Loading…
Slowly rotating black holes in Hořava-Lifshitz gravity
In a recent paper we claimed that there are no slowly rotating, stationary, axisymmetric black holes in the infrared limit of Horava-Lifshitz gravity, provided that they are regular everywhere apart from the central singularity. Here we point out a subtlety in the relation between Einstein-aether th...
Saved in:
Published in: | Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2013-04, Vol.87 (8), Article 087504 |
---|---|
Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | cdi_FETCH-LOGICAL-c424t-e2df178ce38bcbb1e133865d7bc3b13c643ab09f60742266573fe5edde15d9993 |
---|---|
cites | cdi_FETCH-LOGICAL-c424t-e2df178ce38bcbb1e133865d7bc3b13c643ab09f60742266573fe5edde15d9993 |
container_end_page | |
container_issue | 8 |
container_start_page | |
container_title | Physical review. D, Particles, fields, gravitation, and cosmology |
container_volume | 87 |
creator | Barausse, Enrico Sotiriou, Thomas P. |
description | In a recent paper we claimed that there are no slowly rotating, stationary, axisymmetric black holes in the infrared limit of Horava-Lifshitz gravity, provided that they are regular everywhere apart from the central singularity. Here we point out a subtlety in the relation between Einstein-aether theory and the infrared limit of Horava-Lifshitz gravity which was missed in our earlier derivation and drastically modifies our conclusion: our earlier calculations (which are otherwise technically correct) do not really imply that there are no slowly rotating black holes in Horava-Lifshitz gravity, but that there are no slowly rotating black holes in the latter that are also solutions of Einstein-aether theory and vice versa. That is, even though the two theories share the static, spherically symmetric solutions, there are no slowly rotating black holes that are solutions to both theories. We proceed to generate slowly rotating black-hole solutions in the infrared limit of Horava-Lifshitz gravity, and we show that the configuration of the foliation-defining scalar remains the same as in spherical symmetry, thus these black holes are expected to possess a universal horizon. |
doi_str_mv | 10.1103/PhysRevD.87.087504 |
format | article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1709752042</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1709752042</sourcerecordid><originalsourceid>FETCH-LOGICAL-c424t-e2df178ce38bcbb1e133865d7bc3b13c643ab09f60742266573fe5edde15d9993</originalsourceid><addsrcrecordid>eNo1kLtOwzAARS0EEqXwA0wZWRL8iF8jKtAiVQLxmC3bcVqDGxc7LQp_wgfxX4BapnuHozMcAM4RrBCC5PJhOeRHt72uBK-g4BTWB2CEKIUlJkwc7j-XUhyDk5xfISSYcT4C_CnEjzAUKfa6992iMEHbt2IZg8uF74pZ_P7SW13OfZuXvv8sFklvfT-cgqNWh-zO9jsGL7c3z5NZOb-f3k2u5qWtcd2XDjct4sI6Iow1BjlEiGC04cYSg4hlNdEGypZBXmPMGOWkddQ1jUO0kVKSMbjYedcpvm9c7tXKZ-tC0J2Lm6wQh5JTDGv8i-IdalPMOblWrZNf6TQoBNVfJfVfSQmudpXID1dmXRg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1709752042</pqid></control><display><type>article</type><title>Slowly rotating black holes in Hořava-Lifshitz gravity</title><source>American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)</source><creator>Barausse, Enrico ; Sotiriou, Thomas P.</creator><creatorcontrib>Barausse, Enrico ; Sotiriou, Thomas P.</creatorcontrib><description>In a recent paper we claimed that there are no slowly rotating, stationary, axisymmetric black holes in the infrared limit of Horava-Lifshitz gravity, provided that they are regular everywhere apart from the central singularity. Here we point out a subtlety in the relation between Einstein-aether theory and the infrared limit of Horava-Lifshitz gravity which was missed in our earlier derivation and drastically modifies our conclusion: our earlier calculations (which are otherwise technically correct) do not really imply that there are no slowly rotating black holes in Horava-Lifshitz gravity, but that there are no slowly rotating black holes in the latter that are also solutions of Einstein-aether theory and vice versa. That is, even though the two theories share the static, spherically symmetric solutions, there are no slowly rotating black holes that are solutions to both theories. We proceed to generate slowly rotating black-hole solutions in the infrared limit of Horava-Lifshitz gravity, and we show that the configuration of the foliation-defining scalar remains the same as in spherical symmetry, thus these black holes are expected to possess a universal horizon.</description><identifier>ISSN: 1550-7998</identifier><identifier>EISSN: 1550-2368</identifier><identifier>DOI: 10.1103/PhysRevD.87.087504</identifier><language>eng</language><subject>Black holes (astronomy) ; Cosmology ; Derivation ; Gravitation ; Infrared ; Rotating ; Scalars ; Symmetry</subject><ispartof>Physical review. D, Particles, fields, gravitation, and cosmology, 2013-04, Vol.87 (8), Article 087504</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c424t-e2df178ce38bcbb1e133865d7bc3b13c643ab09f60742266573fe5edde15d9993</citedby><cites>FETCH-LOGICAL-c424t-e2df178ce38bcbb1e133865d7bc3b13c643ab09f60742266573fe5edde15d9993</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Barausse, Enrico</creatorcontrib><creatorcontrib>Sotiriou, Thomas P.