We calculate the spectral function in pseudoscalar (scalar) channel in the high temperature phase of QCD in presence of a background magnetic field. Spatial and temporal screening masses are determined from the long distance behavior of the corresponding correlation functions.
Contents1 Formalism 3 2 Spectral Function 5 3 Screening masses 8 4 Outlook 11 A Imaginary part of one loop self energy 11 B Evaluation of T intergrals 12Under extreme conditions of temperature and baryon density, strongly interacting matter of quantum chromodynamics (QCD) liberates a large number of degrees of freedom indicating a phase transition to a deconfined, quasi-ideal state known as quark gluon plasma (QGP) [1]. There is an overall consensus that heavy ion collision experiments have shown us glimpses of such a state of matter. It is known for sometime that ultra-relativistic motion of charged particles create an intense magnetic field in the early stage of non-central heavy ion collision. The energy scale of the magnetic field thus generated is comparable with the characteristic scale of QCD, for example, B ∼ m 2 π /e at RHIC and could be as high as B ∼ 10m 2 π /e at LHC [2][3][4][5][6]. Here m π is pion mass in vacuum and e is charge of proton. An external magnetic field modifies the QCD vacuum and entails a rich spectrum of phenomena -chiral magnetic effect (CME) [2, 7-9], chiral vortical effect (CVE), magnetic catalysis, modification of the phase diagram [10-12] and so on. There are tremendous amount of activities, both theoretical and experimental, going on to understand the properties of QCD matter under an external magnetic field [13]. Apart from QCD, effects induced by an external magnetic field is important in astrophysics [14], cosmology [15], physics beyond standard model [16], or condensed matter physics [17].Hadronic correlation functions are useful objects to understand the intricate dynamics of QCD [18][19][20]. Spectral densities of correlation functions encode information of inmedium hadron properties, transport coefficients and electromagnetic emissivity from the hot and dense plasma. Mesonic spectral functions at finite temperature have been calculated in the literature using analytic methods [21][22][23][24][25] or numerical simulations of lattice QCD [26][27][28][29]. Hadronic correlators in a background magnetic field have also been studied in different settings, see [30][31][32][33][34][35][36][37][38] for latest development in the field.The purport of the present paper is to discuss the modification of mesonic spectral densities in the high temperature deconfined phase of QCD. We shall work to O α 0 s in the strong coupling constant albeit the effect of magnetic field, by construction, is included to all orders. Neglect of QCD radiative corrections provides a clean benchmark