# In-medium viscous coefficients of a hot hadronic gas mixture

**Authors:** Utsab Gangopadhyaya, Snigdha Ghosh, Sukanya Mitra, Sourav Sarkar

arXiv: 1703.03584 · 2017-03-13

## TL;DR

This paper calculates the shear and bulk viscosities of a hot hadronic gas mixture of pions and nucleons using in-medium scattering amplitudes, revealing significant temperature and density effects.

## Contribution

It introduces in-medium scattering amplitudes into the kinetic theory calculation of viscosities, improving upon vacuum cross-section assumptions.

## Key findings

- In-medium cross-sections are suppressed at finite temperature and density.
- Viscosity coefficients show strong dependence on temperature and baryon chemical potential.
- In-medium effects significantly alter the transport properties of the hadronic gas.

## Abstract

We estimate the shear and the bulk viscous coefficients for a hot hadronic gas mixture constituting of pions and nucleons. The viscosities are evaluated in the relativistic kinetic theory approach by solving the transport equation in the relaxation time approximation for binary collisions ($\pi\pi$,$\pi N$ and $NN$). Instead of vacuum cross-sections usually used in the literature we employ in-medium scattering amplitudes in the estimation of the relaxation times. The modified cross-sections for $\pi\pi$ and $\pi N$ scattering are obtained using one-loop modified thermal propagators for $\rho$, $\sigma$ and $\Delta$ in the scattering amplitudes which are calculated using effective interactions. The resulting suppression of the cross sections at finite temperature and baryon density is observed to significantly affect the $T$ and $\mu_N$ dependence of the viscosities of the system.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1703.03584/full.md

## References

51 references — full list in the complete paper: https://tomesphere.com/paper/1703.03584/full.md

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Source: https://tomesphere.com/paper/1703.03584