Gravitational radiation background from boson star binaries

We calculate the gravitational radiation background generated from boson star binaries formed in locally dense clusters with formation rate tracked by the regular star formation rate. We compute how the frequency window in gravitational waves is affected by the boson field mass and repulsive self-co...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physics letters. B 2018-08, Vol.783 (C), p.158-162
Hauptverfasser: Croon, Djuna, Gleiser, Marcelo, Mohapatra, Sonali, Sun, Chen
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 162
container_issue C
container_start_page 158
container_title Physics letters. B
container_volume 783
creator Croon, Djuna
Gleiser, Marcelo
Mohapatra, Sonali
Sun, Chen
description We calculate the gravitational radiation background generated from boson star binaries formed in locally dense clusters with formation rate tracked by the regular star formation rate. We compute how the frequency window in gravitational waves is affected by the boson field mass and repulsive self-coupling, anticipating constraints from EPTA and LISA. We also comment on the possible detectability of these binaries.
doi_str_mv 10.1016/j.physletb.2018.03.055
format Article
fullrecord <record><control><sourceid>elsevier_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_1438055</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S037026931830251X</els_id><sourcerecordid>S037026931830251X</sourcerecordid><originalsourceid>FETCH-LOGICAL-c387t-39348f321ff83468bc83d00f3ba6162a465efc4ecc5a9e10bc2285ab7a5b78f53</originalsourceid><addsrcrecordid>eNqFUF1LwzAUDaLgnP4FKb633iRNmuGLMnQKA1_0OSRp4lK3ZiRxsH9va_XZp3u4nA_OQegaQ4UB89uu2m-OaWuzrghgUQGtgLETNMOioSWpa3aKZkAbKAlf0HN0kVIHAJgBn6G7VVQHn1X2oVfbIqrW_-BCK_P5EcNX3xYuhl2hQxq-KatYaN-r6G26RGdObZO9-r1z9P70-LZ8Ltevq5flw7o0VDS5pAtaC0cJdk7QmgttBG0BHNWKY05UzZl1prbGMLWwGLQhRDClG8V0Ixyjc3Qz-YaUvUzGZ2s2JvS9NVnimoqh7kDiE8nEkFK0Tu6j36l4lBjkuJPs5N9OctxJApWT8H4S2qHCwds4Jtje2NbHMaAN_j-Lb4__dV8</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Gravitational radiation background from boson star binaries</title><source>DOAJ Directory of Open Access Journals</source><source>ScienceDirect Journals (5 years ago - present)</source><source>EZB-FREE-00999 freely available EZB journals</source><creator>Croon, Djuna ; Gleiser, Marcelo ; Mohapatra, Sonali ; Sun, Chen</creator><creatorcontrib>Croon, Djuna ; Gleiser, Marcelo ; Mohapatra, Sonali ; Sun, Chen ; Dartmouth College, Hanover, NH (United States)</creatorcontrib><description>We calculate the gravitational radiation background generated from boson star binaries formed in locally dense clusters with formation rate tracked by the regular star formation rate. We compute how the frequency window in gravitational waves is affected by the boson field mass and repulsive self-coupling, anticipating constraints from EPTA and LISA. We also comment on the possible detectability of these binaries.</description><identifier>ISSN: 0370-2693</identifier><identifier>EISSN: 1873-2445</identifier><identifier>DOI: 10.1016/j.physletb.2018.03.055</identifier><language>eng</language><publisher>Netherlands: Elsevier B.V</publisher><subject>ASTRONOMY AND ASTROPHYSICS</subject><ispartof>Physics letters. B, 2018-08, Vol.783 (C), p.158-162</ispartof><rights>2018 The Authors</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c387t-39348f321ff83468bc83d00f3ba6162a465efc4ecc5a9e10bc2285ab7a5b78f53</citedby><cites>FETCH-LOGICAL-c387t-39348f321ff83468bc83d00f3ba6162a465efc4ecc5a9e10bc2285ab7a5b78f53</cites><orcidid>0000-0003-3359-3706 ; 0000000333593706</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/j.physletb.2018.03.055$$EHTML$$P50$$Gelsevier$$Hfree_for_read</linktohtml><link.rule.ids>230,314,780,784,864,885,3548,27923,27924,45994</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/1438055$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Croon, Djuna</creatorcontrib><creatorcontrib>Gleiser, Marcelo</creatorcontrib><creatorcontrib>Mohapatra, Sonali</creatorcontrib><creatorcontrib>Sun, Chen</creatorcontrib><creatorcontrib>Dartmouth College, Hanover, NH (United States)</creatorcontrib><title>Gravitational radiation background from boson star binaries</title><title>Physics letters. B</title><description>We calculate the gravitational radiation background generated from boson star binaries formed in locally dense clusters with formation rate tracked by the regular star formation rate. We compute how the frequency window in gravitational waves is affected by the boson field mass and repulsive self-coupling, anticipating constraints from EPTA and LISA. We also comment on the possible detectability of these binaries.