activity
20112026
most citedCan extra dimensional effects allow wormholes without exotic matter?

67 citations · 162 across the 19 of their papers we have counts for

collaborators

20 papers

gr-qc2026

Viscosity effects on the shadow of a non-rotating black hole

Sayantani Lahiri, Sergio Gimeno-Soler, Alejandro Cruz-Osorio +2

We study the effect of shear viscosity in stationary magnetized accretion tori on synthetic images of non-rotating black hole shadows. Shear viscosity and spacetime-curvature contr…

gr-qc2025

Equilibrium models of Weyssenhoff spin fluid accretion tori around Kerr black holes

Sergio Gimeno-Soler, Sayantani Lahiri, Claus Lämmerzahl

The construction of equilibrium models of accretion disks around compact objects has become a highly relevant topic in the recent times, thanks to the current understanding that in…

gr-qc2023

Stationary equilibrium torus supported by Weyssenhoff ideal spin fluid in Schwarzschild spacetime -- I: Case of constant specific angular momentum distribution

Sayantani Lahiri, Claus Laemmerzahl

We consider a non-self-gravitating geometrically thick torus described by Weyssenhoff ideal spin fluid in a black hole spacetime. The Weyssenhof spin fluid shares the same symmetri…

gr-qc2023★ 3 cited

Sustaining quasi de-Sitter inflation with bulk viscosity

Sayantani Lahiri, Luciano Rezzolla

We here investigate bulk-viscosity driven quasi de-Sitter inflation, that is, the period of accelerated expansion in the early universe during which , with …

cond-mat.quant-gas2023★ 6 cited

Quantum phases of constrained bosons on a two-leg Bose-Hubbard ladder

Ashirbad Padhan, Rajashri Parida, Sayan Lahiri +2

Bosons in periodic potentials with very strong local interactions, known as the constrained bosons often exhibit interesting physical behavior. We investigate the ground state prop…

gr-qc2021★ 9 cited

Stationary models of magnetized viscous tori around a Schwarzschild black hole

Sayantani Lahiri, Sergio Gimeno-Soler, José A. Font +1

We present stationary solutions of magnetized, viscous thick accretion disks around a Schwarzschild black hole. We assume that the tori are not self-gravitating, are endowed with a…