Public Release of RELXILL_NK: A Relativistic Reflection Model for Testing Einstein's Gravity
We present the public release version of relxill_nk, an X-ray reflection model for testing the Kerr hypothesis and general relativity. This model extends the relxill model that assumes the black hole (BH) spacetime is described by the Kerr metric. We also present relxilllp_nk, the first non-Kerr X-r...
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Veröffentlicht in: | The Astrophysical journal 2019-06, Vol.878 (2), p.91 |
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creator | Abdikamalov, Askar B. Ayzenberg, Dimitry Bambi, Cosimo Dauser, Thomas García, Javier A. Nampalliwar, Sourabh |
description | We present the public release version of relxill_nk, an X-ray reflection model for testing the Kerr hypothesis and general relativity. This model extends the relxill model that assumes the black hole (BH) spacetime is described by the Kerr metric. We also present relxilllp_nk, the first non-Kerr X-ray reflection model with a lamppost corona configuration, as well as all other models available in the full relxill_nk package. In all models the relevant relativistic effects are calculated through a general relativistic ray-tracing code that can be applied to any well-behaved, stationary, axisymmetric, and asymptotically flat BH spacetime. We show that the numerical error introduced by using a ray-tracing code is not significant compared with the observational error present in current X-ray reflection spectrum observations. In addition, we present the reflection spectrum for the Johannsen metric as calculated by relxill_nk. |
doi_str_mv | 10.3847/1538-4357/ab1f89 |
format | Article |
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This model extends the relxill model that assumes the black hole (BH) spacetime is described by the Kerr metric. We also present relxilllp_nk, the first non-Kerr X-ray reflection model with a lamppost corona configuration, as well as all other models available in the full relxill_nk package. In all models the relevant relativistic effects are calculated through a general relativistic ray-tracing code that can be applied to any well-behaved, stationary, axisymmetric, and asymptotically flat BH spacetime. We show that the numerical error introduced by using a ray-tracing code is not significant compared with the observational error present in current X-ray reflection spectrum observations. 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J</addtitle><description>We present the public release version of relxill_nk, an X-ray reflection model for testing the Kerr hypothesis and general relativity. This model extends the relxill model that assumes the black hole (BH) spacetime is described by the Kerr metric. We also present relxilllp_nk, the first non-Kerr X-ray reflection model with a lamppost corona configuration, as well as all other models available in the full relxill_nk package. In all models the relevant relativistic effects are calculated through a general relativistic ray-tracing code that can be applied to any well-behaved, stationary, axisymmetric, and asymptotically flat BH spacetime. We show that the numerical error introduced by using a ray-tracing code is not significant compared with the observational error present in current X-ray reflection spectrum observations. In addition, we present the reflection spectrum for the Johannsen metric as calculated by relxill_nk.</description><subject>accretion, accretion disks</subject><subject>Astrophysics</subject><subject>black hole physics</subject><subject>Black holes</subject><subject>Corona</subject><subject>gravitation</subject><subject>Model testing</subject><subject>Ray tracing</subject><subject>Relativism</subject><subject>Relativistic effects</subject><subject>Relativity</subject><subject>Spacetime</subject><subject>X ray reflection</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp9kM9LwzAUx4MoOKd3jwEFL9YlTdok3mTMOaw_GBN2EEKaJpJR25p0g_33tk70Ip4e730_3_ceXwBOMboinLIRTgiPKEnYSOXYcrEHBj-jfTBACNEoJWx5CI5CWPVtLMQAvD6v89JpODelUcHA2sL5JFvOskw-3l_Dm15Qrdu40H5RtjS6dXUFH-rClNDWHi5Mp1VvcOKq0BpXXQQ49Wrj2u0xOLCqDObkuw7By-1kMb6LsqfpbHyTRZow0UYqZcbQFBlKdYyV5YlBSCBFuaWUJalOFSu4iQsVFyYmJmFMp1QUAosc57ogQ3C229v4-mPdvSNX9dpX3UkZk7TDecJ4R6EdpX0dgjdWNt69K7-VGMk-Q9kHJvvA5C7DznK5s7i6-d35D37-B66aleSMy1gKLJvCkk8Qbn5p</recordid><startdate>20190620</startdate><enddate>20190620</enddate><creator>Abdikamalov, Askar B.</creator><creator>Ayzenberg, Dimitry</creator><creator>Bambi, Cosimo</creator><creator>Dauser, Thomas</creator><creator>García, Javier A.</creator><creator>Nampalliwar, Sourabh</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-3180-9502</orcidid></search><sort><creationdate>20190620</creationdate><title>Public Release of RELXILL_NK: A Relativistic Reflection Model for Testing Einstein's Gravity</title><author>Abdikamalov, Askar B. ; Ayzenberg, Dimitry ; Bambi, Cosimo ; Dauser, Thomas ; García, Javier A. ; Nampalliwar, Sourabh</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c379t-a67ee460e44c21af85e0090a48f44756c6a7d8e2da2de23e577c649d919b1bcd3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>accretion, accretion disks</topic><topic>Astrophysics</topic><topic>black hole physics</topic><topic>Black holes</topic><topic>Corona</topic><topic>gravitation</topic><topic>Model testing</topic><topic>Ray tracing</topic><topic>Relativism</topic><topic>Relativistic effects</topic><topic>Relativity</topic><topic>Spacetime</topic><topic>X ray reflection</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Abdikamalov, Askar B.</creatorcontrib><creatorcontrib>Ayzenberg, Dimitry</creatorcontrib><creatorcontrib>Bambi, Cosimo</creatorcontrib><creatorcontrib>Dauser, Thomas</creatorcontrib><creatorcontrib>García, Javier A.</creatorcontrib><creatorcontrib>Nampalliwar, Sourabh</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Abdikamalov, Askar B.</au><au>Ayzenberg, Dimitry</au><au>Bambi, Cosimo</au><au>Dauser, Thomas</au><au>García, Javier A.</au><au>Nampalliwar, Sourabh</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Public Release of RELXILL_NK: A Relativistic Reflection Model for Testing Einstein's Gravity</atitle><jtitle>The Astrophysical journal</jtitle><stitle>APJ</stitle><addtitle>Astrophys. 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subjects | accretion, accretion disks Astrophysics black hole physics Black holes Corona gravitation Model testing Ray tracing Relativism Relativistic effects Relativity Spacetime X ray reflection |
title | Public Release of RELXILL_NK: A Relativistic Reflection Model for Testing Einstein's Gravity |
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