activity
19942019
most citedPhantom and non-phantom dark energy: The cosmological relevance of non-locally corrected gravity

151 citations · 1.6k across the 46 of their papers we have counts for

collaborators

46 papers

gr-qc2019★ 2 cited

Component separation map-making for stochastic gravitational wave background

Abhishek Parida, Jishnu Suresh, Sanjit Mitra +1

Superposition of unresolved sources of gravitational waves (GW) is expected to create a persistent background of stochastic gravitational wave background (SGWB). Different types of…

gr-qc2017★ 4 cited

Energy emission from high curvature region and its backreation

Takafumi Kokubu, Sanjay Jhingan, Tomohiro Harada

A strong gravity naked singular region can give important clues towards understanding classical as well as spontaneous nature of General Relativity. We propose here a model for ene…

astro-ph.CO2016★ 140 cited

Primordial black hole formation in the matter-dominated phase of the Universe

Tomohiro Harada, Chul-Moon Yoo, Kazunori Kohri +2

We investigate primordial black hole formation in the matter-dominated phase of the Universe, where nonspherical effects in gravitational collapse play a crucial role. This is in c…

gr-qc2015★ 24 cited

Spherical and nonspherical models of primordial black hole formation: exact solutions

Tomohiro Harada, Sanjay Jhingan

We construct spacetimes which provide spherical and nonspherical models of black hole formation in the flat Friedmann--Lemaitre--Robertson--Walker (FLRW) universe with the Lemaitre…

astro-ph.CO2015★ 23 cited

Component Separation of a Isotropic Gravitational Wave Background

Abhishek Parida, Sanjit Mitra, Sanjay Jhingan

A Gravitational Wave Background (GWB) is expected in the universe from the superposition of a large number of unresolved astrophysical sources and phenomena in the early universe.…

astro-ph.HE2015★ 1 cited

XMM-Newton view of a hard X-ray transient IGR J17497-2821

Md. Shah Alam, Dipanjan Mukherjee, Aditya S. Mondal +3

We present spectral and energy dependent timing characteristics of the hard X-ray transient IGR J17497-2821 based on XMM-Newton observations performed five and nine days after its…