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Conservative scattering of Reissner-Nordström black holes at third post-Minkowskian order
A bstract Using a recently developed effective field theory formalism for extreme mass ratios arXiv:2308.14832, we present a calculation of charged black hole scattering at third post-Minkowskian order. The charges and masses are kept arbitrary, and the result interpolates from the scattering of Sch...
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| Published in: | The journal of high energy physics 2024-05, Vol.2024 (5), p.265-29, Article 265 |
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| container_end_page | 29 |
| container_issue | 5 |
| container_start_page | 265 |
| container_title | The journal of high energy physics |
| container_volume | 2024 |
| creator | Wilson-Gerow, Jordan |
| description | A
bstract
Using a recently developed effective field theory formalism for extreme mass ratios arXiv:2308.14832, we present a calculation of charged black hole scattering at third post-Minkowskian order. The charges and masses are kept arbitrary, and the result interpolates from the scattering of Schwarzschild to extremal charged black holes, and beyond to charged particles in electrodynamics — agreeing with previously reported results in all such limits. The computation of the radial action is neatly organized in powers of the mass ratio. The probe (0SF) contributions are readily computed by direct integration of the radial momentum, and we use the effective field theory to compute the subleading (1SF) contributions via background-field Feynman rules supplemented by an operator encoding recoil of the background. Together these contributions completely determine the conservative physics at order
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| doi_str_mv | 10.1007/JHEP05(2024)265 |
| format | article |
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bstract
Using a recently developed effective field theory formalism for extreme mass ratios arXiv:2308.14832, we present a calculation of charged black hole scattering at third post-Minkowskian order. The charges and masses are kept arbitrary, and the result interpolates from the scattering of Schwarzschild to extremal charged black holes, and beyond to charged particles in electrodynamics — agreeing with previously reported results in all such limits. The computation of the radial action is neatly organized in powers of the mass ratio. The probe (0SF) contributions are readily computed by direct integration of the radial momentum, and we use the effective field theory to compute the subleading (1SF) contributions via background-field Feynman rules supplemented by an operator encoding recoil of the background. Together these contributions completely determine the conservative physics at order
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3
.</description><identifier>ISSN: 1029-8479</identifier><identifier>EISSN: 1029-8479</identifier><identifier>DOI: 10.1007/JHEP05(2024)265</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Approximation ; Black Holes ; Charged particles ; Classical and Quantum Gravitation ; Efective Field Theories ; Effective Field Theories ; Electrodynamics ; Elementary Particles ; Field theory ; Gravitational waves ; Mass ratios ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Quantum Physics ; Regular Article - Theoretical Physics ; Relativity Theory ; Scattering ; Spacetime ; String Theory ; Theory of relativity</subject><ispartof>The journal of high energy physics, 2024-05, Vol.2024 (5), p.265-29, Article 265</ispartof><rights>The Author(s) 2024</rights><rights>The Author(s) 2024. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c328t-ca07b70e8c79522b2645c7e02582296313e76026661fd12abe77f7fc993937693</cites><orcidid>0000-0002-1955-8018 ; 0000000219558018</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/3061553807/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/3061553807?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>230,314,780,784,885,25753,27924,27925,37012,44590,74998</link.rule.ids><backlink>$$Uhttps://www.osti.gov/servlets/purl/2479637$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Wilson-Gerow, Jordan</creatorcontrib><creatorcontrib>California Institute of Technology (CalTech), Pasadena, CA (United States)</creatorcontrib><title>Conservative scattering of Reissner-Nordström black holes at third post-Minkowskian order</title><title>The journal of high energy physics</title><addtitle>J. High Energ. Phys</addtitle><description>A
bstract
Using a recently developed effective field theory formalism for extreme mass ratios arXiv:2308.14832, we present a calculation of charged black hole scattering at third post-Minkowskian order. The charges and masses are kept arbitrary, and the result interpolates from the scattering of Schwarzschild to extremal charged black holes, and beyond to charged particles in electrodynamics — agreeing with previously reported results in all such limits. The computation of the radial action is neatly organized in powers of the mass ratio. The probe (0SF) contributions are readily computed by direct integration of the radial momentum, and we use the effective field theory to compute the subleading (1SF) contributions via background-field Feynman rules supplemented by an operator encoding recoil of the background. Together these contributions completely determine the conservative physics at order
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3
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bstract
Using a recently developed effective field theory formalism for extreme mass ratios arXiv:2308.14832, we present a calculation of charged black hole scattering at third post-Minkowskian order. The charges and masses are kept arbitrary, and the result interpolates from the scattering of Schwarzschild to extremal charged black holes, and beyond to charged particles in electrodynamics — agreeing with previously reported results in all such limits. The computation of the radial action is neatly organized in powers of the mass ratio. The probe (0SF) contributions are readily computed by direct integration of the radial momentum, and we use the effective field theory to compute the subleading (1SF) contributions via background-field Feynman rules supplemented by an operator encoding recoil of the background. Together these contributions completely determine the conservative physics at order
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.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1007/JHEP05(2024)265</doi><tpages>29</tpages><orcidid>https://orcid.org/0000-0002-1955-8018</orcidid><orcidid>https://orcid.org/0000000219558018</orcidid><oa>free_for_read</oa></addata></record> |
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| subjects | Approximation Black Holes Charged particles Classical and Quantum Gravitation Efective Field Theories Effective Field Theories Electrodynamics Elementary Particles Field theory Gravitational waves Mass ratios Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Quantum Physics Regular Article - Theoretical Physics Relativity Theory Scattering Spacetime String Theory Theory of relativity |
| title | Conservative scattering of Reissner-Nordström black holes at third post-Minkowskian order |
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