Interacting Geodesics: Binary Systems around a Black Hole
We present a novel method to study interacting orbits in a fixed mean gravitational field associated with a solution of the Einstein field equations. The idea is to consider the Newton gravity among the orbiting particles in a geometry given by the main source. We apply the technique in the of study...
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| creator | Gueron, Eduardo Letelier, Patricio S |
| description | We present a novel method to study interacting orbits in a fixed mean
gravitational field associated with a solution of the Einstein field equations.
The idea is to consider the Newton gravity among the orbiting particles in a
geometry given by the main source. We apply the technique in the of study two
and three self-gravitating particles moving around a black hole, i.e., in a
Schwarzschild geometry. We also compare with the equivalent Newtonian problem
and noted differences in the structural stability, e.g., binary systems were
found only in the general relativistic approach. |
| doi_str_mv | 10.48550/arxiv.astro-ph/0302578 |
| format | Article |
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gravitational field associated with a solution of the Einstein field equations.
The idea is to consider the Newton gravity among the orbiting particles in a
geometry given by the main source. We apply the technique in the of study two
and three self-gravitating particles moving around a black hole, i.e., in a
Schwarzschild geometry. We also compare with the equivalent Newtonian problem
and noted differences in the structural stability, e.g., binary systems were
found only in the general relativistic approach.</description><identifier>DOI: 10.48550/arxiv.astro-ph/0302578</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Earth and Planetary Astrophysics ; Physics - General Relativity and Quantum Cosmology ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics</subject><creationdate>2003-02</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/astro-ph/0302578$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.astro-ph/0302578$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Gueron, Eduardo</creatorcontrib><creatorcontrib>Letelier, Patricio S</creatorcontrib><title>Interacting Geodesics: Binary Systems around a Black Hole</title><description>We present a novel method to study interacting orbits in a fixed mean
gravitational field associated with a solution of the Einstein field equations.
The idea is to consider the Newton gravity among the orbiting particles in a
geometry given by the main source. We apply the technique in the of study two
and three self-gravitating particles moving around a black hole, i.e., in a
Schwarzschild geometry. We also compare with the equivalent Newtonian problem
and noted differences in the structural stability, e.g., binary systems were
found only in the general relativistic approach.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - General Relativity and Quantum Cosmology</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2003</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj7FuwjAURb10qKDfUC8dAzaOnTy2glpAQmIoe_RsvxSrIYnstCp_TwRMV1dXOrqHsVcpZnmptZhj_A9_M0xD7LL-NBdKLHRRPjPYtQNFdENov_mGOk8puLTkq9BivPCvSxronDjG7rf1HPmqQffDt11DU_ZUY5Po5ZETdvz8OK632f6w2a3f9xkWUGa1dmAlFVYQope1BlqYvARy2oDNpTdWgTDeg_U1KpHLcRyrE9IahEJN2NsdezOo-hjO47HqZlL1p-phoq7on0cH</recordid><startdate>20030227</startdate><enddate>20030227</enddate><creator>Gueron, Eduardo</creator><creator>Letelier, Patricio S</creator><scope>GOX</scope></search><sort><creationdate>20030227</creationdate><title>Interacting Geodesics: Binary Systems around a Black Hole</title><author>Gueron, Eduardo ; Letelier, Patricio S</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a798-f5c9b1e7b0eaad1f59e26489ec569b41d6b3906dd9bdfa30414896ddc01b6a973</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2003</creationdate><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - General Relativity and Quantum Cosmology</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Gueron, Eduardo</creatorcontrib><creatorcontrib>Letelier, Patricio S</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Gueron, Eduardo</au><au>Letelier, Patricio S</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Interacting Geodesics: Binary Systems around a Black Hole</atitle><date>2003-02-27</date><risdate>2003</risdate><abstract>We present a novel method to study interacting orbits in a fixed mean
gravitational field associated with a solution of the Einstein field equations.
The idea is to consider the Newton gravity among the orbiting particles in a
geometry given by the main source. We apply the technique in the of study two
and three self-gravitating particles moving around a black hole, i.e., in a
Schwarzschild geometry. We also compare with the equivalent Newtonian problem
and noted differences in the structural stability, e.g., binary systems were
found only in the general relativistic approach.</abstract><doi>10.48550/arxiv.astro-ph/0302578</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - General Relativity and Quantum Cosmology Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
| title | Interacting Geodesics: Binary Systems around a Black Hole |
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