</creatorcontrib><title>Slowly rotating black holes in Hořava-Lifshitz gravity</title><title>Physical review. D, Particles, fields, gravitation, and cosmology</title><description>In a recent paper we claimed that there are no slowly rotating, stationary, axisymmetric black holes in the infrared limit of Horava-Lifshitz gravity, provided that they are regular everywhere apart from the central singularity. Here we point out a subtlety in the relation between Einstein-aether theory and the infrared limit of Horava-Lifshitz gravity which was missed in our earlier derivation and drastically modifies our conclusion: our earlier calculations (which are otherwise technically correct) do not really imply that there are no slowly rotating black holes in Horava-Lifshitz gravity, but that there are no slowly rotating black holes in the latter that are also solutions of Einstein-aether theory and vice versa. That is, even though the two theories share the static, spherically symmetric solutions, there are no slowly rotating black holes that are solutions to both theories. We proceed to generate slowly rotating black-hole solutions in the infrared limit of Horava-Lifshitz gravity, and we show that the configuration of the foliation-defining scalar remains the same as in spherical symmetry, thus these black holes are expected to possess a universal horizon.</description><subject>Black holes (astronomy)</subject><subject>Cosmology</subject><subject>Derivation</subject><subject>Gravitation</subject><subject>Infrared</subject><subject>Rotating</subject><subject>Scalars</subject><subject>Symmetry</subject><issn>1550-7998</issn><issn>1550-2368</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNo1kLtOwzAARS0EEqXwA0wZWRL8iF8jKtAiVQLxmC3bcVqDGxc7LQp_wgfxX4BapnuHozMcAM4RrBCC5PJhOeRHt72uBK-g4BTWB2CEKIUlJkwc7j-XUhyDk5xfISSYcT4C_CnEjzAUKfa6992iMEHbt2IZg8uF74pZ_P7SW13OfZuXvv8sFklvfT-cgqNWh-zO9jsGL7c3z5NZOb-f3k2u5qWtcd2XDjct4sI6Iow1BjlEiGC04cYSg4hlNdEGypZBXmPMGOWkddQ1jUO0kVKSMbjYedcpvm9c7tXKZ-tC0J2Lm6wQh5JTDGv8i-IdalPMOblWrZNf6TQoBNVfJfVfSQmudpXID1dmXRg</recordid><startdate>20130423</startdate><enddate>20130423</enddate><creator>Barausse, Enrico</creator><creator>Sotiriou, Thomas P.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20130423</creationdate><title>Slowly rotating black holes in Hořava-Lifshitz gravity</title><author>Barausse, Enrico ; Sotiriou, Thomas P.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c424t-e2df178ce38bcbb1e133865d7bc3b13c643ab09f60742266573fe5edde15d9993</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Black holes (astronomy)</topic><topic>Cosmology</topic><topic>Derivation</topic><topic>Gravitation</topic><topic>Infrared</topic><topic>Rotating</topic><topic>Scalars</topic><topic>Symmetry</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Barausse, Enrico</creatorcontrib><creatorcontrib>Sotiriou, Thomas P.</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physical review. D, Particles, fields, gravitation, and cosmology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Barausse, Enrico</au><au>Sotiriou, Thomas P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Slowly rotating black holes in Hořava-Lifshitz gravity</atitle><jtitle>Physical review. D, Particles, fields, gravitation, and cosmology</jtitle><date>2013-04-23</date><risdate>2013</risdate><volume>87</volume><issue>8</issue><artnum>087504</artnum><issn>1550-7998</issn><eissn>1550-2368</eissn><abstract>In a recent paper we claimed that there are no slowly rotating, stationary, axisymmetric black holes in the infrared limit of Horava-Lifshitz gravity, provided that they are regular everywhere apart from the central singularity. Here we point out a subtlety in the relation between Einstein-aether theory and the infrared limit of Horava-Lifshitz gravity which was missed in our earlier derivation and drastically modifies our conclusion: our earlier calculations (which are otherwise technically correct) do not really imply that there are no slowly rotating black holes in Horava-Lifshitz gravity, but that there are no slowly rotating black holes in the latter that are also solutions of Einstein-aether theory and vice versa. That is, even though the two theories share the static, spherically symmetric solutions, there are no slowly rotating black holes that are solutions to both theories. We proceed to generate slowly rotating black-hole solutions in the infrared limit of Horava-Lifshitz gravity, and we show that the configuration of the foliation-defining scalar remains the same as in spherical symmetry, thus these black holes are expected to possess a universal horizon.</abstract><doi>10.1103/PhysRevD.87.087504</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1550-7998 |
ispartof | Physical review. D, Particles, fields, gravitation, and cosmology, 2013-04, Vol.87 (8), Article 087504 |
issn | 1550-7998 1550-2368 |
language | eng |
recordid | cdi_proquest_miscellaneous_1709752042 |
source | American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list) |
subjects | Black holes (astronomy) Cosmology Derivation Gravitation Infrared Rotating Scalars Symmetry |
title | Slowly rotating black holes in Hořava-Lifshitz gravity |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-24T20%3A00%3A35IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Slowly%20rotating%20black%20holes%20in%20Ho%C5%99ava-Lifshitz%20gravity&rft.jtitle=Physical%20review.%20D,%20Particles,%20fields,%20gravitation,%20and%20cosmology&rft.au=Barausse,%20Enrico&rft.date=2013-04-23&rft.volume=87&rft.issue=8&rft.artnum=087504&rft.issn=1550-7998&rft.eissn=1550-2368&rft_id=info:doi/10.1103/PhysRevD.87.087504&rft_dat=%3Cproquest_cross%3E1709752042%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c424t-e2df178ce38bcbb1e133865d7bc3b13c643ab09f60742266573fe5edde15d9993%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1709752042&rft_id=info:pmid/&rfr_iscdi=true |