Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Rao, Suvrat"'
Autor:
Schmirander, Thorben, Miltchev, Velizar, Rao, Suvrat, Brüggen, Marcus, Grüner, Florian, Hillert, Wolfgang, Liske, Jochen
This work for the first time addresses the feasibility of measuring millihertz gravitational waves (mHz GWs) with a storage ring-based detector. While this overall challenge consists of several partial problems, here we focus solely on quantifying de
Externí odkaz:
http://arxiv.org/abs/2408.16374
We simulate the response of a Storage Ring Gravitational-Wave Observatory (SRGO) to astrophysical millihertz (mHz) gravitational waves (GWs), numerically obtaining its sensitivity curve and optimal choices for some controllable experiment parameters.
Externí odkaz:
http://arxiv.org/abs/2301.08331
Autor:
Rao, Suvrat, Pezzotti, Camilla, Meynet, Georges, Eggenberger, Patrick, Buldgen, Gaël, Mordasini, Christoph, Bourrier, Vincent, Ekström, Sylvia, Georgy, Cyril
Publikováno v:
A&A 651, A50 (2021)
Tidal interactions and planet evaporation processes impact the evolution of close-in star-planet systems. We study the impact of stellar rotation on these processes. We compute the time evolution of star-planet systems consisting of a planet with ini
Externí odkaz:
http://arxiv.org/abs/2104.07397
Here we calculate the effects of astrophysical gravitational waves (GWs) on the travel times of proton bunch test masses in circular particle accelerators. We show that a high-precision proton bunch time-tagging detector could turn a circular particl
Externí odkaz:
http://arxiv.org/abs/2012.00529
Akademický článek
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Autor:
Rao, Suvrat, Meynet, Georges, Eggenberger, Patrick, Haemmerlé, Lionel, Privitera, Giovanni, Georgy, Cyril, Ekström, Sylvia, Mordasini, Christoph
Publikováno v:
A&A 618, A18 (2018)
When planets are formed from the protoplanetary disk and after the disk has dissipated, the evolution of their orbits is governed by tidal interactions, friction, and gravitational drag, and also by changes in the mass of the star and planet. These i
Externí odkaz:
http://arxiv.org/abs/1807.01474
Autor:
Rao, Suvrat, Meynet, Georges, Eggenberger, Patrick, Haemmerlé, Lionel, Privitera, Giovanni, Georgy, Cyril, Ekström, Sylvia, Mordasini, Christoph
When planets are formed from the protoplanetary disk and after the disk has dissipated, the evolution of their orbits is governed by tidal interactions, friction, and gravitational drag, and also by changes in the mass of the star and planet. These i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::914329604b7ec7ce2aafd22ab1c7f0cf
Akademický článek
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Autor:
'Rao, Suvrat
Publikováno v:
Pezzotti, Camilla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=r3c4b2081b22::4df2f405ddfd7181e0fc3a2e8c350b48
Autor:
Rao, Suvrat, Pezzotti, Camilla, Meynet, Georges, Eggenberger, Patrick, Buldgen, Gaël, Mordasini, Christoph, Bourrier, Vincent, Ekström, Sylvia, Georgy, Cyril
Publikováno v:
Astronomy & Astrophysics. 651:A50
Context. Tidal interactions and planetary evaporation processes impact the evolution of close-in star–planet systems. Aims. We study the impact of stellar rotation on these processes. Methods. We compute the time evolution of star–planet systems
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78521a8d48ccbe63602b156162918094