Zobrazeno 1 - 10
of 12
pro vyhledávání: '"Yonadav Barry Ginat"'
Autor:
Yonadav Barry Ginat, Hagai B. Perets
Publikováno v:
Physical Review X, Vol 11, Iss 3, p 031020 (2021)
We present a statistical approximate solution of the bound, nonhierarchical three-body problem, and extend it to a general analysis of encounters between hard binary systems and single stars. Any such encounter terminates when one of the three stars
Externí odkaz:
https://doaj.org/article/87f00987300d460d8c94bec89b4adc93
Autor:
Yonadav Barry Ginat
Publikováno v:
The Sixteenth Marcel Grossmann Meeting.
Autor:
Hagai Perets, Yonadav Barry Ginat
Chaotic three-body interactions may lead to the formation of gravitational-wave sources. Here, by modelling the encounter as a series of close, non-hierarchical, triple approaches, interspersed with hierarchical phases, in which the system consists o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d4c35bcdfcad3c44471e9463f3d6a3ce
http://arxiv.org/abs/2205.15957
http://arxiv.org/abs/2205.15957
We study the small-scale asymptotic behaviour of the cold dark matter density fluctuation power spectrum in the Zel'dovich approximation, without introducing an ultraviolet cut-off. Assuming an initially correlated Gaussian random field and spectral
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef378777f6d1c90e754d703f33a7c6ff
Autor:
Yonadav Barry Ginat, Hagai B. Perets
Binary evolution is influenced by dynamical scattering with other stars in dense environments. Heggie's law states that, due to their environments, hard binaries (whose orbital energy surpasses the typical energy of single stars) tend to harden (incr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7cc869649e0d2b1f697e2fff1684e305
http://arxiv.org/abs/2108.01085
http://arxiv.org/abs/2108.01085
We propose a novel source of gravitational wave emission: the inspirals of compact fragments inside primordial supermassive stars (SMSs). Such systems are thought to be an essential channel in the as-yet little understood formation of supermassive bl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8ccfcea8010d763cf6b5abe4e6d83b20
https://doi.org/10.1093/mnras/stab1415
https://doi.org/10.1093/mnras/stab1415
The coalescence of compact binary stars is expected to produce a stochastic background of gravitational waves (GW) observable with future GW detectors. Such backgrounds are usually characterized by their power spectrum as a function of frequency. Her
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fcb21045f5041ed9abb3451e0a4aff25
https://resolver.caltech.edu/CaltechAUTHORS:20201002-091639268
https://resolver.caltech.edu/CaltechAUTHORS:20201002-091639268
Scalar, tensor waves induce oscillatory perturbations in Keplerian systems that can be probed with measurements of pulsar timing residuals. In this paper, we consider the imprint of coherent oscillations produced by ultralight axion dark matter on th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77060fa7a9e9baf27ef2e5e44d36fa6f
http://arxiv.org/abs/2003.10552
http://arxiv.org/abs/2003.10552
We explore the implications of a single observer's viewpoint on measurements of galaxy clustering statistics. We focus on the Bardeen potentials, which imprint characteristic scale-dependent signatures in the observed galaxy power spectrum. The exist
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::65ba3c986b6b4c81becea5ab9f10919e
Detection of gravitational-wave (GW) sources enables the characterisation of binary compact objects and of their in-spiral. However, other dissipative processes can affect the in-spiral. Here we show that the in-spiral of compact objects through a ga
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f1bc198f1683e9bc2d8390d91b1b7308
http://arxiv.org/abs/1903.11072
http://arxiv.org/abs/1903.11072