Has NANOGrav Found First Evidence for Cosmic Strings?
The North American Nanohertz Observatory for Gravitational Waves has recently reported strong evidence for a stochastic common-spectrum process affecting the pulsar timing residuals in its 12.5-year data set. We demonstrate that this process admits an interpretation in terms of a stochastic gravitat...
Gespeichert in:
| Veröffentlicht in: | Physical review letters 2021-01, Vol.126 (4), p.041305-041305, Article 041305 |
|---|---|
| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 041305 |
|---|---|
| container_issue | 4 |
| container_start_page | 041305 |
| container_title | Physical review letters |
| container_volume | 126 |
| creator | Blasi, Simone Brdar, Vedran Schmitz, Kai |
| description | The North American Nanohertz Observatory for Gravitational Waves has recently reported strong evidence for a stochastic common-spectrum process affecting the pulsar timing residuals in its 12.5-year data set. We demonstrate that this process admits an interpretation in terms of a stochastic gravitational-wave background emitted by a cosmic-string network in the early Universe. We study stable Nambu-Goto strings in dependence of their tension Gμ and loop size α and show that the entire viable parameter space will be probed by an array of future experiments. |
| doi_str_mv | 10.1103/PhysRevLett.126.041305 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_2489252196</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2489252196</sourcerecordid><originalsourceid>FETCH-LOGICAL-c476t-7216a4580910398c35c29410a4bee5fd50b17c1fb9dc2ac84904735730b47c393</originalsourceid><addsrcrecordid>eNpdkF1LwzAYhYMobk7_wih4403n-zZJ01zJGPsQxiZ-XIc2TbVjbWfSDvbvjWyKeHVunnM4PIQMEUaIQO-fPg7u2eyXpm1HGMUjYEiBn5E-gpChQGTnpA9AMZQAokeunNsAgEeTS9KjlIs45qJP-CJ1wWq8Ws9tug9mTVfnway0rg2m-zI3tTZB0dhg0riq1MFLa8v63T1ck4si3Tpzc8oBeZtNXyeLcLmeP07Gy1AzEbehiDBOGU9A-ssy0ZTrSDKElGXG8CLnkKHQWGQy11GqEyaBCX-NQsaEppIOyN1xd2ebz864VlWl02a7TWvTdE5FLJERj1DGHr39h26aztb-nack54AC0FPxkdK2cc6aQu1sWaX2oBDUt1j1R6zyttRRrC8OT_NdVpn8t_Zjkn4Bi45zQw</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2495501701</pqid></control><display><type>article</type><title>Has NANOGrav Found First Evidence for Cosmic Strings?</title><source>American Physical Society Journals</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><creator>Blasi, Simone ; Brdar, Vedran ; Schmitz, Kai</creator><creatorcontrib>Blasi, Simone ; Brdar, Vedran ; Schmitz, Kai</creatorcontrib><description>The North American Nanohertz Observatory for Gravitational Waves has recently reported strong evidence for a stochastic common-spectrum process affecting the pulsar timing residuals in its 12.5-year data set. We demonstrate that this process admits an interpretation in terms of a stochastic gravitational-wave background emitted by a cosmic-string network in the early Universe. We study stable Nambu-Goto strings in dependence of their tension Gμ and loop size α and show that the entire viable parameter space will be probed by an array of future experiments.</description><identifier>ISSN: 0031-9007</identifier><identifier>EISSN: 1079-7114</identifier><identifier>DOI: 10.1103/PhysRevLett.126.041305</identifier><identifier>PMID: 33576657</identifier><language>eng</language><publisher>United States: American Physical Society</publisher><subject>Gravitation ; Gravitational waves ; Pulsars ; Strings</subject><ispartof>Physical review letters, 2021-01, Vol.126 (4), p.041305-041305, Article 041305</ispartof><rights>Copyright American Physical Society Jan 29, 2021</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c476t-7216a4580910398c35c29410a4bee5fd50b17c1fb9dc2ac84904735730b47c393</citedby><cites>FETCH-LOGICAL-c476t-7216a4580910398c35c29410a4bee5fd50b17c1fb9dc2ac84904735730b47c393</cites><orcidid>0000-0003-2807-6472</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,2863,2864,27901,27902</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/33576657$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Blasi, Simone</creatorcontrib><creatorcontrib>Brdar, Vedran</creatorcontrib><creatorcontrib>Schmitz, Kai</creatorcontrib><title>Has NANOGrav Found First Evidence for Cosmic Strings?