Parametric instability induced scalar gravitational waves from a model pulsating neutron star
We identify a new dynamical mechanism for a strong scalar gravitational field effect. To illustrate this mechanism, we investigate the parametric excitation and emission of scalar gravitational waves by a radially pulsating model neutron star.
Gespeichert in:
| Veröffentlicht in: | Physics letters. B 2011-11, Vol.705 (1-2), p.148-151 |
|---|---|
| Hauptverfasser: | , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 151 |
|---|---|
| container_issue | 1-2 |
| container_start_page | 148 |
| container_title | Physics letters. B |
| container_volume | 705 |
| creator | Wang, Charles H.-T. Bonifacio, Paolo M. Bingham, Robert Mendonça, J. Tito |
| description | We identify a new dynamical mechanism for a strong scalar gravitational field effect. To illustrate this mechanism, we investigate the parametric excitation and emission of scalar gravitational waves by a radially pulsating model neutron star. |
| doi_str_mv | 10.1016/j.physletb.2011.09.111 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_963860027</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S0370269311012111</els_id><sourcerecordid>963860027</sourcerecordid><originalsourceid>FETCH-LOGICAL-c422t-8e0cc0e2ca2d12bc9054f3d18a891fd202c7db241d7ab3fac3e507671908d07c3</originalsourceid><addsrcrecordid>eNqFkE1r3DAQhkVoIdtt_kLQJfRkZyR_31qWNgkE2kNyDGIsjRMtsr2V5A3776tlk15zmoF5P5iHsUsBuQBRX2_z3cshOIp9LkGIHLpcCHHGVqJtikyWZfWJraBoIJN1V5yzLyFsAUBUUK_Y0x_0OFL0VnM7hYi9dTYe0m4WTYYHjQ49f_a4txGjnSd0_BX3FPjg55EjH2dDju8WF9J5euYTLdHPE09Z_iv7PKALdPE21-zx18-HzW12__vmbvPjPtOllDFrCbQGkhqlEbLXHVTlUBjRYtuJwUiQujG9LIVpsC8G1AVV0NSN6KA10Ohizb6dcnd-_rtQiGq0QZNzONG8BNXVRVsDyCYp65NS-zkET4PaeTuiPygB6ohTbdU7TnXEqaBTCWcyXr1V4JHJ4HHSNvx3y6rs2hbKpPt-0lH6d2_Jq6AtTYml9aSjMrP9qOofZSaRCA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>963860027</pqid></control><display><type>article</type><title>Parametric instability induced scalar gravitational waves from a model pulsating neutron star</title><source>ScienceDirect Journals (5 years ago - present)</source><creator>Wang, Charles H.-T. ; Bonifacio, Paolo M. ; Bingham, Robert ; Mendonça, J. Tito</creator><creatorcontrib>Wang, Charles H.-T. ; Bonifacio, Paolo M. ; Bingham, Robert ; Mendonça, J. Tito</creatorcontrib><description>We identify a new dynamical mechanism for a strong scalar gravitational field effect. To illustrate this mechanism, we investigate the parametric excitation and emission of scalar gravitational waves by a radially pulsating model neutron star.</description><identifier>ISSN: 0370-2693</identifier><identifier>EISSN: 1873-2445</identifier><identifier>DOI: 10.1016/j.physletb.2011.09.111</identifier><identifier>CODEN: PYLBAJ</identifier><language>eng</language><publisher>Kidlington: Elsevier B.V</publisher><subject>Elementary particles ; Emission ; Emission analysis ; Exact sciences and technology ; General relativity ; Gravitational fields ; Gravitational waves ; Instability ; Neutron stars ; Nuclear physics ; Physics ; Pulsating stars ; Scalar waves ; Scalar-tensor gravity ; Scalars ; The physics of elementary particles and fields</subject><ispartof>Physics letters. B, 2011-11, Vol.705 (1-2), p.148-151</ispartof><rights>2011 Elsevier B.V.</rights><rights>2015 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c422t-8e0cc0e2ca2d12bc9054f3d18a891fd202c7db241d7ab3fac3e507671908d07c3</citedby><cites>FETCH-LOGICAL-c422t-8e0cc0e2ca2d12bc9054f3d18a891fd202c7db241d7ab3fac3e507671908d07c3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/j.physletb.2011.09.111$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,780,784,3548,27923,27924,45994</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=25498804$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Wang, Charles H.-T.</creatorcontrib><creatorcontrib>Bonifacio, Paolo M.</creatorcontrib><creatorcontrib>Bingham, Robert</creatorcontrib><creatorcontrib>Mendonça, J. Tito</creatorcontrib><title>Parametric instability induced scalar gravitational waves from a model pulsating neutron star</title><title>Physics letters. B</title><description>We identify a new dynamical mechanism for a strong scalar gravitational field effect. To illustrate this mechanism, we investigate the parametric excitation and emission of scalar gravitational waves by a radially pulsating model neutron star.