Zobrazeno 1 - 8
of 8
pro vyhledávání: '"José A. Jiménez Madrid"'
Autor:
Jordi Isern-Fontanet, Emilio García-Ladona, José Antonio Jiménez-Madrid, Estrella Olmedo, Marcos García-Sotillo, Alejandro Orfila, Antonio Turiel
Publikováno v:
Remote Sensing, Vol 12, Iss 4, p 724 (2020)
Surface currents in the Alboran Sea are characterized by a very fast evolution that is not well captured by altimetric maps due to sampling limitations. On the contrary, satellite infrared measurements provide high resolution synoptic images of the o
Externí odkaz:
https://doaj.org/article/c3576394b47848fcb8f91b31bf3438a7
Autor:
Oriol Sánchez, Emilio García-Ladona, Pedro Elosegui, Josep Lluís Pelegrí, J. Ballabrera, Jordi Font, Joaquim Salvador, Jordi Isern-Fontanet, Pere Fernandez, José A. Jiménez Madrid, Fernando Rull Pérez, Jordi Salat
Publikováno v:
Scientia Marina; Vol. 80 No. S1 (2016); 141-158
Scientia Marina; Vol. 80 Núm. S1 (2016); 141-158
Scientia Marina
Consejo Superior de Investigaciones Científicas (CSIC)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Scientia Marina, Vol 80, Iss S1, Pp 141-158 (2016)
Scientia Marina; Vol. 80 Núm. S1 (2016); 141-158
Scientia Marina
Consejo Superior de Investigaciones Científicas (CSIC)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Scientia Marina, Vol 80, Iss S1, Pp 141-158 (2016)
Special volume: Planet Ocean. Scientia Marina 80(Suppl.1) 2016.-- 18 pages, 22 figures, 1 table
[EN] Since the mid-1980s, physical oceanographers at the Institute of Marine Sciences have been involved in the use of Lagrangian drifters as a compl
[EN] Since the mid-1980s, physical oceanographers at the Institute of Marine Sciences have been involved in the use of Lagrangian drifters as a compl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9443849a4d98fb9559b0a4408e6b568a
http://hdl.handle.net/10261/138198
http://hdl.handle.net/10261/138198
Autor:
José A. Jiménez Madrid
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
This Letter deals with the study of the accretion of a generalized Chaplygin gas with equation of state p=-A/ρα onto wormholes. We have obtained that when dominant energy condition is violated the size of wormhole increases with the scale factor up
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
10 pags., 5 figs. -- PACS: 04.60.-m; 98.80.Cq
Primordial inflation is regarded to be driven by a phantom field which is here implemented as a scalar field satisfying an equation of state p=ωρ, with ω
This work wassupported by DGICYT unde
Primordial inflation is regarded to be driven by a phantom field which is here implemented as a scalar field satisfying an equation of state p=ωρ, with ω
This work wassupported by DGICYT unde
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
The Babichev-Dokuchaev-Eroshenko model for the accretion of dark energy onto black holes has been extended to deal with black holes with non-static metrics. The possibility that for an asymptotic observer a black hole with large mass will rapidly inc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7689d66c898eadcf99b66171d4e23c4d
This paper deals with the study of the accretion of dark energy with equation of state $p=w\rho$ onto Kerr-Newman black holes. We have obtained that when $w>-1$ the mass and specific angular momentum increase, and that whereas the specific angular mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::99868cbf09471a96c35a11931416f502
http://arxiv.org/abs/astro-ph/0510051
http://arxiv.org/abs/astro-ph/0510051
This paper deals with a study of the cylindrically symmetric accretion of dark energy with equation of state $p=w��$ onto wiggly straight cosmic strings. We have obtained that when $w>-1$ the linear energy density in the string core gradually inc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4eb527bd50083acdb2dabb76fe9aba36
http://arxiv.org/abs/astro-ph/0506717
http://arxiv.org/abs/astro-ph/0506717
Publikováno v:
Journal of Cosmology and Astroparticle Physics. 2005:005-005
We discuss dark energy models which might describe effectively the actual acceleration of the universe. More precisely, for a 4-dimensional Friedmann-Lema\^{\i}tre-Robertson-Walker (FLRW) universe we consider two situations: First of them, we model d