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SMWDs as SGRs/AXPs and the lepton number violation
Possible nature of strongly magnetized white dwarfs (SMWDs) is studied. It is shown that for relatively low values of the equatorial surface magnetic field B ∼ 109 − 1011 G they can be good candidates for soft gamma-ray repeaters and anomalous X-ray pulsars (SGRs/AXPs). For the case of iron SMWDs th...
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creator | Adam, J. Truhlík, E. Belyaev, V. B. Ricci, P. Šimkovic, F. Bogolyubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna 141980 |
description | Possible nature of strongly magnetized white dwarfs (SMWDs) is studied. It is shown that for relatively low values of the equatorial surface magnetic field B ∼ 109 − 1011 G they can be good candidates for soft gamma-ray repeaters and anomalous X-ray pulsars (SGRs/AXPs). For the case of iron SMWDs the influence of a neutrinoless electron to positron conversion on the SGRs/AXPs luminosity is estimated. |
doi_str_mv | 10.1063/1.4934917 |
format | conference_proceeding |
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B. ; Ricci, P. ; Šimkovic, F. ; Bogolyubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna 141980</creator><creatorcontrib>Adam, J. ; Truhlík, E. ; Belyaev, V. B. ; Ricci, P. ; Šimkovic, F. ; Bogolyubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna 141980</creatorcontrib><description>Possible nature of strongly magnetized white dwarfs (SMWDs) is studied. It is shown that for relatively low values of the equatorial surface magnetic field B ∼ 109 − 1011 G they can be good candidates for soft gamma-ray repeaters and anomalous X-ray pulsars (SGRs/AXPs). For the case of iron SMWDs the influence of a neutrinoless electron to positron conversion on the SGRs/AXPs luminosity is estimated.</description><identifier>ISSN: 0094-243X</identifier><identifier>EISSN: 1551-7616</identifier><identifier>DOI: 10.1063/1.4934917</identifier><language>eng</language><publisher>Melville: American Institute of Physics</publisher><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; ELECTRONS ; GAMMA RADIATION ; IRON ; LEPTON NUMBER ; Leptons ; LUMINOSITY ; MAGNETIC FIELDS ; NEUTRINOS ; POSITRONS ; PULSARS ; Soft gamma ray repeaters ; SURFACES ; VIOLATIONS ; WHITE DWARF STARS ; X RADIATION</subject><ispartof>AIP conference proceedings, 2015, Vol.1686 (1)</ispartof><rights>2015 AIP Publishing LLC.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,309,310,314,780,784,789,790,885,23929,23930,25139,27923,27924</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22492680$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Adam, J.</creatorcontrib><creatorcontrib>Truhlík, E.</creatorcontrib><creatorcontrib>Belyaev, V. B.</creatorcontrib><creatorcontrib>Ricci, P.</creatorcontrib><creatorcontrib>Šimkovic, F.</creatorcontrib><creatorcontrib>Bogolyubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna 141980</creatorcontrib><title>SMWDs as SGRs/AXPs and the lepton number violation</title><title>AIP conference proceedings</title><description>Possible nature of strongly magnetized white dwarfs (SMWDs) is studied. It is shown that for relatively low values of the equatorial surface magnetic field B ∼ 109 − 1011 G they can be good candidates for soft gamma-ray repeaters and anomalous X-ray pulsars (SGRs/AXPs). For the case of iron SMWDs the influence of a neutrinoless electron to positron conversion on the SGRs/AXPs luminosity is estimated.</description><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>ELECTRONS</subject><subject>GAMMA RADIATION</subject><subject>IRON</subject><subject>LEPTON NUMBER</subject><subject>Leptons</subject><subject>LUMINOSITY</subject><subject>MAGNETIC FIELDS</subject><subject>NEUTRINOS</subject><subject>POSITRONS</subject><subject>PULSARS</subject><subject>Soft gamma ray repeaters</subject><subject>SURFACES</subject><subject>VIOLATIONS</subject><subject>WHITE DWARF STARS</subject><subject>X RADIATION</subject><issn>0094-243X</issn><issn>1551-7616</issn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2015</creationdate><recordtype>conference_proceeding</recordtype><recordid>eNpFjstKAzEYRoMoOFYXvsGA62nz5zbJslStQkWxit0NudIpY1KbjM9vQcHVx4HD4UPoGvAUsKAzmDJFmYL2BFXAOTStAHGKKowVawijm3N0kfMOY6LaVlaIrJ8-bnOtc71evubZfPNyhOjqsvX14PclxTqOn8Yf6u8-Dbr0KV6is6CH7K_-doLe7-_eFg_N6nn5uJivmkQASgNBgTJaCxkcluCFYYER7kAyYYUJxnKHW8UwBMmc815oJY3TPlhQynM6QTe_3ZRL32XbF2-3NsXobekIYYoIif-t_SF9jT6XbpfGQzwe6wgQKjlmjNIfQ2VQPw</recordid><startdate>20151028</startdate><enddate>20151028</enddate><creator>Adam, J.</creator><creator>Truhlík, E.</creator><creator>Belyaev, V. 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B.</au><au>Ricci, P.</au><au>Šimkovic, F.</au><au>Bogolyubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna 141980</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>SMWDs as SGRs/AXPs and the lepton number violation</atitle><btitle>AIP conference proceedings</btitle><date>2015-10-28</date><risdate>2015</risdate><volume>1686</volume><issue>1</issue><issn>0094-243X</issn><eissn>1551-7616</eissn><abstract>Possible nature of strongly magnetized white dwarfs (SMWDs) is studied. It is shown that for relatively low values of the equatorial surface magnetic field B ∼ 109 − 1011 G they can be good candidates for soft gamma-ray repeaters and anomalous X-ray pulsars (SGRs/AXPs). For the case of iron SMWDs the influence of a neutrinoless electron to positron conversion on the SGRs/AXPs luminosity is estimated.</abstract><cop>Melville</cop><pub>American Institute of Physics</pub><doi>10.1063/1.4934917</doi></addata></record> |
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subjects | CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ELECTRONS GAMMA RADIATION IRON LEPTON NUMBER Leptons LUMINOSITY MAGNETIC FIELDS NEUTRINOS POSITRONS PULSARS Soft gamma ray repeaters SURFACES VIOLATIONS WHITE DWARF STARS X RADIATION |
title | SMWDs as SGRs/AXPs and the lepton number violation |
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