activity
20152021
most citedDark matters on the scale of galaxies

95 citations · 175 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2021★ 9 cited

Probing the shape of the Milky Way dark matter halo with hypervelocity stars: a new method

Arianna Gallo, Luisa Ostorero, Sankha Subhra Chakrabarty +2

We propose a new method to determine the shape of the gravitational potential of the dark matter (DM) halo of the Milky Way (MW) with the galactocentric tangential velocities of a…

hep-ph2021★ 6 cited

Density perturbations in axion-like particles: classical vs quantum field treatment

Sankha Subhra Chakrabarty

Axions and axion-like particles are bosonic quantum fields. They are often assumed to follow classical field equations due to their high degeneracy in the phase space. In this work…

astro-ph.GA2021★ 7 cited

Probing modified Newtonian dynamics with hypervelocity stars

Sankha Subhra Chakrabarty, Luisa Ostorero, Arianna Gallo +2

We show that measuring the velocity components of hypervelocity stars (HVSs) can discriminate between modified Newtonian dynamics (MOND) and Newtonian gravity. HVSs are ejected fro…

astro-ph.CO2020★ 95 cited

Dark matters on the scale of galaxies

Ivan de Martino, Sankha S. Chakrabarty, Valentina Cesare +3

The cold dark matter model successfully explains both the emergence and evolution of cosmic structures on large scales and, when we include a cosmological constant, the properties…

astro-ph.GA2020★ 1 cited

Implications of triangular features in the Gaia skymap for the Caustic Ring Model of the Milky Way halo

Sankha S. Chakrabarty, Yaqi Han, Anthony H. Gonzalez +1

The Gaia map of the Milky Way reveals a pair of triangular features at nearly symmetric locations on opposite sides of the Galactic Center. In this paper we explore the implication…

hep-th2019★ 2 cited

Duration of Classicality of an inhomogeneous quantum field with repulsive contact self-interactions

Ariel Arza, Sankha S. Chakrabarty, Seishi Enomoto +2

Quantum fields with large degeneracy are often approximated as classical fields. Here, we show how quantum and classical evolution of a highly degenerate quantum field with repulsi…

hep-ph2019★ 6 cited

Search for dark photon, axion-like particles, dark scalar, or light dark matter in Compton-like processes

Sankha S. Chakrabarty, Igal Jaeglé

We propose a novel way to search for the dark photon (), the axion-like pseudo-scalar (), the dark scalar (), and the light dark matter () in the Compton-like processe…

astro-ph.GA2018★ 7 cited

Effects of a caustic ring of dark matter on the distribution of stars and interstellar gas

Sankha S. Chakrabarty, Pierre Sikivie

Caustic rings of dark matter with cross-section were predicted to lie in the galactic disk. Their radii increase on cosmological time scales at a rate of order $…

hep-ph2017

Duration of Classicality of Homogeneous Condensates with Attractive Interactions

Sankha Chakrabarty, Seishi Enomoto, Yaqi Han +2

Dark matter axions and other highly degenerate bosonic fluids are commonly described by classical field equations. In a recent paper \cite{BECprop} we calculated the duration of cl…

hep-ph2017★ 17 cited

Gravitational self-interactions of a degenerate quantum scalar field

Sankha S. Chakrabarty, Seishi Enomoto, Yaqi Han +2

We develop a formalism to help calculate in quantum field theory the departures from the description of a system by classical field equations. We apply the formalism to a homogeneo…

hep-ph2016★ 21 cited

Duration of classicality in highly degenerate interacting Bosonic systems

Pierre Sikivie, Elisa M. Todarello

We study sets of oscillators that have high quantum occupancy and that interact by exchanging quanta. It is shown by analytical arguments and numerical simulation that such systems…

astro-ph.CO2015★ 4 cited

Rotation of the polarization vector from distant radio galaxies in the perturbed FRW metric

Sankha Subhra Chakrabarty

Analysis of the correlation between the angular positions of distant radio galaxies on the sky and the orientations of their polarization vectors with respect to their major axes,…