activity
20122023
most citedMHD simulations of oscillating cusp-filling tori around neutron stars -- missing upper kHz QPO

10 citations · 27 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2023★ 5 cited

Magnetically threaded accretion disks in resistive magnetohydrodynamic simulations and asymptotic expansion

Miljenko Čemeljić, Włodek Kluźniak, Varadarajan Parthasarathy

Aims. A realistic model of magnetic linkage between a central object and its accretion disk is a prerequisite for understanding the spin history of stars and stellar remnants. To t…

astro-ph.SR2019★ 1 cited

A magnetized thin accretion disk: numerical simulations compared with asymptotic expansion

M. Čemeljić, W. Kluźniak, V. Parthasarathy

To obtain a simple description of a geometrically thin magnetic accretion disk, we apply the method of asymptotic expansion. For the first time we write a full set of stationary as…

astro-ph.SR2018

Analytical solution for magnetized thin accretion disk in comparison with numerical simulations

Miljenko Čemeljić, Varadarajan Parthasarathy, Włodek Kluźniak

We obtained equations for a thin magnetic accretion disk, using the method of asymptotic approximation. They cannot be solved analytically-without solutions for a magnetic field in…

astro-ph.HE2018★ 3 cited

MHD simulations of resistive viscous accretion disk around millisecond pulsar

M. Čemeljić, V. Parthasarathy, W. Kluźniak

We perform MHD simulations of a thin resistive and viscous accretion disk around a neutron star with the surface dipolar magnetic field of 10 Gauss. The system evolution is fol…

astro-ph.HE2017★ 10 cited

MHD simulations of oscillating cusp-filling tori around neutron stars -- missing upper kHz QPO

Varadarajan Parthasarathy, Wlodek Kluzniak, Miljenko Cemeljic

We performed axisymmetric, grid-based, ideal magnetohydrodynamic (MHD) simulations of oscillating cusp-filling tori orbiting a non-rotating neutron star. A pseudo-Newtonian potenti…

astro-ph.HE2016★ 1 cited

Numerical simulations of oscillating tori in a pseudo-Newtonian potential

Varadarajan Parthasarathy, Antonios Manousakis, Wlodek Kluzniak

We have modeled hydrodynamical tori in the Klu{ź}niak-Lee pseudo-Newtonian potential. The tori in equilibrium were perturbed with uniform sub-sonic velocity fields: vertical, radia…

astro-ph.HE2015★ 5 cited

Quasi-periodic oscillations of perturbed tori

Varadarajan Parthasarathy, Antonios Manousakis, Wlodek Kluzniak

We performed axisymmetric hydrodynamical simulations of oscillating tori orbiting a non-rotating black hole. The tori in equilibrium were constructed with a constant distribution o…

astro-ph.HE2014

Numerical simulations of thin accretion discs with PLUTO

Varadarajan Parthasarathy, Wlodek Kluzniak

Our goal is to perform global simulations of thin accretion discs around compact bodies like neutron stars with dipolar magnetic profile and black holes by exploiting the facilitie…

astro-ph.CO2012★ 2 cited

An Analysis On Ward Identity For Multi-Field Inflation

Varadarajan Parthasarathy

Given a correlation function (or n-point function), can the corresponding nature of space-time be determined ? To answer this question it is required to derive the Ward Identity (W…