Zobrazeno 1 - 10
of 1 339
pro vyhledávání: '"Hunter, C. J."'
Publikováno v:
The Modern Language Review, 1986 Jan 01. 81(1), 162-164.
Externí odkaz:
https://www.jstor.org/stable/3728780
Autor:
Tallack, Douglas
Publikováno v:
The Review of English Studies, 1982 Aug 01. 33(131), 363-365.
Externí odkaz:
https://www.jstor.org/stable/515650
Autor:
Osborne, John
Publikováno v:
The Modern Language Review, 1979 Apr 01. 74(2), 403-404.
Externí odkaz:
https://www.jstor.org/stable/3727804
Autor:
Colomb, Gregory G.
Publikováno v:
The Modern Language Review, 1983 Oct 01. 78(4), 885-886.
Externí odkaz:
https://www.jstor.org/stable/3729504
Autor:
Thomson, Peter
Publikováno v:
The Modern Language Review, 1981 Apr 01. 76(2), 455-456.
Externí odkaz:
https://www.jstor.org/stable/3726447
Publikováno v:
Phys.Rev.D59:064005,1999
In asymptotically flat space a rotating black hole cannot be in thermodynamic equilibrium because the thermal radiation would have to be co-rotating faster than light far from the black hole. However in asymptotically anti-de Sitter space such equili
Externí odkaz:
http://arxiv.org/abs/hep-th/9811056
Publikováno v:
Phys.Rev.D59:044033,1999
It has been proposed that spacetimes with a U(1) isometry group have contributions to the entropy from Misner strings as well as from the area of $d-2$ dimensional fixed point sets. In this paper we test this proposal by constructing Taub-Nut-AdS and
Externí odkaz:
http://arxiv.org/abs/hep-th/9809035
Autor:
Hawking, S. W., Hunter, C. J.
Publikováno v:
Phys.Rev. D59 (1999) 044025
The underlying reason for the existence of gravitational entropy is traced to the impossibility of foliating topologically non-trivial Euclidean spacetimes with a time function to give a unitary Hamiltonian evolution. In $d$ dimensions the entropy ca
Externí odkaz:
http://arxiv.org/abs/hep-th/9808085
Autor:
Hunter, C. J.
Publikováno v:
Phys.Rev. D59 (1999) 024009
We examine the effect of a non-trivial nut charge on the action of non-compact four-dimensional instantons with a U(1) isometry. If the instanton action is calculated by dimensionally reducing along the isometry, then the nut charge is found to make
Externí odkaz:
http://arxiv.org/abs/gr-qc/9807010
Autor:
Hawking, S. W., Hunter, C. J.
Publikováno v:
Class.Quant.Grav.13:2735-2752,1996
This paper generalizes earlier work on Hamiltonian boundary terms by omitting the requirement that the spacelike hypersurfaces $\Sigma_t$ intersect the timelike boundary $\cal B$ orthogonally. The expressions for the action and Hamiltonian are calcul
Externí odkaz:
http://arxiv.org/abs/gr-qc/9603050