Zobrazeno 1 - 10
of 62
pro vyhledávání: '"Boco, Lumen"'
Autor:
Gabrielli, Francesco, Boco, Lumen, Ghirlanda, Giancarlo, Salafia, Om Sharan, Salvaterra, Ruben, Spera, Mario, Lapi, Andrea
The stellar initial-mass function (IMF) represents a fundamental quantity in astrophysics and cosmology, describing the mass distribution of stars from low to very-high masses. It is intimately linked to a wide variety of topics, including stellar an
Externí odkaz:
http://arxiv.org/abs/2409.09118
Autor:
Gabrielli, Francesco, Lapi, Andrea, Boco, Lumen, Ugolini, Cristiano, Costa, Guglielmo, Sgalletta, Cecilia, Shepherd, Kendall, Di Carlo, Ugo N., Bressan, Alessandro, Limongi, Marco, Spera, Mario
Pair-instability supernovae (PISNe) have crucial implications for many astrophysical topics, including the search for very massive stars, the black hole mass spectrum, and galaxy chemical enrichment. To this end, we need to understand where PISNe are
Externí odkaz:
http://arxiv.org/abs/2408.16823
We devise and exploit a data-driven, semi-empirical framework of galaxy formation and evolution, coupling it to recipes for planet formation from stellar and planetary science, to compute the cosmic planet formation rate, and the properties of the pl
Externí odkaz:
http://arxiv.org/abs/2408.08611
Autor:
Fu, Hao, Shankar, Francesco, Ayromlou, Mohammadreza, Koutsouridou, Ioanna, Cattaneo, Andrea, Bertemes, Caroline, Bellstedt, Sabine, Martín-Navarro, Ignacio, Leja, Joel, Allevato, Viola, Bernardi, Mariangela, Boco, Lumen, Dimauro, Paola, Gruppioni, Carlotta, Lapi, Andrea, Menci, Nicola, Rodríguez, Iván Muñoz, Puglisi, Annagrazia, Alonso-Tetilla, Alba V.
In a hierarchical, dark matter-dominated Universe, stellar mass functions (SMFs), galaxy merger rates, star formation histories (SFHs), satellite abundances, and intracluster light, should all be intimately connected observables. However, the systema
Externí odkaz:
http://arxiv.org/abs/2406.07605
Autor:
Ronconi, Tommaso, Lapi, Andrea, Torsello, Martina, Bressan, Alessandro, Donevski, Darko, Pantoni, Lara, Behiri, Meriem, Boco, Lumen, Cimatti, Andrea, D'Amato, Quirino, Danese, Luigi, Giulietti, Marika, Perrotta, Francesca, Silva, Laura, Talia, Margherita, Massardi, Marcella
Publikováno v:
A&A 685, A161 (2024)
Fostered by upcoming data from new generation observational campaigns, we are about to enter a new era for the study of how galaxies form and evolve. The unprecedented quantity of data that will be collected, from distances only marginally grasped up
Externí odkaz:
http://arxiv.org/abs/2402.12427
Autor:
Lapi, Andrea, Boco, Lumen, Cueli, Marcos M., Haridasu, Balakrishna S., Ronconi, Tommaso, Baccigalupi, Carlo, Danese, Luigi
[abridged] We propose a model of the Universe (dubbed $\eta$CDM) featuring a stochastic evolution of the cosmological quantities, that is meant to render small deviations from homogeneity/isotropy on scales of $30-50\, h^{-1}$ Mpc at late cosmic time
Externí odkaz:
http://arxiv.org/abs/2310.06028
In recent years, increasing attention has been devoted to semi empirical, data-driven models to tackle some aspects of the complex and still largely debated topic of galaxy formation and evolution. We here present a new semi empirical model whose mar
Externí odkaz:
http://arxiv.org/abs/2307.13036
Autor:
Sgalletta, Cecilia, Iorio, Giuliano, Mapelli, Michela, Artale, M. Celeste, Boco, Lumen, Chattopadhyay, Debatri, Lapi, Andrea, Possenti, Andrea, Rinaldi, Stefano, Spera, Mario
Galactic binary neutron stars (BNSs) are a unique laboratory to probe the evolution of BNSs and their progenitors. Here, we use a new version of the population synthesis code SEVN to evolve the population of Galactic BNSs, by modeling the spin up and
Externí odkaz:
http://arxiv.org/abs/2305.04955
Many recent works have shown that the angular resolution of ground-based detectors is too poor to characterize the anisotropies of the stochastic gravitational-wave background (SGWB). For this reason, we asked ourselves if a constellation of space-ba
Externí odkaz:
http://arxiv.org/abs/2212.06162
Autor:
Fu, Hao, Shankar, Francesco, Ayromlou, Mohammadreza, Dickson, Max, Koutsouridou, Ioanna, Rosas-Guevara, Yetli, Marsden, Christopher, Brocklebank, Kristina, Bernardi, Mariangela, Shiamtanis, Nikolaos, Williams, Joseph, Zanisi, Lorenzo, Allevato, Viola, Boco, Lumen, Bonoli, Silvia, Cattaneo, Andrea, Dimauro, Paola, Jiang, Fangzhou, Lapi, Andrea, Menci, Nicola, Petropoulou, Stefani, Villforth, Carolin
The relative roles of mergers and star formation in regulating galaxy growth are still a matter of intense debate. We here present our DECODE, a new Discrete statistical sEmi-empiriCal mODEl specifically designed to predict rapidly and efficiently, i
Externí odkaz:
http://arxiv.org/abs/2208.00014