21 citations · 114 across the 13 of their papers we have counts for
14 papers
Resonant Dynamics of Gravitational Wave and Chiral Alfvén wave in the Early Universe
Arun Kumar Pandey, Subalakshmi A, Sampurn Anand
In this work, we investigate the resonant interaction between stochastic gravitational waves (GWs) and chiral Alfvén waves in a magnetized chiral plasma in the early Universe. Star…
Thermal SZ effect in a magnetized IGM dominated by interacting DM decay/annihilation during dark ages
Arun Kumar Pandey, Sunil Malik
During cosmic dawn, the thermal history of the universe is well studied, and a study of this era can give us some of the most useful insight into the universe before the recombinat…
Generating Seed magnetic field à la Chiral Biermann battery
Arun Kumar Pandey, Sampurn Anand
Cosmological and astrophysical observations indicate the presence of magnetic field over all scales. In order to explain these magnetic fields, it is assumed that there exists a se…
Gravitational waves in neutrino plasma and NANOGrav signal
Arun Kumar Pandey
The recent finding of the gravitational wave (GW) signal by the NANOGrav collaboration in the nHZ frequency range has opened up the door for the existence of stochastic GWs. In the…
Implications of baryon-dark matter interaction on IGM temperature and tSZ effect with magnetic field
Arun Kumar Pandey, Sunil Malik, T. R. Seshadri
We show that the combined effect of cosmic magnetic field and a possible non-standard interaction between baryons and dark matter has interesting consequences on the thermal Sunyae…
Magnetic fields in a hot dense neutrino plasma and the Gravitational Waves
Arun Kumar Pandey, Pravin Kumar Natwariya, Jitesh R Bhatt
In the present work, we have studied the spectrum of the primordial gravitational waves due to magnetic instability in the presence of neutrino asymmetry. The magnetic instability…
Viscosity in cosmic fluids
Pravin Kumar Natwariya, Jitesh R Bhatt, Arun Kumar Pandey
The effective theory of large-scale structure formation based on CDM paradigm predicts finite dissipative effects in the resulting fluid equations. In this work, we study how vi…
Baryon-Dark matter interaction in presence of magnetic fields in light of EDGES signal
Jitesh R. Bhatt, Pravin Kumar Natwariya, Alekha C. Nayak +1
We have shown that in presence of a cosmic magnetic field the bounds on baryon dark matter cross-section (), dark-matter mass () and values of the magnetic field ($B_0…
Chiral plasma instability and primordial Gravitational wave
Sampurn Anand, Jitesh R. Bhatt, Arun Kumar Pandey
It is known that cosmic magnetic field, if present, can generate anisotropic stress in the plasma and hence, can act as a source of gravitational waves. These cosmic magnetic field…
Origin and dynamics of the Primordial Magnetic field in a parity violating plasma
Arun Kumar Pandey
In this thesis, we have studied the generation and evolution of the magnetic field in the early Universe. We investigated the generation of magnetic fields in the presence of chira…
Chiral Battery, scaling laws and magnetic fields
Sampurn Anand, Jitesh R. Bhatt, Arun Kumar Pandey
We study the generation and evolution of magnetic field in the presence of chiral imbalance and gravitational anomaly which gives an additional contribution to the vortical current…
Effect of background magnetic field on the normal modes of conformal dissipative chiral hydro and a novel mechanism for explaining pulsar kicks
Arun Kumar Pandey, Manu George
In the present work, we have studied the collective behaviour of a chiral plasma with first and second order dissipative corrections allowed by conformal symmetry. We have derived…
Primordial Generation of Magnetic Fields
Arun Kumar Pandey, Jitesh R. Bhatt
We reexamine generation of the primordial magnetic fields, at temperature TeV, by applying a consistent kinetic theory framework which is suitably modified to take the quantu…
Primordial magnetic field and kinetic theory with Berry curvature
Jitesh R. Bhatt, Arun Kumar Pandey
We study the generation of magnetic field in the primordial plasma of the standard model (SM) particles at temperature ~TeV much higher than the electroweak scale. It is assu…