activity
20192026
most citedAsymmetric accretion and thermal `mountains' in magnetized neutron star crusts

33 citations · 145 across the 14 of their papers we have counts for

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Showing astro-ph.HEShow all

9 papers · 1 filter

astro-ph.HE2026

Remnant recoil and host environments of GWTC-4.0 binary black-hole mergers

Joan Llobera-Querol, Eleanor Hamilton, Neha Singh +8

Determining the astrophysical origin of binary black holes and whether merger remnants are retained in their birth environments is essential for understanding hierarchical mergers…

astro-ph.HE2025

Estimating the binary neutron star merger rate density evolution with Einstein Telescope

Neha Singh, Tomasz Bulik, Aleksandra Olejak

The Einstein Telescope (ET) is a proposed third-generation, wide-band gravitational wave (GW) detector which will have an improved detection sensitivity in low frequencies, leading…

astro-ph.HE2023★ 3 cited

An Optically Targeted Search for Gravitational Waves emitted by Core-Collapse Supernovae during the Third Observing Run of Advanced LIGO and Advanced Virgo

Marek J. Szczepańczyk, Yanyan Zheng, Javier M. Antelis +35

We present the results from a search for gravitational-wave transients associated with core-collapse supernovae observed optically within 30 Mpc during the third observing run of A…

astro-ph.HE2023★ 3 cited

Reconstructing the star formation rate for compact binary populations with the Einstein telescope

Neha Singh, Tomasz Bulik, Krzysztof Belczynski +2

The Einstein Telescope (ET) is a proposed third-generation, wide-band gravitational wave (GW) detector. Given its improved detection sensitivity in comparison to the second-generat…

astro-ph.HE2021★ 25 cited

Exploring compact binary populations with the Einstein Telescope

Neha Singh, Tomasz Bulik, Krzysztof Belczynski +1

The Einstein Telescope (ET), a wide-band, future third generation gravitational wave detector, is expected to have detection rates of binary black hole (BBH) det…

astro-ph.HE2021★ 4 cited

Constraining parameters of low mass merging compact binary systems with Einstein Telescope alone

Neha Singh, Tomasz Bulik

The Einstein Telescope (ET), a future third-generation gravitational wave detector will have detection sensitivity for gravitational wave signals down to 1 Hz. This improved low-fr…

astro-ph.HE2021★ 6 cited

Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era

Marek Szczepanczyk, Javier Antelis, Michael Benjamin +17

We performed a detailed analysis of the detectability of a wide range of gravitational waves derived from core-collapse supernova simulations using gravitational-wave detector nois…

astro-ph.HE2020★ 6 cited

Constraining parameters of coalescing stellar mass binary black hole systems with the Einstein Telescope alone

Neha Singh, Tomasz Bulik

The Einstein Telescope (ET) is the future third generation gravitational wave detector consisting of three independent interferometers arranged in a triangular configuration, with…

astro-ph.HE2019★ 33 cited

Asymmetric accretion and thermal `mountains' in magnetized neutron star crusts

Neha Singh, Brynmor Haskell, Dipanjan Mukherjee +1

Accreting neutron stars are one of the main targets for continuous gravitational wave searches, as asymmetric accretion may lead to quadrupolar deformations, or `mountains', on the…