</description><subject>Elementary particles</subject><subject>Emission</subject><subject>Emission analysis</subject><subject>Exact sciences and technology</subject><subject>General relativity</subject><subject>Gravitational fields</subject><subject>Gravitational waves</subject><subject>Instability</subject><subject>Neutron stars</subject><subject>Nuclear physics</subject><subject>Physics</subject><subject>Pulsating stars</subject><subject>Scalar waves</subject><subject>Scalar-tensor gravity</subject><subject>Scalars</subject><subject>The physics of elementary particles and fields</subject><issn>0370-2693</issn><issn>1873-2445</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNqFkE1r3DAQhkVoIdtt_kLQJfRkZyR_31qWNgkE2kNyDGIsjRMtsr2V5A3776tlk15zmoF5P5iHsUsBuQBRX2_z3cshOIp9LkGIHLpcCHHGVqJtikyWZfWJraBoIJN1V5yzLyFsAUBUUK_Y0x_0OFL0VnM7hYi9dTYe0m4WTYYHjQ49f_a4txGjnSd0_BX3FPjg55EjH2dDju8WF9J5euYTLdHPE09Z_iv7PKALdPE21-zx18-HzW12__vmbvPjPtOllDFrCbQGkhqlEbLXHVTlUBjRYtuJwUiQujG9LIVpsC8G1AVV0NSN6KA10Ohizb6dcnd-_rtQiGq0QZNzONG8BNXVRVsDyCYp65NS-zkET4PaeTuiPygB6ohTbdU7TnXEqaBTCWcyXr1V4JHJ4HHSNvx3y6rs2hbKpPt-0lH6d2_Jq6AtTYml9aSjMrP9qOofZSaRCA</recordid><startdate>20111103</startdate><enddate>20111103</enddate><creator>Wang, Charles H.-T.</creator><creator>Bonifacio, Paolo M.</creator><creator>Bingham, Robert</creator><creator>Mendonça, J. Tito</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20111103</creationdate><title>Parametric instability induced scalar gravitational waves from a model pulsating neutron star</title><author>Wang, Charles H.-T. ; Bonifacio, Paolo M. ; Bingham, Robert ; Mendonça, J. Tito</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c422t-8e0cc0e2ca2d12bc9054f3d18a891fd202c7db241d7ab3fac3e507671908d07c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>Elementary particles</topic><topic>Emission</topic><topic>Emission analysis</topic><topic>Exact sciences and technology</topic><topic>General relativity</topic><topic>Gravitational fields</topic><topic>Gravitational waves</topic><topic>Instability</topic><topic>Neutron stars</topic><topic>Nuclear physics</topic><topic>Physics</topic><topic>Pulsating stars</topic><topic>Scalar waves</topic><topic>Scalar-tensor gravity</topic><topic>Scalars</topic><topic>The physics of elementary particles and fields</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Wang, Charles H.-T.</creatorcontrib><creatorcontrib>Bonifacio, Paolo M.</creatorcontrib><creatorcontrib>Bingham, Robert</creatorcontrib><creatorcontrib>Mendonça, J. Tito</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physics letters. B</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wang, Charles H.-T.</au><au>Bonifacio, Paolo M.</au><au>Bingham, Robert</au><au>Mendonça, J. Tito</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Parametric instability induced scalar gravitational waves from a model pulsating neutron star</atitle><jtitle>Physics letters. B</jtitle><date>2011-11-03</date><risdate>2011</risdate><volume>705</volume><issue>1-2</issue><spage>148</spage><epage>151</epage><pages>148-151</pages><issn>0370-2693</issn><eissn>1873-2445</eissn><coden>PYLBAJ</coden><abstract>We identify a new dynamical mechanism for a strong scalar gravitational field effect. To illustrate this mechanism, we investigate the parametric excitation and emission of scalar gravitational waves by a radially pulsating model neutron star.</abstract><cop>Kidlington</cop><pub>Elsevier B.V</pub><doi>10.1016/j.physletb.2011.09.111</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0370-2693 |
| ispartof | Physics letters. B, 2011-11, Vol.705 (1-2), p.148-151 |
| issn | 0370-2693 1873-2445 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_963860027 |
| source | ScienceDirect Journals (5 years ago - present) |
| subjects | Elementary particles Emission Emission analysis Exact sciences and technology General relativity Gravitational fields Gravitational waves Instability Neutron stars Nuclear physics Physics Pulsating stars Scalar waves Scalar-tensor gravity Scalars The physics of elementary particles and fields |
| title | Parametric instability induced scalar gravitational waves from a model pulsating neutron star |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-11T12%3A32%3A14IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Parametric%20instability%20induced%20scalar%20gravitational%20waves%20from%20a%20model%20pulsating%20neutron%20star&rft.jtitle=Physics%20letters.%20B&rft.au=Wang,%20Charles%20H.-T.&rft.date=2011-11-03&rft.volume=705&rft.issue=1-2&rft.spage=148&rft.epage=151&rft.pages=148-151&rft.issn=0370-2693&rft.eissn=1873-2445&rft.coden=PYLBAJ&rft_id=info:doi/10.1016/j.physletb.2011.09.111&rft_dat=%3Cproquest_cross%3E963860027%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=963860027&rft_id=info:pmid/&rft_els_id=S0370269311012111&rfr_iscdi=true |