Abstract
We have studied the effects of weak magnetic field and finite chemical potential on the transport of charge and heat in hot QCD matter by estimating their respective response functions, viz. the electrical conductivity (\(\sigma _{\textrm{el}}\)), the Hall conductivity (\(\sigma _{\textrm{H}}\)), the thermal conductivity (\(\kappa _0\)) and the Hall-type thermal conductivity (\(\kappa _1\)). The expressions of charge and heat transport coefficients are obtained by solving the relativistic Boltzmann transport equation in the relaxation time approximation at weak magnetic field and finite chemical potential. The interactions among partons are incorporated through their thermal masses. We have observed that \(\sigma _{{\textrm{el}}}\) and \(\kappa _0\) decrease and \(\sigma _{{\textrm{H}}}\) and \(\kappa _1\) increase with the magnetic field in the weak magnetic field regime. On the other hand, the presence of a finite chemical potential increases these transport coefficients. The effects of weak magnetic field and finite chemical potential on aforesaid transport coefficients are found to be more conspicuous at low temperatures, whereas at high temperatures, they have only a mild dependence on magnetic field and chemical potential. We have found that the presence of finite chemical potential further extends the lifetime of the magnetic field. Furthermore, we have explored the effects of weak magnetic field and finite chemical potential on the Knudsen number, the elliptic flow coefficient and the Wiedemann–Franz law.
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Acknowledgements
One of us (S. R.) would like to acknowledge the Indian Institute of Technology Bombay for the Institute postdoctoral fellowship.
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Appendices
Appendices
Derivation of equation (31)
By substituting the following partial derivatives in eq. (30),
and then dropping higher order velocity terms, we get
Comparing the coefficients of \(v_z\) on both sides of Eq. (A.62), we get \(\Gamma _z=0\). Then, we have
where the cyclotron frequency, \(\omega _c=\frac{qB}{\omega _f}\). Equating coefficients of \(v_x\) and \(v_y\) on both sides of Eq. (A.63), we get
After solving Eqs. (A.64) and (A.65), we obtain
Now, ansatz (29) can be written as
By using \(\frac{\partial f_f^0}{\partial p_x}=v_x\frac{\partial f_f^0}{\partial \omega _f}=-v_x\beta f_f^0\left( 1-f_f^0\right) \) and \(\frac{\partial f_f^0}{\partial p_y}=v_y\frac{\partial f_f^0}{\partial \omega _f}=-v_y\beta f_f^0\left( 1-f_f^0\right) \), eq. (A.68) gets simplified into
This leads to the determination of \(\delta f_f\) as
Derivation of Eq. (45)
Substituting the value of L (44) in eq. (43) and simplifying, we have
Equating the coefficients of \(v_x\) and \(v_y\) on both sides of the above equation, we obtain
By solving Eqs. (B.72) and (B.73), \(\Gamma _x\) and \(\Gamma _y\) are respectively determined as
Using the values of \(\Gamma _x\) and \(\Gamma _y\) in ansatz (29) and then simplifying, we get the infinitesimal change of the quark distribution function as
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Rath, S., Dash, S. Effects of weak magnetic field and finite chemical potential on the transport of charge and heat in hot QCD matter. Eur. Phys. J. A 59, 25 (2023). https://doi.org/10.1140/epja/s10050-023-00941-9
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DOI: https://doi.org/10.1140/epja/s10050-023-00941-9