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20002024
most citedDetermining neutron star masses and radii using energy-resolved waveforms of X-ray burst oscillations

110 citations · 2k across the 94 of their papers we have counts for

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Showing 2016Show all

5 papers · 1 filter

astro-ph.HE2016★ 48 cited

The Effect of Transient Accretion on the Spin-Up of Millisecond Pulsars

Sudip Bhattacharyya, Deepto Chakrabarty

A millisecond pulsar is a neutron star that has been substantially spun up by accretion from a binary companion. A previously unrecognized factor governing the spin evolution of su…

gr-qc2016★ 72 cited

Distinguishing Kerr naked singularities and black holes using the spin precession of a test gyro in strong gravitational fields

Chandrachur Chakraborty, Prashant Kocherlakota, Mandar Patil +3

We study here the precession of the spin of a test gyroscope attached to a stationary observer in the Kerr spacetime, specifically, to distinguish naked singularity (NS) from black…

astro-ph.HE2016★ 20 cited

Neutron Star Physics in the Square Kilometer Array Era : An Indian Perspective

Sushan Konar, Manjari Bagchi, Debades Bandyopadhyay +14

It is an exceptionally opportune time for Astrophysics when a number of next-generation mega-instruments are poised to observe the universe across the entire electromagnetic spectr…

astro-ph.HE2016

On the evolution of the inner disk radius with flux in the neutron star low-mass X-ray binary Serpens X-1

Chia-Ying Chiang, Robert A. Morgan, Edward M. Cackett +3

We analyze the latest \emph{Suzaku} observation of the bright neutron star low-mass X-ray binary Serpens X-1 taken in 2013 October and 2014 April. The observation was taken using t…

astro-ph.HE2016★ 56 cited

Fast spinning strange stars: possible ways to constrain interacting quark matter parameters

Sudip Bhattacharyya, Ignazio Bombaci, Domenico Logoteta +1

For a set of equation of state (EoS) models involving interacting strange quark matter, characterized by an effective bag constant (B_eff) and a perturbative QCD corrections term (…