The Missing Link: Merging Neutron Stars Naturally Produce Jet-like Structures and Can Power Short Gamma-ray Bursts
Short gamma-ray bursts (SGRBs) are among the most luminous explosions in the universe, releasing in less than one second the energy emitted by our Galaxy over one year. Despite decades of observations, the nature of their 'central engine' remains unknown. Considering a binary of magnetized...
Gespeichert in:
Veröffentlicht in: | Astrophysical journal. Letters 2011-05, Vol.732 (1), p.L6-jQuery1323917774770='48' |
---|---|
Hauptverfasser: | , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext bestellen |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | jQuery1323917774770='48' |
---|---|
container_issue | 1 |
container_start_page | L6 |
container_title | Astrophysical journal. Letters |
container_volume | 732 |
creator | Rezzolla, Luciano Giacomazzo, Bruno Baiotti, Luca Granot, Jonathan Kouveliotou, Chryssa Aloy, Miguel A |
description | Short gamma-ray bursts (SGRBs) are among the most luminous explosions in the universe, releasing in less than one second the energy emitted by our Galaxy over one year. Despite decades of observations, the nature of their 'central engine' remains unknown. Considering a binary of magnetized neutron stars and solving the Einstein equations, we show that their merger results in a rapidly spinning black hole surrounded by a hot and highly magnetized torus. Lasting over 35 ms and much longer than previous simulations, our study reveals that magnetohydrodynamical instabilities amplify an initially turbulent magnetic field of ~1012 G to produce an ordered poloidal field of ~1015 G along the black hole spin axis, within a half-opening angle of ~30?, which may naturally launch a relativistic jet. The broad consistency of our ab initio calculations with SGRB observations shows that the merger of magnetized neutron stars can provide the basic physical conditions for the central engine of SGRBs. |
doi_str_mv | 10.1088/2041-8205/732/1/L6 |
format | Article |
fullrecord | <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_proquest_miscellaneous_920791422</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>920791422</sourcerecordid><originalsourceid>FETCH-LOGICAL-c423t-2b504fb9af197d7d4d9694f18fb4d06e00aa75f2fd5829a26ae4107fdc7d01d73</originalsourceid><addsrcrecordid>eNqNkTtPwzAUhSMEEs8_wGSJATGEXjsPJ2xQ8VQolYDZcu1rakjjYjtC_fekKmJhYbqv79zhnCQ5pnBOoapGDHKaVgyKEc_YiI6acivZ-1nSbPu3h2I32Q_hHYBBSau9xL_MkTzaEGz3RhrbfVyQR_Rv62mCffSuI89R-kAmMvZetu2KTL3TvULygDFt7QcOgO_VcMVAZKfJWHZk6r7Qk-e585HcysVCpl6uyFXvQwyHyY6RbcCjn3qQvN5cv4zv0ubp9n582aQqZ1lM2ayA3MxqaWjNNde5rss6N7Qys1xDiQBS8sIwo4uK1ZKVEnMK3GjFNVDNs4PkZPPXhWhFUDaimivXdaiiYLQoGYdqoE431NK7zx5DFAsbFLat7ND1QdQMeE1zxgaSbUjlXQgejVh6u5B-JSiIdQpibbJYmyyGFAQVTTmI0o3IuuX_-LO__F9OLLXJvgHLUJTo</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>920791422</pqid></control><display><type>article</type><title>The Missing Link: Merging Neutron Stars Naturally Produce Jet-like Structures and Can Power Short Gamma-ray Bursts</title><source>Institute of Physics Open Access Journal Titles</source><creator>Rezzolla, Luciano ; Giacomazzo, Bruno ; Baiotti, Luca ; Granot, Jonathan ; Kouveliotou, Chryssa ; Aloy, Miguel A</creator><creatorcontrib>Rezzolla, Luciano ; Giacomazzo, Bruno ; Baiotti, Luca ; Granot, Jonathan ; Kouveliotou, Chryssa ; Aloy, Miguel A</creatorcontrib><description>Short