Zobrazeno 1 - 10
of 192
pro vyhledávání: '"Feo, Alessandra"'
The contamination impact and the migration of the contaminant into the surrounding environment due to the presence of a spilled oil pipeline will cause significant damage to the natural ecosystem. For this reason, it is decisive to develop a rapid re
Externí odkaz:
http://arxiv.org/abs/2211.01279
Autor:
Feo, Alessandra, Celico, Fulvio
Publikováno v:
PLoS ONE 2022; 17(4): e0266486
Numerical modeling of the migration of three-phase immiscible fluid flow in variably saturated zones is challenging due to the different behavior of the system between unsaturated and saturated zones. This behavior results in the use of different num
Externí odkaz:
http://arxiv.org/abs/2112.14229
Autor:
De Feo, Alessandra1 (AUTHOR) alessandra.defeo@ior.it, Manfredi, Marcello2 (AUTHOR) marcello.manfredi@uniupo.it, Mancarella, Caterina1 (AUTHOR) caterina.mancarella@ior.it, Maqueda, Joaquín J.1 (AUTHOR) joaquin.juradomaqueda@ior.it, De Giorgis, Veronica2 (AUTHOR) veronica.degiorgis@uniupo.it, Pignochino, Ymera3,4 (AUTHOR) ymera.pignochino@ircc.it, Sciandra, Marika1 (AUTHOR) marika.sciandra@ior.it, Cristalli, Camilla1 (AUTHOR) camilla.cristalli@ior.it, Donadelli, Massimo5 (AUTHOR) massimo.donadelli@univr.it, Scotlandi, Katia1 (AUTHOR) massimo.donadelli@univr.it
Publikováno v:
International Journal of Molecular Sciences. Feb2024, Vol. 25 Issue 3, p1588. 19p.
Akademický článek
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Autor:
De Pietri, Roberto, Feo, Alessandra, Font, José A., Löffler, Frank, Pasquali, Michele, Stergioulas, Nikolaos
Publikováno v:
Phys. Rev. D 101, 064052 (2020)
We analyze the properties of the gravitational wave signal emitted after the merger of a binary neutron star system when the remnant survives for more than a 80 ms (and up to 140ms). We employ four different piecewise polytropic equations of state su
Externí odkaz:
http://arxiv.org/abs/1910.04036
Autor:
De Pietri, Roberto, Drago, Alessandro, Feo, Alessandra, Pagliara, Giuseppe, Pasquali, Michele, Traversi, Silvia, Wiktorowicz, Grzegorz
We analyse the phenomenological implications of the two-families scenario on the merger of compact stars. That scenario is based on the coexistence of both hadronic stars and strange quark stars. After discussing the classification of the possible me
Externí odkaz:
http://arxiv.org/abs/1904.01545
Autor:
De Pietri, Roberto, Feo, Alessandra, Font, José A., Löffler, Frank, Maione, Francesco, Pasquali, Michele, Stergioulas, Nikolaos
Publikováno v:
Phys. Rev. Lett. 120, 221101 (2018)
We present the first very long-term simulations (extending up to ~140 ms after merger) of binary neutron star mergers with piecewise polytropic equations of state and in full general relativity. Our simulations reveal that at a time of 30-50 ms after
Externí odkaz:
http://arxiv.org/abs/1802.03288
Publikováno v:
Phys. Rev. D 96, 063011 (2017)
In this work we analyze the gravitational wave signal from hypermassive neutron stars formed after the merger of binary neutron star systems, focusing on its spectral features. The gravitational wave signals are extracted from numerical relativity si
Externí odkaz:
http://arxiv.org/abs/1707.03368
Akademický článek
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We present a study of the merger of six different known galactic systems of binary neutron stars (BNS) of unequal mass with a mass ratio between $0.75$ and $0.99$. Specifically, these systems are J1756-2251, J0737-3039A, J1906+0746, B1534+12, J0453+1
Externí odkaz:
http://arxiv.org/abs/1608.02810