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20022026
most citedThe second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

1k citations · 2.3k across the 73 of their papers we have counts for

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astro-ph2008★ 9 cited

Rotational parameters of strange stars in comparison with neutron stars

Manjari Bagchi

I study stellar structures the mass, the radius, the moment of inertia and the oblateness parameter at different spin frequencies for strange stars and neutron stars in a co…

astro-ph2008

Strange Stars : An interesting member of the compact object family

Manjari Bagchi, Subharthi Ray, Jishnu Dey +1

We have studied strange star properties both at zero temperature and at finite temperatures and searched signatures of strange stars in gamma-ray, x-ray and radio astronomy. We hav…

astro-ph2007

Importance of constraining the dense matter Equation of State in pulsar astrophysics

Manjari Bagchi

We study the dependence of the surface magnetic fields of radio pulsars on the choice of Equations of State, pulsar masses and the values of the angle between the magnetic axis and…

astro-ph2007★ 1 cited

Bound for entropy and viscosity ratio for strange quark matter

Manjari Bagchi, Jishnu Dey, Mira Dey +4

High energy density ($\eps$) and temperature (T) links general relativity and hydrodynamics leading to a lower bound for the ratio of shear viscosity () and entropy density (…

astro-ph2006★ 3 cited

Members of the double pulsar system PSR J0737-3039 : neutron stars or strange stars ?

Manjari Bagchi, Jishnu Dey, Sushan Konar +2

One interesting method of constraining the dense matter Equations of State is to measure the advancement of the periastron of the orbit of a binary radio pulsar (when it belongs to…

astro-ph2006★ 61 cited

A three stage model for the inner engine of Gamma Ray Burst: Prompt emission and early afterglow

Jan Staff, Rachid Ouyed, Manjari Bagchi

We propose a new model within the ``Quark-nova'' scenario to interpret the recent observations of early afterglows of long Gamma-Ray Bursts (GRB) with the Swift satellite. This is…

astro-ph2006★ 2 cited

Chromo-thermal oscillations and collapse of strange stars to black holes : Astrophysical Implications

Manjari Bagchi, Rachid Ouyed, Jan Staff +3

The effects of temperature on strange stars are studied and it is found that the maximum mass of the star decreases with the increase of temperature since at high temperatures the…

astro-ph2006★ 7 cited

Evidence for strange stars from joint observation of harmonic absorption bands and of redshift

Manjari Bagchi, Subharthi Ray, Mira Dey +1

From recent reports on terrestrial heavy ion collision experiments it appears that one may not obtain information about the existence of asymptotic freedom (AF) and chiral symmetry…

astro-ph2006★ 3 cited

Strange stars at finite temperature

Subharthi Ray, Manjari Bagchi, Jishnu Dey +1

We calculate strange star properties, using large N_c approximation with built-in chiral symmetry restoration (CSM). We used a relativistic Hartree Fock mean field approximation me…

astro-ph2006★ 17 cited

Compact strange stars with a medium dependence in gluons at finite temperature

Manjari Bagchi, Subharthi Ray, Mira Dey +1

The possible existence of strange stars in the universe will help in the understanding of various properties of quantum chromodynamics, like asymptotic freedom and chiral symmetry…

astro-ph2005★ 5 cited

Strange Pulsar Hypothesis

Raka Dona Ray Mandal, Monika Sinha, Manjari Bagchi +3

It appears that there is a genuine shortage of radio pulsars with surface magnetic fields significantly smaller than Gauss. We propose that the pulsars with very low ma…

astro-ph2005★ 1 cited

Strange Star Equation of State With a Modified Richardson Potential

Manjari Bagchi, Subharthi Ray, Mira Dey +1

Richardson potential is an phenomenological interquark interaction taking care of two aspects of QCD, namely the asymptotic freedom and the confinement. The original potential has…

astro-ph2005★ 5 cited

Newtonian and general relativistic contribution of gravity to surface tension of strange stars

Manjari Bagchi, Monika Sinha, Mira Dey +2

Surface tension (S) is due to the inward force experienced by particles at the surface and usually gravitation does not play an important role in this force. But in compact stars t…