</description><subject>ASTRONOMY AND ASTROPHYSICS</subject><issn>0370-2693</issn><issn>1873-2445</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNqFUF1LwzAUDaLgnP4FKb633iRNmuGLMnQKA1_0OSRp4lK3ZiRxsH9va_XZp3u4nA_OQegaQ4UB89uu2m-OaWuzrghgUQGtgLETNMOioSWpa3aKZkAbKAlf0HN0kVIHAJgBn6G7VVQHn1X2oVfbIqrW_-BCK_P5EcNX3xYuhl2hQxq-KatYaN-r6G26RGdObZO9-r1z9P70-LZ8Ltevq5flw7o0VDS5pAtaC0cJdk7QmgttBG0BHNWKY05UzZl1prbGMLWwGLQhRDClG8V0Ixyjc3Qz-YaUvUzGZ2s2JvS9NVnimoqh7kDiE8nEkFK0Tu6j36l4lBjkuJPs5N9OctxJApWT8H4S2qHCwds4Jtje2NbHMaAN_j-Lb4__dV8</recordid><startdate>20180810</startdate><enddate>20180810</enddate><creator>Croon, Djuna</creator><creator>Gleiser, Marcelo</creator><creator>Mohapatra, Sonali</creator><creator>Sun, Chen</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>6I.</scope><scope>AAFTH</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0003-3359-3706</orcidid><orcidid>https://orcid.org/0000000333593706</orcidid></search><sort><creationdate>20180810</creationdate><title>Gravitational radiation background from boson star binaries</title><author>Croon, Djuna ; Gleiser, Marcelo ; Mohapatra, Sonali ; Sun, Chen</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c387t-39348f321ff83468bc83d00f3ba6162a465efc4ecc5a9e10bc2285ab7a5b78f53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>ASTRONOMY AND ASTROPHYSICS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Croon, Djuna</creatorcontrib><creatorcontrib>Gleiser, Marcelo</creatorcontrib><creatorcontrib>Mohapatra, Sonali</creatorcontrib><creatorcontrib>Sun, Chen</creatorcontrib><creatorcontrib>Dartmouth College, Hanover, NH (United States)</creatorcontrib><collection>ScienceDirect Open Access Titles</collection><collection>Elsevier:ScienceDirect:Open Access</collection><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Physics letters. B</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Croon, Djuna</au><au>Gleiser, Marcelo</au><au>Mohapatra, Sonali</au><au>Sun, Chen</au><aucorp>Dartmouth College, Hanover, NH (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Gravitational radiation background from boson star binaries</atitle><jtitle>Physics letters. B</jtitle><date>2018-08-10</date><risdate>2018</risdate><volume>783</volume><issue>C</issue><spage>158</spage><epage>162</epage><pages>158-162</pages><issn>0370-2693</issn><eissn>1873-2445</eissn><abstract>We calculate the gravitational radiation background generated from boson star binaries formed in locally dense clusters with formation rate tracked by the regular star formation rate. We compute how the frequency window in gravitational waves is affected by the boson field mass and repulsive self-coupling, anticipating constraints from EPTA and LISA. We also comment on the possible detectability of these binaries.</abstract><cop>Netherlands</cop><pub>Elsevier B.V</pub><doi>10.1016/j.physletb.2018.03.055</doi><tpages>5</tpages><orcidid>https://orcid.org/0000-0003-3359-3706</orcidid><orcidid>https://orcid.org/0000000333593706</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0370-2693
ispartof Physics letters. B, 2018-08, Vol.783 (C), p.158-162
issn 0370-2693
1873-2445
language eng
recordid cdi_osti_scitechconnect_1438055
source DOAJ Directory of Open Access Journals; ScienceDirect Journals (5 years ago - present); EZB-FREE-00999 freely available EZB journals
subjects ASTRONOMY AND ASTROPHYSICS
title Gravitational radiation background from boson star binaries
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-11T19%3A23%3A51IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-elsevier_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Gravitational%20radiation%20background%20from%20boson%20star%20binaries&rft.jtitle=Physics%20letters.%20B&rft.au=Croon,%20Djuna&rft.aucorp=Dartmouth%20College,%20Hanover,%20NH%20(United%20States)&rft.date=2018-08-10&rft.volume=783&rft.issue=C&rft.spage=158&rft.epage=162&rft.pages=158-162&rft.issn=0370-2693&rft.eissn=1873-2445&rft_id=info:doi/10.1016/j.physletb.2018.03.055&rft_dat=%3Celsevier_osti_%3ES037026931830251X%3C/elsevier_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rft_els_id=S037026931830251X&rfr_iscdi=true