gamma-ray bursts (SGRBs) are among the most luminous explosions in the universe, releasing in less than one second the energy emitted by our Galaxy over one year. Despite decades of observations, the nature of their 'central engine' remains unknown. Considering a binary of magnetized neutron stars and solving the Einstein equations, we show that their merger results in a rapidly spinning black hole surrounded by a hot and highly magnetized torus. Lasting over 35 ms and much longer than previous simulations, our study reveals that magnetohydrodynamical instabilities amplify an initially turbulent magnetic field of ~1012 G to produce an ordered poloidal field of ~1015 G along the black hole spin axis, within a half-opening angle of ~30?, which may naturally launch a relativistic jet. The broad consistency of our ab initio calculations with SGRB observations shows that the merger of magnetized neutron stars can provide the basic physical conditions for the central engine of SGRBs.</description><identifier>ISSN: 2041-8205</identifier><identifier>EISSN: 2041-8213</identifier><identifier>DOI: 10.1088/2041-8205/732/1/L6</identifier><language>eng</language><publisher>United States: IOP Publishing</publisher><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; BLACK HOLES ; COSMIC GAMMA BURSTS ; COSMIC RADIATION ; EINSTEIN FIELD EQUATIONS ; EQUATIONS ; FIELD EQUATIONS ; FLUID MECHANICS ; GALAXIES ; GRAVITATIONAL WAVES ; HYDRODYNAMICS ; INSTABILITY ; IONIZING RADIATIONS ; JETS ; MAGNETIC FIELDS ; MAGNETOHYDRODYNAMICS ; MECHANICS ; NEUTRON STARS ; PRIMARY COSMIC RADIATION ; RADIATIONS ; SIMULATION ; STARS</subject><ispartof>Astrophysical journal. Letters, 2011-05, Vol.732 (1), p.L6-jQuery1323917774770='48'</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c423t-2b504fb9af197d7d4d9694f18fb4d06e00aa75f2fd5829a26ae4107fdc7d01d73</citedby><cites>FETCH-LOGICAL-c423t-2b504fb9af197d7d4d9694f18fb4d06e00aa75f2fd5829a26ae4107fdc7d01d73</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/2041-8205/732/1/L6/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>230,314,776,780,881,1547,27605,27901,27902,53879,53906</link.rule.ids><linktorsrc>$$Uhttp://iopscience.iop.org/2041-8205/732/1/L6$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttps://www.osti.gov/biblio/21562708$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Rezzolla, Luciano</creatorcontrib><creatorcontrib>Giacomazzo, Bruno</creatorcontrib><creatorcontrib>Baiotti, Luca</creatorcontrib><creatorcontrib>Granot, Jonathan</creatorcontrib><creatorcontrib>Kouveliotou, Chryssa</creatorcontrib><creatorcontrib>Aloy, Miguel A</creatorcontrib><title>The Missing Link: Merging Neutron Stars Naturally Produce Jet-like Structures and Can Power Short Gamma-ray Bursts</title><title>Astrophysical journal. Letters</title><description>Short gamma-ray bursts (SGRBs) are among the most luminous explosions in the universe, releasing in less than one second the energy emitted by our Galaxy over one year. Despite decades of observations, the nature of their 'central engine' remains unknown. Considering a binary of magnetized neutron stars and solving the Einstein equations, we show that their merger results in a rapidly spinning black hole surrounded by a hot and highly magnetized torus. Lasting over 35 ms and much longer than previous simulations, our study reveals that magnetohydrodynamical instabilities amplify an initially turbulent magnetic field of ~1012 G to produce an ordered poloidal field of ~1015 G along the black hole spin axis, within a half-opening angle of ~30?, which may naturally launch a relativistic jet. The broad consistency of our ab initio calculations with SGRB observations shows that the merger of magnetized neutron stars can provide the basic physical conditions for the central engine of SGRBs.