From aptm@kharkov.ua Tue Jan 25 15:15:00 2000 Return-Path: Received: from ktts.kharkov.ua (root@ktts.kharkov.ua [193.124.57.65]) by xray.sai.msu.su (8.9.3/8.9.3) with ESMTP id PAA13656 for ; Tue, 25 Jan 2000 15:12:10 +0300 Received: from aptm (ppp-2.ktts.kharkov.ua [194.44.3.3]) by ktts.kharkov.ua (8.9.3/8.9.3) with SMTP id NAA24659 for ; Tue, 25 Jan 2000 13:53:04 +0200 (EET) Message-ID: <001901bf672a$829d56a0$03032cc2@kharkov.ua> From: "O.B.Zaslavskii" To: Subject: black holes Date: Mon, 24 Jan 2000 22:54:32 +0200 Organization: The Tarielle Station MIME-Version: 1.0 Content-Type: multipart/mixed; boundary="----=_NextPart_000_001B_01BF66BD.FA7E5A60" X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.00.2615.200 X-MimeOLE: Produced By Microsoft MimeOLE V5.00.2615.200 Status: R This is a multi-part message in MIME format. ------=_NextPart_000_001B_01BF66BD.FA7E5A60 Content-Type: text/plain; charset="koi8-r" Content-Transfer-Encoding: 7bit Please find enclosed the attached file with the abstract of my talk which I suggest for the colloquium on black holes (3 March). It is based on my two recent papers hep-th/9911077 (Phys. Rev. D, in press) and hep-th/ 0001090 (accepted in Phys. Lett. B). I would greatly appreciate you for financial support including travel since in our situation any support (and even salary) are now absent in our Kharkov University, so such a support is the only chance for me to participate in the meeting. Sincerely, Oleg Zaslavskii, Department of Physics, Kharkov Karazin's National university, Svoboda Square 4, Kharkov 61077, Ukraine ------=_NextPart_000_001B_01BF66BD.FA7E5A60 Content-Type: application/octet-stream; name="abstract.tex" Content-Transfer-Encoding: quoted-printable Content-Disposition: attachment; filename="abstract.tex" %%% = =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D %%% @LaTeX-file{ %%% filename =3D "template.aps", %%% version =3D "3.0", %%% date =3D "November 10, 1992", %%% ISO-date =3D "1992.11.10", %%% time =3D "15:41:54.18 EST", %%% author =3D "American Physical Society", %%% contact =3D "Christopher B. Hamlin", %%% address =3D "APS Publications Liaison Office %%% 500 Sunnyside Blvd. %%% Woodbury, NY 11797", %%% telephone =3D "(516) 576-2390", %%% FAX =3D "(516) 349-7817", %%% email =3D "mis@aps.org (Internet)", %%% supported =3D "yes", %%% archived =3D "pinet.aip.org/pub/revtex, %%% Niord.SHSU.edu:[FILESERV.REVTEX]", %%% keywords =3D "REVTeX, version 3.0, template, %%% American Physical Society", %%% codetable =3D "ISO/ASCII", %%% checksum =3D "20084 100 485 3540", %%% docstring =3D "This is the Americal Physical Society %%% template for creating a manuscript under %%% REVTeX 3.0 (release of November 10, 1992). %%% The checksum field above contains a CRC-16 %%% checksum as the first value, followed by the %%% equivalent of the standard UNIX wc (word %%% count) utility output of lines, words, and %%% characters. This is produced by Robert %%% Solovay's checksum utility." %%% } %%% = =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D % ****** Start of file template.aps ****** % % This file is part of the APS files in the REVTeX 3.0 distribution. % Version 3.0 of REVTeX, November 10, 1992. % Copyright (c) 1992 The American Physical Society. % See the REVTeX 3.0 README file for restrictions and more = information. % This is a template for producing files for use with REVTEX 3.0. % Copy this file to another name and then work on that file. % That way, you always have this original template file to use. \documentstyle[aps,12pt]{revtex} %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%= %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% %TCIDATA{Created=3DMon Feb 16 15:48:48 1998} %TCIDATA{LastRevised=3DMon Jan 24 22:47:16 2000} \begin{document} \draft \author{O. B. Zaslavskii} \address{Department of Physics, Kharkov Karazin's National University, = Svoboda Sq.4,\\ Kharkov\\ 61077, Ukraine\\ E-mail: aptm@kharkov.ua} \title{Dilaton gravity and black holes with finite curvature at the = horizon away from the Hawking temperature} \maketitle \begin{abstract} % insert abstract here \end{abstract} \pacs{} %\date{\today} It is shown that static solutions with a finite curvature at the horizon = may exist in dilaton gravity at temperatures $T\neq T_{H}$ (including = $T=3D0$) where $T_{H}\,$is the Hawking temperature. Hawking radiation is absent = and the state of a system represents thermal excitation over the Boulware vacuum. The horizon remains unattainable for an observer because of the thermal divergences in the stress-energy of quantum fields there. = However, the curvature at the horizon is finite, when measured from outside, = since these divergences are compensated by those in the gradients of the = dilaton field. The Spacetimes under consideration are geodesically incomplete = and the coupling between the dilaton and gravity diverges at the horizon, so = we have a ''singularity without singularity''. % \draft command makes pacs numbers print % repeat the \author\address pair as needed % insert suggested PACS numbers in braces on next line % body of paper here % now the references. delete or change fake bibitem. delete next three % lines and directly read in your .bbl file if you use bibtex. % figures follow here % % Here is an example of the general form of a figure: % Fill in the caption in the braces of the \caption{} command. Put the = label % that you will use with \ref{} command in the braces of the \label{} = command. % % \begin{figure} % \caption{} % \label{} % \end{figure} % tables follow here % % Here is an example of the general form of a table: % Fill in the caption in the braces of the \caption{} command. Put the = label % that you will use with \ref{} command in the braces of the \label{} = command. % Insert the column specifiers (l, r, c, d, etc.) in the empty braces of = the % \begin{tabular}{} command. % % \begin{table} % \caption{} % \label{} % \begin{tabular}{} % \end{tabular} % \end{table} \end{document} ------=_NextPart_000_001B_01BF66BD.FA7E5A60--