Zobrazeno 1 - 10
of 28
pro vyhledávání: '"C. Gonzalez-Boquera"'
Publikováno v:
Physics Letters B, Vol 803, Iss , Pp - (2020)
A set of equations of state obtained from finite-range Gogny forces and momentum-dependent interactions is used to investigate the recent observation of gravitational waves from the binary neutron star merger GW170817 event. For this set of interacti
Externí odkaz:
https://doaj.org/article/2210ae1f8ec34fc9b9a6845f256d400e
Publikováno v:
Physics Letters B, Vol 779, Iss , Pp 195-200 (2018)
The D1 family of parametrizations of the Gogny interaction commonly suffers from a rather soft neutron matter equation of state that leads to maximal masses of neutron stars well below the observational value of two solar masses. We propose a reparam
Externí odkaz:
https://doaj.org/article/cbe1982c695841e4a2c99b986a039adb
Publikováno v:
Physical Review C. 103
It has been recently shown that some Gogny finite-range interactions suffer from finite-size instabilities in coordinate-space calculations [Eur. Phys. J. A 55, 150 (2019)]. We confirm this finding by using the Hartree-Fock (HF) method in the quasilo
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
Publikováno v:
Physics Letters B, Vol 779, Iss, Pp 195-200 (2018)
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Physics Letters B
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Physics Letters B
The D1 family of parametrizations of the Gogny interaction commonly suffers from a rather soft neutron matter equation of state that leads to maximal masses of neutron stars well below the observational value of two solar masses. We propose a reparam
Publikováno v:
Physical Review C. 100
The properties of the core-crust transition in neutron stars are investigated using effective nuclear forces of finite range. Special attention is paid to the so-called dynamical method for locating the transition point, which, apart from the stabili
We analyze the effects of including $\Delta(1232)$ isobars in an equation of state (EoS) for cold, $\beta$-stable neutron star matter, employing relativistic nuclear mean field theory. The selected EoS reproduces the properties of nuclear matter and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ca468a83d1c93c75f2d373dc3cc213c
http://arxiv.org/abs/1907.08583
http://arxiv.org/abs/1907.08583
Publikováno v:
Biblos-e Archivo: Repositorio Institucional de la UAM
Universidad Autónoma de Madrid
Acta Physica Polonica B Proceedings Supplement, ISSN 1899-2358, 2019, Vol. 12, No. 3
Archivo Digital UPM
Universidad Politécnica de Madrid
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Universidad Autónoma de Madrid
Acta Physica Polonica B Proceedings Supplement, ISSN 1899-2358, 2019, Vol. 12, No. 3
Archivo Digital UPM
Universidad Politécnica de Madrid
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
The symmetry energy of the D1 family of Gogny interactions, which describe finite nuclei properties in good agreement with experimental data, shows too soft a behaviour above saturation density. As a consequence, the D1 family of Gogny forces often c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3f69601e3452d3de03630cab174ea61
https://hdl.handle.net/10486/691423
https://hdl.handle.net/10486/691423
Publikováno v:
Springer Proceedings in Physics ISBN: 9783030222031
We propose a new Gogny parametrization, which we call D1M\(^{*}\), aimed to be successful in the study of the properties of neutron stars and, at the same time, to describe finite nuclei with a similar quality as the D1M Gogny interaction. D1M\(^{*}\
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8cb610629ada350b4d0dc7713a045158
https://doi.org/10.1007/978-3-030-22204-8_26
https://doi.org/10.1007/978-3-030-22204-8_26
Autor:
X. Viñas, M. Bhuyan, Mariana Dutra, C. Gonzalez-Boquera, Odilon Lourenço, M. Centelles, C. H. Lenzi
Publikováno v:
Physics Letters B, Vol 803, Iss, Pp-(2020)
Dipòsit Digital de la UB
Universidad de Barcelona
Physics Letters
Dipòsit Digital de la UB
Universidad de Barcelona
Physics Letters
A set of equations of state obtained from finite-range Gogny forces and momentum-dependent interactions is used to investigate the recent observation of gravitational waves from the binary neutron star merger GW170817 event. For this set of interacti