27–29 Jul 2022
Europe/Zurich timezone

Charge and heat transport in hot quark matter with chiral dependent quark masses

Not scheduled
2h
Poster presentation Poster session

Speaker

Ms Pushpa Panday (Indian Institute of Technology Roorkee)

Description

As the strength of the magnetic field ($B$) becomes weak, novel phenomena,
similar to the Hall effect in condensed matter physics
emerges both in charge and heat transport in a thermal
QCD medium with a finite quark chemical potential ($\mu$).
So we have calculated the transport coefficients
in a kinetic theory within a quasiparticle framework,
wherein we compute the effective mass of quarks for the
aforesaid medium in a weak magnetic field (B) limit
($|eB|< QCD up to one loop, which depends on $T$ and $B$ differently to
left- (L) and right-handed (R) chiral modes of quarks, lifting
the prevalent degeneracy in L and R modes in a strong magnetic field
limit ($|eB|>>T^2$). Another implication of weak
$B$ is that the transport coefficients assume a tensorial structure:
The diagonal elements represent the usual (electrical and thermal)
conductivities: $\sigma_{\rm Ohmic}$ and $\kappa_0$ as the
coefficients of charge and heat transport, respectively
and the off-diagonal elements denote their Hall counterparts:
$\sigma_{\rm Hall}$ and $\kappa_1$, respectively.
It is found in charge transport that the magnetic field acts on
L- and R-modes of the Ohmic-part of electrical conductivity in
opposite manner, viz. $\sigma_{\rm Ohmic}$ for L- mode decreases
and for R- mode increases with $B$ whereas the Hall-part $\sigma_{\rm Hall}$
for both L- and R-modes always increases with $B$.
In heat transport too, the effect of the magnetic field on the usual thermal
conductivity ($\kappa_0$) and Hall-type coefficient ($\kappa_1$) in both
modes are identical to the abovementioned effect of $B$ on charge
transport coefficients.

We have then derived some coefficients from the above transport
coefficients, namely Knudsen number ($\Omega$ is the ratio of
the mean free path to the length scale of the system)
and Lorenz number in Wiedemann-Franz law. The effect of $B$ on $\Omega$
either with $\kappa_0$ or with $\kappa_1$ for both modes are identical to
the behavior of $\kappa_0$ and $\kappa_1$ with $B$. The value of
$\Omega$ is always less than unity for the entire temperature range,
validating our calculations. Lorenz number ($\kappa_0/\sigma_{{\text{Ohmic}}}T$) and
Hall-Lorenz number ($\kappa_1/\sigma_{{\text{Hall}}}T$) for L-mode
decreases and for R-mode increases with a magnetic
field. It also does not remain constant with T, except for
the R-mode Hall-Lorenz number where it remains almost constant
for smaller values of B.

Primary author

Ms Pushpa Panday (Indian Institute of Technology Roorkee)

Co-author

Prof. Binoy Krishna Patra (Indian Institute of Technology Roorkee)

Presentation materials