Zobrazeno 1 - 10
of 146
pro vyhledávání: '"Bosch, Pablo"'
Autor:
Curtis, Sanjana, Bosch, Pablo, Mösta, Philipp, Radice, David, Bernuzzi, Sebastiano, Perego, Albino, Haas, Roland, Schnetter, Erik
We present a 3D general-relativistic magnetohydrodynamic simulation of a short-lived neutron star remnant formed in the aftermath of a binary neutron star merger. The simulation uses an M1 neutrino transport scheme to track neutrino-matter interactio
Externí odkaz:
http://arxiv.org/abs/2305.07738
The origin of short gamma-ray bursts (sGRBs) is associated with outflows powered by the remnant of a binary neutron star merger. This remnant can be either a black hole or a highly magnetized, fastly spinning neutron star, also known as a magnetar. H
Externí odkaz:
http://arxiv.org/abs/2209.07514
We investigate the influence of parametric magnetic field configurations of a hypermassive neutron star (HMNS) on electromagnetic (EM) observables, specifically the kilonova lightcurves and nucleosynthesis yields. We perform three-dimensional (3D) dy
Externí odkaz:
http://arxiv.org/abs/2208.05330
Publikováno v:
Phys. Rev. D 105, 064046 (2022)
Gravitational-wave observations of black hole ringdowns are commonly used to characterize binary merger remnants and to test general relativity. These analyses assume linear black hole perturbation theory, in particular that the ringdown can be descr
Externí odkaz:
http://arxiv.org/abs/2112.11168
Autor:
Cheng, Li-Hsin, Bosch, Pablo B. J., Hofman, Rutger F. H., Brakenhoff, Timo B., Bruggemans, Eline F., van der Geest, Rob J., Holman, Eduard R.
Background. With the rise of highly portable, wireless, and low-cost ultrasound devices and automatic ultrasound acquisition techniques, an automated interpretation method requiring only a limited set of views as input could make preliminary cardiova
Externí odkaz:
http://arxiv.org/abs/2110.12915
Publikováno v:
Phys. Rev. D 102, 044014 (2020)
We study the dynamics of unstable Reissner-Nordstr\"om anti-de Sitter black holes under charged scalar field perturbations in spherical symmetry. We unravel their general behavior and approach to the final equlibrium state. In the first part of this
Externí odkaz:
http://arxiv.org/abs/1912.05598
Autor:
Ley Bosch, Pablo1 (AUTHOR), de Castro González, Óscar1 (AUTHOR), García Sánchez, Francisco2 (AUTHOR) franciscojose.garcia@unican.es
Publikováno v:
Environment, Development & Sustainability. Apr2024, Vol. 26 Issue 4, p10765-10785. 21p.
Autor:
Ebel, Francisca A., Liaudat, Ana C., Blois, Damián A., Capella, Virginia, Broglia, Martin F., Barbero, Cesar A., Rodríguez, Nancy, Bosch, Pablo, Rivarola, Claudia R.
Publikováno v:
In Colloids and Surfaces B: Biointerfaces November 2023 231
In holographic applications one can encounter scenarios where a long-wavelength instability can arise. In such situations, it is often the case that the dynamical end point of the instability is a new equilibrium phase with a nonlinear scalar hair co
Externí odkaz:
http://arxiv.org/abs/1704.05454
Publikováno v:
Phys. Rev. Lett. 116, 141102 (2016)
We describe the full nonlinear development of the superradiant instability for a charged massless scalar field, coupled to general relativity and electromagnetism, in the vicinity of a Reissner-Nordstrom-AdS black hole. The presence of the negative c
Externí odkaz:
http://arxiv.org/abs/1601.01384