Zobrazeno 1 - 10
of 183
pro vyhledávání: '"Miralles, Juan A."'
A generic characteristic of self-graviting systems is that they have a negative heat capacity. An important example of this behaviour is given by the Schwarzschild black hole. The case of charged and rotating black holes is even more interesting, sin
Externí odkaz:
http://arxiv.org/abs/2407.10885
We study the coupling of the force-free magnetosphere to the long-term internal evolution of a magnetar. We allow the relation between the poloidal and toroidal stream functions - that characterizes the magnetosphere - to evolve freely without constr
Externí odkaz:
http://arxiv.org/abs/1807.09021
We extend our previous study of equilibrium solutions of non-rotating force-free magnetospheres of neutron stars. We show that multiple solutions exist for the same sets of parameters, implying that the solutions are degenerate. We are able to obtain
Externí odkaz:
http://arxiv.org/abs/1709.10044
We study the long-term quasi-steady evolution of the force-free magnetosphere of a magnetar coupled to its internal magnetic field. We find that magnetospheric currents can be maintained on long timescales of the order of thousands of years. Meanwhil
Externí odkaz:
http://arxiv.org/abs/1706.07990
We revisit the various approximations employed to study the long-term evolution of the magnetic field in neutron star cores and discuss their limitations and possible improvements. A recent controversy on the correct form of the induction equation an
Externí odkaz:
http://arxiv.org/abs/1704.02016
We study ambipolar diffusion in strongly magnetised neutron stars, with special focus on the effects of neutrino reaction rates and the impact of a superfluid/superconducting transition in the neutron star core. For axisymmetric magnetic field config
Externí odkaz:
http://arxiv.org/abs/1608.00001
We present a detailed analysis of the properties of twisted, force-free magnetospheres of non-rotating neutron stars, which are of interest in the modelling of magnetar properties and evolution. In our models the magnetic field smoothly matches to a
Externí odkaz:
http://arxiv.org/abs/1605.02253
Autor:
Torrego, Alfons, Mena, Alicia Habernau, Viña, Antolín López, Arrondo, Antonio Parra, Crespo, Astrid, Santana, Aythamy Henrquez, Cisneros, Carolina, Picado, César, Domingo, Cristian, Antolin, Dario, Álvarez, Francisco, Soto, Gregorio, Ercoreca, Ignacio Antepara, Ojanguren, Íñigo, Bobolea, Irina, Urrutia, Isabel, Moguel, Ismael García, Dominguez, Joaquín Sastre, Rivera, José María Olaguibel, Chicote, José María Vega, Serrano, José, Miralles, Juan Carlos, Romero, Julio Delgado, Prado, Manuel Jorge Rial, Mosteiro, Mar, Blanco, Marina, Perpiñá, Miguel, Mozo, Paloma Campo, Sanz, Pilar Barranco, Contreras, Remedios Cardenas, Gancedo, Santiago Quirce, De Cabrës, Valentina Gutiérrez Vall, Plaza, Vicente, Gallardo, Victoria García, Muñoz, Xavi, Pérez de Llano, Luis, Dávila, Ignacio, Martínez-Moragón, Eva, Domínguez-Ortega, Javier, Almonacid, Carlos, Colás, Carlos, García-Rivero, Juan Luis, Carmona, Loreto, García de Yébenes, María Jesús, Cosío, Borja G.
Publikováno v:
In The Journal of Allergy and Clinical Immunology: In Practice July 2021 9(7):2725-2731
Autor:
Rea, Nanda, Gullon, Miguel, Pons, Jose' A., Perna, Rosalba, Dainotti, Maria G., Miralles, Juan A., Torres, Diego F.
A large fraction of Gamma Ray Bursts (GRBs) displays an X-ray plateau phase within <10^{5} s from the prompt emission, proposed to be powered by the spin-down energy of a rapidly spinning newly born magnetar. In this work we use the properties of the
Externí odkaz:
http://arxiv.org/abs/1510.01430
Autor:
Ibáñez, José-María, Cordero-Carrión, Isabel, Aloy, Miguel-Ángel, Martí, José-María, Miralles, Juan-Antonio
We analyze the influence of the magnetic field in the convexity properties of the relativistic magnetohydrodynamics system of equations. To this purpose we use the approach of Lax, based on the analysis of the linearly degenerate/genuinely non-linear
Externí odkaz:
http://arxiv.org/abs/1503.00978