Gravitational wave from extreme mass-ratio inspirals as a probe of extra dimensions
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Publication:5880472
DOI10.1088/1475-7516/2023/01/046OpenAlexW4318481444MaRDI QIDQ5880472
Mostafizur Rahman, Arpan Bhattacharyya, Shailesh Kumar
Publication date: 2 March 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2212.01404
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- The hierarchy problem and new dimensions at a millimeter
- Signatures of the sources in the gravitational waves of a perturbed Schwarzschild black hole
- Heterotic and type I string dynamics from eleven dimensions
- Fate of strong cosmic censorship conjecture in presence of higher spacetime dimensions
- Gravitational Radiation from a Kerr Black Hole. I. Formulation and a Method for Numerical Analysis
- Inner structure of a charged black hole: An exact mass-inflation solution
- Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- The interior of charged black holes and the problem of uniqueness in general relativity
- Rotating black string and the effective Teukolsky equation in the braneworld
- Leakage of gravitational waves into an extra dimension in the DGP model
- Looking for extra dimensions in the observed quasi-periodic oscillations of black holes
- Gravitational radiation from a binary system in odd-dimensional spacetime
- Gravitational wave echoes induced by a point mass plunging into a black hole
- Intermediate and extreme mass-ratio inspirals—astrophysics, science applications and detection using LISA
- Mapping spacetimes with LISA: inspiral of a test body in a ‘quasi-Kerr’ field
- Gravitational wave from extreme mass-ratio inspirals as a probe of extra dimensions
- Brane-world gravity
- The motion of point particles in curved spacetime
- Black holes on the brane
