Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Estels de neutrons"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 512(4), 5269-5277. Oxford University Press
Transitional millisecond pulsars (tMSPs) have emerged in the last decade as a unique class of neutron stars at the crossroads between accretion- and rotation-powered phenomena. In their (sub-luminous) accretion disk state, with X-ray luminosities of
Autor:
F. M. Vincentelli, J. Neilsen, A. J. Tetarenko, Y. Cavecchi, N. Castro Segura, S. del Palacio, J. van den Eijnden, G. Vasilopoulos, D. Altamirano, M. Armas Padilla, C. D. Bailyn, T. Belloni, D. J. K. Buisson, V. A. Cúneo, N. Degenaar, C. Knigge, K. S. Long, F. Jiménez-Ibarra, J. Milburn, T. Muñoz Darias, M. Özbey Arabacı, R. Remillard, T. Russell
Accretion disks around compact objects are expected to enter an unstable phase at high luminosity. One instability may occur when the radiation pressure generated by accretion modifies the disk viscosity, resulting in the cyclic depletion and refilli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0cbde99a5ba53c3a1e4148acf451f3f5
https://eprints.soton.ac.uk/476105/
https://eprints.soton.ac.uk/476105/
Autor:
Arnau Rios
Bayesian history matching is a statistical tool used to calibrate complex numerical models. Now, it has been applied to first-principles simulations of several nuclei, including 208 Pb, whose properties are linked to the interior of neutron stars
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::59f1447f37b891e74251653bddce6c4f
http://hdl.handle.net/2445/197007
http://hdl.handle.net/2445/197007
Autor:
Xifra Goya, Georgina
Publikováno v:
Dipòsit Digital de la UB
Universidad de Barcelona
Universidad de Barcelona
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutora: Àngels Ramos Gómez
We study how the presence of bosonic self-interacting dark matter influences the properties of admixed neutron stars. We
We study how the presence of bosonic self-interacting dark matter influences the properties of admixed neutron stars. We
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::988d8e4788b49aca76911bd151c832c9
http://hdl.handle.net/2445/189040
http://hdl.handle.net/2445/189040
Autor:
Nadal Matosas, Adriana
Publikováno v:
Dipòsit Digital de la UB
Universidad de Barcelona
Universidad de Barcelona
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutor: Arnau Rios Huguet
In the era of gravitational waves detection, the need to understand matter at finite temperature has arisen. The thermal inde
In the era of gravitational waves detection, the need to understand matter at finite temperature has arisen. The thermal inde
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::3b312f6f677c4278d769ab1e51c943e5
http://hdl.handle.net/2445/188747
http://hdl.handle.net/2445/188747
Publikováno v:
Dipòsit Digital de la UB
Universidad de Barcelona
Digital.CSIC. Repositorio Institucional del CSIC
instname
Universidad de Barcelona
Digital.CSIC. Repositorio Institucional del CSIC
instname
Several supersonic runaway pulsar wind nebulae (sPWNe) with jet-like extended structures have been recently discovered in X-rays. If these structures are the product of electrons escaping the system and diffusing into the surrounding interstellar med
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c7743c4d0beb38f4f01c1a2b003f89b5
http://arxiv.org/abs/2109.00320
http://arxiv.org/abs/2109.00320
Autor:
Gómez Subils, Javier
Publikováno v:
TDX (Tesis Doctorals en Xarxa)
TDR: Tesis Doctorales en Red
CBUC, CESCA
TDR. Tesis Doctorales en Red
instname
Dipòsit Digital de la UB
Universidad de Barcelona
TDR: Tesis Doctorales en Red
CBUC, CESCA
TDR. Tesis Doctorales en Red
instname
Dipòsit Digital de la UB
Universidad de Barcelona
[eng] In this thesis we have employed the holographic duality to study the non-perturbative regime of a one-parameter family of theories with multi-scale dynamics. Normally, this (super)string theory motivated duality identifies gauge theories in fla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::4d17f35c7b1e0517d165dcdb8de402cb
http://hdl.handle.net/2445/179465
http://hdl.handle.net/2445/179465
Autor:
Gimeno Estivill, Patrícia
Publikováno v:
Dipòsit Digital de la UB
Universidad de Barcelona
Universidad de Barcelona
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutora: Àngels Ramos Gomez
On the basis of a simple model for the energy of nuclear matter, we parametrize different equations of state within the c
On the basis of a simple model for the energy of nuclear matter, we parametrize different equations of state within the c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::848154638f6df44f24a74e107fe39988
http://hdl.handle.net/2445/180306
http://hdl.handle.net/2445/180306
Publikováno v:
Dipòsit Digital de la UB
Universidad de Barcelona
Symmetry
Symmetry, 2021, 13 (9), pp.1613. ⟨10.3390/sym13091613⟩
Volume 13
Issue 9
Symmetry, Vol 13, Iss 1613, p 1613 (2021)
Universidad de Barcelona
Symmetry
Symmetry, 2021, 13 (9), pp.1613. ⟨10.3390/sym13091613⟩
Volume 13
Issue 9
Symmetry, Vol 13, Iss 1613, p 1613 (2021)
The most popular Gogny parametrizations, namely D1S, D1N and D1M, describe accurately the ground-state properties of spherical and deformed finite nuclei all across the mass table obtained with Hartree--Fock--Bogoliubov (HFB) calculations. However, t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9739245aa3aca21297677a75d90e93fd
http://hdl.handle.net/2445/184236
http://hdl.handle.net/2445/184236
Autor:
Tort Vives, Gerard
Publikováno v:
Dipòsit Digital de la UB
Universidad de Barcelona
Universidad de Barcelona
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutor: Arnau Rios Huguet
Neutron star cores reach high values of density where nuclear matter can interact via weakly short range forces. We consider
Neutron star cores reach high values of density where nuclear matter can interact via weakly short range forces. We consider
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::16f6d022d2b3f4016b0a65553373e08c
http://hdl.handle.net/2445/180966
http://hdl.handle.net/2445/180966