activity
19942023
most citedThe Raychaudhuri equations: a brief review

197 citations · 720 across the 34 of their papers we have counts for

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Showing 2018Show all

7 papers · 1 filter

gr-qc2018

Tidal Love Numbers of Black Holes and Neutron Stars in the Presence of Higher Dimensions: Implications of GW170817

Kabir Chakravarti, Sumanta Chakraborty, Sukanta Bose +1

We calculate the tidal Love numbers of black holes and neutron stars in the presence of higher dimensions. The perturbation equations around an arbitrary static and spherically sym…

gr-qc2018

Fate of Strong Cosmic Censorship Conjecture in Presence of Higher Spacetime Dimensions

Mostafizur Rahman, Sumanta Chakraborty, Soumitra SenGupta +1

Strong cosmic censorship conjecture has been one of the most important leap of faith in the context of general relativity, providing assurance in the deterministic nature of the as…

gr-qc2018

Scalaron tunneling and the fate of antisymmetric tensor fields in gravity

Tanmoy Paul, Soumitra SenGupta

The work provides a possible explanation of a well motivated question - why the present universe is practically free from any noticeable footmarks of higher rank antisymmetric tens…

gr-qc2018

Dynamical suppression of spacetime torsion

Tanmoy Paul, Soumitra SenGupta

A surprising feature of our present four dimensional universe is that its evolution appears to be governed solely by spacetime curvature without any noticeable effect of spacetime…

hep-th2018

Radion induced inflation on non-flat brane and modulus stabilization

Indrani Banerjee, Sumanta Chakraborty, Soumitra SenGupta

Warped braneworld models has the potential to provide a plausible resolution to the gauge hierarchy problem but at the cost of introduction of an additional field, namely the inter…

hep-th2018

Invisibility of antisymmetric tensor fields in the light of gravity

Ashmita Das, Tanmoy Paul, Soumitra SenGupta

A natural question arises from observable signatures of scalar, fermion, and vector degrees of freedom (d.o.f.) in our Universe along with spin 2 symmetric tensor field in the form…