</title><title>Physical review letters</title><addtitle>Phys Rev Lett</addtitle><description>The North American Nanohertz Observatory for Gravitational Waves has recently reported strong evidence for a stochastic common-spectrum process affecting the pulsar timing residuals in its 12.5-year data set. We demonstrate that this process admits an interpretation in terms of a stochastic gravitational-wave background emitted by a cosmic-string network in the early Universe. We study stable Nambu-Goto strings in dependence of their tension Gμ and loop size α and show that the entire viable parameter space will be probed by an array of future experiments.</description><subject>Gravitation</subject><subject>Gravitational waves</subject><subject>Pulsars</subject><subject>Strings</subject><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNpdkF1LwzAYhYMobk7_wih4403n-zZJ01zJGPsQxiZ-XIc2TbVjbWfSDvbvjWyKeHVunnM4PIQMEUaIQO-fPg7u2eyXpm1HGMUjYEiBn5E-gpChQGTnpA9AMZQAokeunNsAgEeTS9KjlIs45qJP-CJ1wWq8Ws9tug9mTVfnway0rg2m-zI3tTZB0dhg0riq1MFLa8v63T1ck4si3Tpzc8oBeZtNXyeLcLmeP07Gy1AzEbehiDBOGU9A-ssy0ZTrSDKElGXG8CLnkKHQWGQy11GqEyaBCX-NQsaEppIOyN1xd2ebz864VlWl02a7TWvTdE5FLJERj1DGHr39h26aztb-nack54AC0FPxkdK2cc6aQu1sWaX2oBDUt1j1R6zyttRRrC8OT_NdVpn8t_Zjkn4Bi45zQw</recordid><startdate>20210129</startdate><enddate>20210129</enddate><creator>Blasi, Simone</creator><creator>Brdar, Vedran</creator><creator>Schmitz, Kai</creator><general>American Physical Society</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7X8</scope><orcidid>https://orcid.org/0000-0003-2807-6472</orcidid></search><sort><creationdate>20210129</creationdate><title>Has NANOGrav Found First Evidence for Cosmic Strings?</title><author>Blasi, Simone ; Brdar, Vedran ; Schmitz, Kai</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c476t-7216a4580910398c35c29410a4bee5fd50b17c1fb9dc2ac84904735730b47c393</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Gravitation</topic><topic>Gravitational waves</topic><topic>Pulsars</topic><topic>Strings</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Blasi, Simone</creatorcontrib><creatorcontrib>Brdar, Vedran</creatorcontrib><creatorcontrib>Schmitz, Kai</creatorcontrib><collection>PubMed</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><collection>MEDLINE - Academic</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Blasi, Simone</au><au>Brdar, Vedran</au><au>Schmitz, Kai</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Has NANOGrav Found First Evidence for Cosmic Strings?</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2021-01-29</date><risdate>2021</risdate><volume>126</volume><issue>4</issue><spage>041305</spage><epage>041305</epage><pages>041305-041305</pages><artnum>041305</artnum><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>The North American Nanohertz Observatory for Gravitational Waves has recently reported strong evidence for a stochastic common-spectrum process affecting the pulsar timing residuals in its 12.5-year data set. We demonstrate that this process admits an interpretation in terms of a stochastic gravitational-wave background emitted by a cosmic-string network in the early Universe. We study stable Nambu-Goto strings in dependence of their tension Gμ and loop size α and show that the entire viable parameter space will be probed by an array of future experiments.</abstract><cop>United States</cop><pub>American Physical Society</pub><pmid>33576657</pmid><doi>10.1103/PhysRevLett.126.041305</doi><tpages>1</tpages><orcidid>https://orcid.org/0000-0003-2807-6472</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0031-9007 |
| ispartof | Physical review letters, 2021-01, Vol.126 (4), p.041305-041305, Article 041305 |
| issn | 0031-9007 1079-7114 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_2489252196 |
| source | American Physical Society Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals |
| subjects | Gravitation Gravitational waves Pulsars Strings |
| title | Has NANOGrav Found First Evidence for Cosmic Strings? |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-16T10%3A05%3A40IST&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=Has%20NANOGrav%20Found%20First%20Evidence%20for%20Cosmic%20Strings?&rft.jtitle=Physical%20review%20letters&rft.au=Blasi,%20Simone&rft.date=2021-01-29&rft.volume=126&rft.issue=4&rft.spage=041305&rft.epage=041305&rft.pages=041305-041305&rft.artnum=041305&rft.issn=0031-9007&rft.eissn=1079-7114&rft_id=info:doi/10.1103/PhysRevLett.126.041305&rft_dat=%3Cproquest_cross%3E2489252196%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=2495501701&rft_id=info:pmid/33576657&rfr_iscdi=true |