Thus, we have empiricized the values in terms of GEF. Hence, using GEF and the , the imaginary part of photon retarded polarization tensor () is calculated, as in Eq.24 (10).
(24)  
Here, the superscript denotes depending on the value of the integration variable .
(25)  
(26)  
(27) 
We will present more results in a different way by defining reduced quantities. After obtaining the versus by using Eq.25, we define the reduced polarization tensor as and reduced Q as in Eqs.26,27. The reduced polarization tensors are calculated for different photon energies, different coupling strengths and temperatures. We plotted these results in balck circles in Figs.5,6 versus . For comparison, results from (12) are shown in red symbols. The agreement of these two symbols is seen to be very good from low to very high photon energies, .
Iii Phenomenology using Generalized Emission Functions
In this section, we obtain the phenomenological fits to virtual photon emission rates from QGP. From the Figures 5,6, it is clear that the reduced quantities depend on only two variables, i.e., instead of {}, we need only {} to generate as in Eq.28. This observation was already reported in (8).
(28) 
In the limit of , ). To study this further, we use Eq.25 to generate imaginary part of polarization tensor for various values of . At first, we generate the at a very low , , for various values of . Using the results, we construct . The results are shown in Figure 7 by symbols labeled GEF method. The results for different merge into a single curve in Fig.7. We fitted this data by suitable functions as given in Eqs.31 along with their parameters. These are two different fits, one for 200 and the other for 100, with an overlap between 100200. These are represented by solid curves and labeled in figure. The below is approximately equal to this function , as given by Eq.29. However, it should be noted that at ultra soft photon energies, the present formalism needs corrections (13).
For the case of finite , we made empirical fits by choosing a function given in Eq.30. In this function, A,B,C
parameters are function of and are determined by fitting the plots for various .
These parameters values for various are tabulated and are shown in Figure 8.
It is very important to have an empirical formula to generate A,B,C values.
Therefore, these A,C,B parameters were fitted by different functional forms
as given in Eqs.33,36,38. The parameters are different for different
regions. Therefore, depending on the requirement, one can select the relevant parameter set to generate A,B,C values.
(29)  
(30) 
(31)  
(32)  
(33)  
(34)  
(35) 
(36)  
(37)  
(38)  
(39)  
(40)  
In conclusion, the photon emission rates from the quark gluon plasma have been
studied as a function of photon mass, considering LPM effects at various temperatures and strong coupling strengths.
We defined generalized dynamical variables for transverse and longitudinal components of bremsstrahlung
and mechanism. In addition, we defined generalized emission functions (GEF)
namely ,,,.
We have obatined empirical fits to these GEF.
In terms of the GEF, we have calculated the imaginary part of retarded photon polarization tensor as a
function of photon energy and mass, plasma temperature and strong coupling strengths.
For phenomenological applications,
we fitted the reduced imaginary polarization tensor by simple functions and provided necessary parameters.
Acknowledgements.
I am thankful to my wife S.V. Ramalakshmi for cooperation during this work.Footnotes
 This fit given in Eq.19 is an improvement over the result reported in (10).
 The Eqs.18,23 are slightly different from the corresponding equations presented in (10).
 The factor T in (Tm in the Eq. 24 is arising from the tilde transformation. This extra T cancels the factor coming from tilde transformation of functions. This T was missing in (10).
 It should be noted that the functional forms having difference of power law for these fits demand high precision of their parameters. Therefore, one should not truncate these parameters, especially the power exponents given by .
References
 L.D. Landau, I.Ya. Pomeranchuk, Dokl. Akad. Nauk. SSR 92, 535 (1953) ; ibid. SSR 92, 735 (1953).
 A.B. Migdal, Phys. Rev. 103, 1811 (1956).
 Peter Arnold, Guy D. Moore and Laurence G. Yaffe, JHEP 11 (2001) 057, [hepph/0109064].
 Peter Arnold, Guy D. Moore and Laurence G. Yaffe, JHEP 12 (2001) 009, [hepph/0111107]
 S. V. S. Sastry, Phys. Rev. C67, 041901(R) (2003), [hepph/0211075] ; [hepph/0208103]
 T. Altherr, P.V. Ruuskanen, Nucl. Phys. B380, 377 (1992).
 M.H. Thoma, C.T. Traxler, Phys. Rev. D56, 198 (1997), [hepph/09701354]
 P. Aurenche, F. Gelis, Guy D. Moore and H. Zaraket, JHEP 12 (2002) 006, [hepph/0211036].
 E. Braaten, R.D. Pisarski, Nucl. Phys. B337, 569 (1990).
 S.V. Suryanarayana, Phys. Rev. C75,021902(R) (2007),[hepph/0606056]
 S.V. Suryanarayana, hepph/0609096, work in progress.

F. Gelis, libLPMv1,
http://wwwspht.cea.fr/articles/T02/150/libLPM/  Guy D. Moore and JeanMarie Robert, arXiv:hepph/0607172.