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20142026
most citedVelocity-dependent Self-interacting Dark Matter from Groups and Clusters of Galaxies

112 citations · 869 across the 36 of their papers we have counts for

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10 papers · 1 filter

gr-qc2025★ 2 cited

Detectability of Massive Boson Stars using Gravitational Waves from Fundamental Oscillations

Swarnim Shirke, Bikram Keshari Pradhan, Debarati Chatterjee +2

Boson Stars are macroscopic self-gravitating configurations made of complex scalar fields. These exotic compact objects would manifest as dark Boson stars and, in the absence of el…

gr-qc2025★ 1 cited

Fundamental oscillations as a tool to distinguish boson stars from neutron stars and black holes

Swarnim Shirke, Bikram Keshari Pradhan, Debarati Chatterjee +2

Massive boson stars are self-gravitating configurations of self-interacting scalar fields and can be modeled by a massive scalar field with a quartic self-interaction potential. It…

gr-qc2024★ 32 cited

Effects of Dark Matter on -mode oscillations of Neutron Stars

Swarnim Shirke, Bikram Keshari Pradhan, Debarati Chatterjee +2

The effect of dark matter (DM) on -mode oscillations in DM admixed neutron stars (NSs) is investigated in a comprehensive analysis with particular attention to the role of the n…

gr-qc2024★ 10 cited

Post-Newtonian effects in compact binaries with a dark matter spike: A Lagrangian approach

Diego Montalvo, Adam Smith-Orlik, Saeed Rastgoo +3

We apply the Lagrangian method to study the post-Newtonian evolution of a compact binary system with environmental effects, including a dark matter spike, and obtain the resulting…

gr-qc2023★ 12 cited

Binary systems in massive scalar-tensor theories: Next-to-leading order gravitational wave phase from effective field theory

Robin Fynn Diedrichs, Daniel Schmitt, Laura Sagunski

Neutron star binaries and their associated gravitational wave signal facilitate precision tests of General Relativity. Any deviation of the detected gravitational waveform from Gen…

gr-qc2023★ 21 cited

Fermion Proca Stars: Vector Dark Matter Admixed Neutron Stars

Cédric Jockel, Laura Sagunski

Dark matter could accumulate around neutron stars in sufficient amounts to affect their global properties. In this work, we study the effect of a specific model for dark matter --…

gr-qc2023★ 53 cited

Tidal Deformability of Fermion-Boson Stars: Neutron Stars Admixed with Ultra-Light Dark Matter

Robin Fynn Diedrichs, Niklas Becker, Cédric Jockel +3

In this work we investigate the tidal deformability of a neutron star admixed with dark matter, modeled as a massive, self-interacting, complex scalar field. We derive the equation…

gr-qc2022★ 39 cited

Comparing Accretion Disks and Dark Matter Spikes in Intermediate Mass Ratio Inspirals

Niklas Becker, Laura Sagunski

Intermediate Mass Ratio Inspirals (IMRIs) will be observable with space-based gravitational wave detectors such as the Laser Interferometer Space Antenna (LISA). To this end, the e…

gr-qc2021★ 58 cited

Circularization vs. Eccentrification in Intermediate Mass Ratio Inspirals inside Dark Matter Spikes

Niklas Becker, Laura Sagunski, Lukas Prinz +1

Inspirals of an Intermediate Mass Black Hole (IMBH) and a solar mass type object will be observable by space based gravitational wave detectors such as The Laser Interferometer Spa…

gr-qc2017★ 86 cited

Neutron star mergers as a probe of modifications of general relativity with finite-range scalar forces

Laura Sagunski, Jun Zhang, Matthew C. Johnson +5

Observations of gravitational radiation from compact binary systems provide an unprecedented opportunity to test General Relativity in the strong field dynamical regime. In this pa…