Zobrazeno 1 - 10
of 25
pro vyhledávání: '"Filippo Santoliquido"'
Publikováno v:
Universe, Vol 9, Iss 12, p 507 (2023)
The origin of the spins of stellar-mass black holes is still controversial, and angular momentum transport inside massive stars is one of the main sources of uncertainty. Here, we apply hierarchical Bayesian inference to derive constraints on spin mo
Externí odkaz:
https://doaj.org/article/228bcc7a03264eb7890d79303eadeab1
Autor:
Michela Mapelli, Filippo Santoliquido, Yann Bouffanais, Manuel Arca Sedda, Maria Celeste Artale, Alessandro Ballone
Publikováno v:
Symmetry, Vol 13, Iss 9, p 1678 (2021)
Hierarchical mergers are one of the distinctive signatures of binary black hole (BBH) formation through dynamical evolution. Here, we present a fast semi-analytic approach to simulate hierarchical mergers in nuclear star clusters (NSCs), globular clu
Externí odkaz:
https://doaj.org/article/a6f5a421dd024a8594444e6ed808bb43
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 516:3297-3317
The merger rate density evolution of binary compact objects and the properties of their host galaxies carry crucial information to understand the sources of gravitational waves. Here, we present galaxyRate, a new code that estimates the merger rate d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bad05d638014af3d4be0c613a268cfa8
https://doi.org/10.1093/mnras/stac2384
https://doi.org/10.1093/mnras/stac2384
Autor:
Guglielmo Costa, Michela Mapelli, Giuliano Iorio, Filippo Santoliquido, Gastón J. Escobar, Alessandro Bressan
Database of input configuration files for SEVN population synthesis code (available at this link, branch Costa23popIII, commit 0f9ae3bf)and numerical results for the paper: Massive binary black holes from Population II and III stars ABSTRACT: Populat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10084701c10295be60d1b2e243559269
Autor:
Barbara Patricelli, Maria Grazia Bernardini, Michela Mapelli, Paolo D’Avanzo, Filippo Santoliquido, Giancarlo Cella, Massimiliano Razzano, Elena Cuoco
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 513:4159-4168
The joint detection of GW170817 and GRB 170817A opened the era of multi-messenger astronomy with gravitational waves (GWs) and provided the first direct probe that at least some binary neutron star (BNS) mergers are progenitors of short gamma-ray bur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e11e591b3136d9c2fa82f7118e4de2b8
https://doi.org/10.1093/mnras/stac1167
https://doi.org/10.1093/mnras/stac1167
Autor:
Ugo N. Di Carlo, M. Celeste Artale, Nicola Giacobbo, Giuliano Iorio, Yann Bouffanais, Filippo Santoliquido, Sara Rastello, Michela Mapelli
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 507:5224-5235
With the recent release of the second gravitational-wave transient catalogue (GWTC-2), which introduced dozens of new detections, we are at a turning point of gravitational wave astronomy, as we are now able to directly infer constraints on the astro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3be2a13f942a0241dcc3bb5713aec780
https://doi.org/10.1093/mnras/stab2438
https://doi.org/10.1093/mnras/stab2438
Autor:
Alessandro Ballone, Giuliano Iorio, Michela Mapelli, Sara Rastello, Ugo N. Di Carlo, Nicola Giacobbo, Filippo Santoliquido, Stefano Torniamenti
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 507:3612-3625
Young star clusters are dynamically active stellar systems and are a common birthplace for massive stars. Low-mass star clusters ($\sim{}300-10^3$ M$_\odot$) are more numerous than massive systems and are characterized by a two-body relaxation time s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::202f8ee264711d1a5f0f38e6fa501b58
https://doi.org/10.1093/mnras/stab2355
https://doi.org/10.1093/mnras/stab2355
Autor:
Filippo Santoliquido
data sets to reproduce figures 7 to 12 and 13 inhttps://arxiv.org/pdf/2205.05099.pdf Description of the naming: HG_model_alphavalue_GSSI_v2_object_snapshot_12Z_50_No_0.14_2 model:M57 stands forMZR, M54 stands for FMR alphavalue:A1, A3, A5 standfor co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::79294cfd9d4bbb04244bcbe1dca442e7
Autor:
Ugo N Di Carlo, Michela Mapelli, Nicola Giacobbo, Mario Spera, Alessandro Ballone, Filippo Santoliquido, Sara Rastello, Giuliano Iorio
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Young star clusters are likely the most common birthplace of massive stars across cosmic time and influence the formation of compact binaries in several ways. Here, we simulate the formation of black hole -- neutron star binaries (BHNSs) in young sta
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e1791f3574dcd2e99e8b01cc76c77ac0
https://doi.org/10.1093/mnras/staa2018
https://doi.org/10.1093/mnras/staa2018
Autor:
Carole Périgois, Filippo Santoliquido, Yann Bouffanais, Ugo N. Di Carlo, Nicola Giacobbo, Sara Rastello, Michela Mapelli, Tania Regimbau
We study the impact of young clusters on the gravitational wave background from compact binary coalescence. We simulate a catalog of sources from population I/II isolated binary stars and stars born in young clusters, corresponding to one year of obs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4befd9405ea5897defd0f963c636f799
https://hdl.handle.net/11577/3460456
https://hdl.handle.net/11577/3460456