Discovering Love numbers through resonance excitation during extreme mass ratio inspirals
From MaRDI portal
Publication:6573751
DOI10.1088/1361-6382/AD563AzbMATH Open1546.83089MaRDI QIDQ6573751
Yotam Sherf, R. Brustein, Shani Avitan
Publication date: 17 July 2024
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Gravitational waves (83C35)
Cites Work
- Title not available (Why is that?)
- On the vanishing of Love numbers for Kerr black holes
- Hidden symmetry of the static response of black holes: applications to Love numbers
- On the viability of regular black holes
- Can we observe fuzzballs or firewalls?
- Gravitational radiation for extreme mass ratio inspirals to the 14th post-Newtonian order
- General Relativistic Fluid Spheres
- The singularities of gravitational collapse and cosmology
- Intermediate and extreme mass-ratio inspirals—astrophysics, science applications and detection using LISA
- Massive spheres in general relativity
- Gravitational Collapse and Space-Time Singularities
- Black holes as collapsed polymers
- Emergent horizon, Hawking radiation and chaos in the collapsed polymer model of a black hole
- The fuzzball proposal for black holes: an elementary review
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
- Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity
- The Non-radial Oscillations of Polytropic Stars
- Ladder symmetries of black holes. Implications for love numbers and no-hair theorems
This page was built for publication: Discovering Love numbers through resonance excitation during extreme mass ratio inspirals
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q6573751)