Zobrazeno 1 - 10
of 3 851
pro vyhledávání: '"A. Iacovelli"'
Autor:
Iacovelli, Giovanni, Sheemar, Chandan Kumar, Khan, Wali Ullah, Mahmood, Asad, Alexandropoulos, George C., Querol, Jorge, Chatzinotas, Symeon
In this article, we propose the integration of the Holographic Multiple Input Multiple Output (HMIMO) as a transformative solution for next generation Non-Terrestrial Networks (NTNs), addressing key challenges, such as high hardware costs, launch exp
Externí odkaz:
http://arxiv.org/abs/2411.10014
Autor:
Maggiore, Michele, Iacovelli, Francesco, Belgacem, Enis, Mancarella, Michele, Muttoni, Niccolò
We study the performances of a world-wide network made by a European third-generation gravitational-wave (GW) detector, together with a 40-km Cosmic Explorer detector in the US, considering three scenarios for the European detector: (1) Einstein Tele
Externí odkaz:
http://arxiv.org/abs/2411.05754
Autor:
Belgacem, Enis, Iacovelli, Francesco, Maggiore, Michele, Mancarella, Michele, Muttoni, Niccolò
At third-generation (3G) gravitational-wave detector networks, compact binaries coalescences produce a ``confusion noise'' due to unresolved sources and to the error in the reconstruction of resolved sources, that can degrade the sensitivity to cosmo
Externí odkaz:
http://arxiv.org/abs/2411.04029
Autor:
Belgacem, Enis, Iacovelli, Francesco, Maggiore, Michele, Mancarella, Michele, Muttoni, Niccolò
We provide a detailed derivation of the spectral density of the stochastic background generated by the superposition of coalescing compact binaries. We show how the expression often used in the literature emerges from an average over the extrinsic pa
Externí odkaz:
http://arxiv.org/abs/2411.04028
Autor:
De Renzis, Viola, Iacovelli, Francesco, Gerosa, Davide, Mancarella, Michele, Pacilio, Costantino
Third-generation gravitational-wave detectors will observe up to millions of merging binary black holes. With such a vast dataset, stacking events into population analyses will arguably be more important than analyzing single sources. We present the
Externí odkaz:
http://arxiv.org/abs/2410.17325
Autor:
Protani, Andrea, Giusti, Lorenzo, Iacovelli, Chiara, Aillet, Albert Sund, Santos, Diogo Reis, Reale, Giuseppe, Zauli, Aurelia, Moci, Marco, Garbuglia, Marta, Brutti, Pierpaolo, Caliandro, Pietro, Serio, Luigi
After an acute stroke, accurately estimating stroke severity is crucial for healthcare professionals to effectively manage patient's treatment. Graph theory methods have shown that brain connectivity undergoes frequency-dependent reorganization post-
Externí odkaz:
http://arxiv.org/abs/2410.07199
Autor:
Iacovelli, Francesco, Belgacem, Enis, Maggiore, Michele, Mancarella, Michele, Muttoni, Niccolò
Recently, detailed studies have been made to compare the performance of the European next generation GW observatory Einstein Telescope (ET) in a single-site triangular configuration with the performance of a configuration featuring two L-shaped detec
Externí odkaz:
http://arxiv.org/abs/2408.14946
Gravitational-wave observations have the potential of allowing the identification of a population of merging primordial black-hole binaries. We provide an overview of the capabilities of present and future GW detectors, with a special emphasis on the
Externí odkaz:
http://arxiv.org/abs/2407.21442
Autor:
Mancarella, Michele, Iacovelli, Francesco, Foffa, Stefano, Muttoni, Niccolò, Maggiore, Michele
Joint gravitational-wave and $\gamma$-ray bursts (GRB) observations are among the best prospects for standard siren cosmology. However, the strong selection effect for the coincident GRB detection, which is possible only for sources with small inclin
Externí odkaz:
http://arxiv.org/abs/2405.02286
Autor:
Santoliquido, Filippo, Dupletsa, Ulyana, Tissino, Jacopo, Branchesi, Marica, Iacovelli, Francesco, Iorio, Giuliano, Mapelli, Michela, Gerosa, Davide, Harms, Jan, Pasquato, Mario
Publikováno v:
A&A 690, A362 (2024)
Third-generation (3G) gravitational-wave detectors such as the Einstein Telescope (ET) will observe binary black hole (BBH) mergers at redshifts up to $z\sim 100$. However, an unequivocal determination of the origin of high-redshift sources will rema
Externí odkaz:
http://arxiv.org/abs/2404.10048