</description><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>BLACK HOLES</subject><subject>COSMIC GAMMA BURSTS</subject><subject>COSMIC RADIATION</subject><subject>EINSTEIN FIELD EQUATIONS</subject><subject>EQUATIONS</subject><subject>FIELD EQUATIONS</subject><subject>FLUID MECHANICS</subject><subject>GALAXIES</subject><subject>GRAVITATIONAL WAVES</subject><subject>HYDRODYNAMICS</subject><subject>INSTABILITY</subject><subject>IONIZING RADIATIONS</subject><subject>JETS</subject><subject>MAGNETIC FIELDS</subject><subject>MAGNETOHYDRODYNAMICS</subject><subject>MECHANICS</subject><subject>NEUTRON STARS</subject><subject>PRIMARY COSMIC RADIATION</subject><subject>RADIATIONS</subject><subject>SIMULATION</subject><subject>STARS</subject><issn>2041-8205</issn><issn>2041-8213</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNqNkTtPwzAUhSMEEs8_wGSJATGEXjsPJ2xQ8VQolYDZcu1rakjjYjtC_fekKmJhYbqv79zhnCQ5pnBOoapGDHKaVgyKEc_YiI6acivZ-1nSbPu3h2I32Q_hHYBBSau9xL_MkTzaEGz3RhrbfVyQR_Rv62mCffSuI89R-kAmMvZetu2KTL3TvULygDFt7QcOgO_VcMVAZKfJWHZk6r7Qk-e585HcysVCpl6uyFXvQwyHyY6RbcCjn3qQvN5cv4zv0ubp9n582aQqZ1lM2ayA3MxqaWjNNde5rss6N7Qys1xDiQBS8sIwo4uK1ZKVEnMK3GjFNVDNs4PkZPPXhWhFUDaimivXdaiiYLQoGYdqoE431NK7zx5DFAsbFLat7ND1QdQMeE1zxgaSbUjlXQgejVh6u5B-JSiIdQpibbJYmyyGFAQVTTmI0o3IuuX_-LO__F9OLLXJvgHLUJTo</recordid><startdate>20110501</startdate><enddate>20110501</enddate><creator>Rezzolla, Luciano</creator><creator>Giacomazzo, Bruno</creator><creator>Baiotti, Luca</creator><creator>Granot, Jonathan</creator><creator>Kouveliotou, Chryssa</creator><creator>Aloy, Miguel A</creator><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>OTOTI</scope></search><sort><creationdate>20110501</creationdate><title>The Missing Link: Merging Neutron Stars Naturally Produce Jet-like Structures and Can Power Short Gamma-ray Bursts</title><author>Rezzolla, Luciano ; Giacomazzo, Bruno ; Baiotti, Luca ; Granot, Jonathan ; Kouveliotou, Chryssa ; Aloy, Miguel A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c423t-2b504fb9af197d7d4d9694f18fb4d06e00aa75f2fd5829a26ae4107fdc7d01d73</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>BLACK HOLES</topic><topic>COSMIC GAMMA BURSTS</topic><topic>COSMIC RADIATION</topic><topic>EINSTEIN FIELD EQUATIONS</topic><topic>EQUATIONS</topic><topic>FIELD EQUATIONS</topic><topic>FLUID MECHANICS</topic><topic>GALAXIES</topic><topic>GRAVITATIONAL WAVES</topic><topic>HYDRODYNAMICS</topic><topic>INSTABILITY</topic><topic>IONIZING RADIATIONS</topic><topic>JETS</topic><topic>MAGNETIC FIELDS</topic><topic>MAGNETOHYDRODYNAMICS</topic><topic>MECHANICS</topic><topic>NEUTRON STARS</topic><topic>PRIMARY COSMIC RADIATION</topic><topic>RADIATIONS</topic><topic>SIMULATION</topic><topic>STARS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Rezzolla, Luciano</creatorcontrib><creatorcontrib>Giacomazzo, Bruno</creatorcontrib><creatorcontrib>Baiotti, Luca</creatorcontrib><creatorcontrib>Granot, Jonathan</creatorcontrib><creatorcontrib>Kouveliotou, Chryssa</creatorcontrib><creatorcontrib>Aloy, Miguel A</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>OSTI.GOV</collection><jtitle>Astrophysical journal. Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Rezzolla, Luciano</au><au>Giacomazzo, Bruno</au><au>Baiotti, Luca</au><au>Granot, Jonathan</au><au>Kouveliotou, Chryssa</au><au>Aloy, Miguel A</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Missing Link: Merging Neutron Stars Naturally Produce Jet-like Structures and Can Power Short Gamma-ray Bursts</atitle><jtitle>Astrophysical journal. Letters</jtitle><date>2011-05-01</date><risdate>2011</risdate><volume>732</volume><issue>1</issue><spage>L6</spage><epage>jQuery1323917774770='48'</epage><pages>L6-jQuery1323917774770='48'</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>Short gamma-ray bursts (SGRBs) are among the most luminous explosions in the universe, releasing in less than one second the energy emitted by our Galaxy over one year. Despite decades of observations, the nature of their 'central engine' remains unknown. Considering a binary of magnetized neutron stars and solving the Einstein equations, we show that their merger results in a rapidly spinning black hole surrounded by a hot and highly magnetized torus. Lasting over 35 ms and much longer than previous simulations, our study reveals that magnetohydrodynamical instabilities amplify an initially turbulent magnetic field of ~1012 G to produce an ordered poloidal field of ~1015 G along the black hole spin axis, within a half-opening angle of ~30?, which may naturally launch a relativistic jet. The broad consistency of our ab initio calculations with SGRB observations shows that the merger of magnetized neutron stars can provide the basic physical conditions for the central engine of SGRBs.</abstract><cop>United States</cop><pub>IOP Publishing</pub><doi>10.1088/2041-8205/732/1/L6</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | ISSN: 2041-8205 |
ispartof | Astrophysical journal. Letters, 2011-05, Vol.732 (1), p.L6-jQuery1323917774770='48' |
issn | 2041-8205 2041-8213 |
language | eng |
recordid | cdi_proquest_miscellaneous_920791422 |
source | Institute of Physics Open Access Journal Titles |
subjects | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BLACK HOLES COSMIC GAMMA BURSTS COSMIC RADIATION EINSTEIN FIELD EQUATIONS EQUATIONS FIELD EQUATIONS FLUID MECHANICS GALAXIES GRAVITATIONAL WAVES HYDRODYNAMICS INSTABILITY IONIZING RADIATIONS JETS MAGNETIC FIELDS MAGNETOHYDRODYNAMICS MECHANICS NEUTRON STARS PRIMARY COSMIC RADIATION RADIATIONS SIMULATION STARS |
title | The Missing Link: Merging Neutron Stars Naturally Produce Jet-like Structures and Can Power Short Gamma-ray Bursts |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-19T02%3A06%3A04IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20Missing%20Link:%20Merging%20Neutron%20Stars%20Naturally%20Produce%20Jet-like%20Structures%20and%20Can%20Power%20Short%20Gamma-ray%20Bursts&rft.jtitle=Astrophysical%20journal.%20Letters&rft.au=Rezzolla,%20Luciano&rft.date=2011-05-01&rft.volume=732&rft.issue=1&rft.spage=L6&rft.epage=jQuery1323917774770='48'&rft.pages=L6-jQuery1323917774770='48'&rft.issn=2041-8205&rft.eissn=2041-8213&rft_id=info:doi/10.1088/2041-8205/732/1/L6&rft_dat=%3Cproquest_O3W%3E920791422%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=920791422&rft_id=info:pmid/&rfr_iscdi=true |