Zobrazeno 1 - 10
of 6 954
pro vyhledávání: '"Antonini, P"'
We establish an equivalence between non-isometry of quantum codes and state-dependence of operator reconstruction, and discuss implications of this equivalence for holographic duality. Specifically, we define quantitative measures of non-isometry and
Externí odkaz:
http://arxiv.org/abs/2411.07296
Autor:
Fantoccoli, Federico, Barber, Jordan, Dosopoulou, Fani, Chattopadhyay, Debatri, Antonini, Fabio
We investigate black hole-star binaries formed in $N$-body simulations of massive, dense star clusters. We simulate 32 clusters with varying initial masses ($10^{4}~\rm M_{\odot}$ to $10^{6}~\rm M_{\odot}$), densities ($1200~\rm M_{\odot}~pc^{-3}$ to
Externí odkaz:
http://arxiv.org/abs/2410.17323
Autor:
Barber, Jordan, Antonini, Fabio
Understanding binary black hole (BBH) dynamics in dense star clusters is key to interpreting the gravitational wave detections by LIGO and Virgo. Here, we perform $N$-body simulations of star clusters, focusing on BBH formation mechanisms, dynamical
Externí odkaz:
http://arxiv.org/abs/2410.03832
Autor:
Antonini, Stefano, Rath, Pratik
We discuss a situation where a holographic CFT state has multiple semiclassical bulk duals. In our example, a given holographic state has two simple, semiclassical descriptions, one with a closed universe, constructed using the gravitational path int
Externí odkaz:
http://arxiv.org/abs/2408.02720
Autor:
Chattopadhyay, Debatri, Al-Shammari, Sama, Antonini, Fabio, Fairhurst, Stephen, Miles, Benjamin, Raymond, Vivien
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters (2024), 536, L19
We investigate the effects of prior selection on the inferred mass and spin parameters of the neutron star-black hole merger GW230529\_181500. Specifically, we explore models motivated by astrophysical considerations, including massive binary and pul
Externí odkaz:
http://arxiv.org/abs/2407.08719
Stellar evolution theories predict a gap in the black hole birth mass spectrum as the result of pair instability processes in the cores of massive stars.This gap, however, is not seen in the binary black hole masses inferred from gravitational wave d
Externí odkaz:
http://arxiv.org/abs/2406.19044
Autor:
Mahapatra, Parthapratim, Chattopadhyay, Debatri, Gupta, Anuradha, Antonini, Fabio, Favata, Marc, Sathyaprakash, B. S., Arun, K. G.
Publikováno v:
ApJ 975 117 (2024)
We propose a Bayesian inference framework to predict the merger history of LIGO-Virgo binary black holes (BHs), whose binary components may have undergone hierarchical mergers in the past. The framework relies on numerical relativity predictions for
Externí odkaz:
http://arxiv.org/abs/2406.06390
The global sports analytics industry has a market value of USD 3.78 billion in 2023. The increase of wearables such as GPS sensors has provided analysts with large fine-grained datasets detailing player performance. Traditional analysis of this data
Externí odkaz:
http://arxiv.org/abs/2407.13109
We construct 4D flat Big Bang-Big Crunch cosmologies and Anti-de Sitter (AdS) planar eternally traversable wormholes using braneworlds embedded in asymptotically AdS${}_5$ spacetimes. The background geometries are the AdS${}_5$ magnetic black brane a
Externí odkaz:
http://arxiv.org/abs/2405.18465
Autor:
Forastier, Bruno Rando, Pina, Daniel Marín, Gieles, Mark, Zwart, Simon Portegies, Antonini, Fabio
Dynamical interactions in star clusters are an efficient mechanism to produce the coalescing binary black holes (BBHs) that have been detected with gravitational waves (GWs). We want to understand how BBH coalescence can occur during - or after - bin
Externí odkaz:
http://arxiv.org/abs/2405.16999