Gravitational-wave cosmological distances in scalar-tensor theories of gravity
DOI10.1088/1475-7516/2021/06/050zbMath1485.83018arXiv2103.00155OpenAlexW3176919916MaRDI QIDQ5028770
Alice Garoffolo, Sabino Matarrese, Gianmassimo Tasinato, Daniele Bertacca
Publication date: 10 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2103.00155
Diffraction, scattering (78A45) Quantum field theory on curved space or space-time backgrounds (81T20) Electromagnetic fields in general relativity and gravitational theory (83C50) Gravitational energy and conservation laws; groups of motions (83C40) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Perturbations in context of PDEs (35B20) Gravitational waves (83C35) Matrix models and tensor models for quantum field theory (81T32)
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Cites Work
- Republication of: ``LX. On the definition of distance in general relativity
- Degenerate higher order scalar-tensor theories beyond Horndeski up to cubic order
- Effective field theory of cosmological perturbations
- Mach's Principle and a Relativistic Theory of Gravitation
- The magnitude–redshift relation in a perturbed Friedmann universe
- Nonlocal gravity. Conceptual aspects and cosmological predictions
- Constraining scalar-tensor modified gravity with gravitational waves and large scale structure surveys
- Testing modified gravity at cosmological distances with LISA standard sirens
- Gravitational waves and geometrical optics in scalar-tensor theories
- Quantum gravity and gravitational-wave astronomy
- General Relativity
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