Non-linear Higgs portal to Dark Matter
A bstract The Higgs portal to scalar Dark Matter is considered in the context of non-linearly realised electroweak symmetry breaking. We determine the dominant interactions of gauge bosons and the physical Higgs particle h to a scalar singlet Dark Matter candidate. Phenomenological consequences are...
Gespeichert in:
Veröffentlicht in: | The journal of high energy physics 2016-04, Vol.2016 (4), p.1-35 |
---|---|
Hauptverfasser: | , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 35 |
---|---|
container_issue | 4 |
container_start_page | 1 |
container_title | The journal of high energy physics |
container_volume | 2016 |
creator | Brivio, I. Gavela, M. B. Merlo, L. Mimasu, K. No, J. M. del Rey, R. Sanz, V. |
description | A
bstract
The Higgs portal to scalar Dark Matter is considered in the context of non-linearly realised electroweak symmetry breaking. We determine the dominant interactions of gauge bosons and the physical Higgs particle
h
to a scalar singlet Dark Matter candidate. Phenomenological consequences are also studied in detail, including the possibility of distinguishing this scenario from the standard Higgs portal in which the electroweak symmetry breaking is linearly realised. Two features of significant impact are: i) the connection between the electroweak scale
v
and the Higgs particle departs from the (
v
+
h
) functional dependence, as the Higgs field is not necessarily an exact electroweak doublet; ii) the presence of specific couplings that arise at different order in the non-linear and in the linear expansions. These facts deeply affect the Dark Matter relic abundance, as well as the expected signals in direct and indirect searches and collider phenomenology, where Dark Matter production rates are enhanced with respect to the standard portal. |
doi_str_mv | 10.1007/JHEP04(2016)141 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1808104671</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1808104671</sourcerecordid><originalsourceid>FETCH-LOGICAL-c356t-6f127076b0e8faf2341f36a114dc7bd2c6f780fd6bb19c0bf066602256cc84203</originalsourceid><addsrcrecordid>eNp1kD1PwzAQQC0EEqUws2ZCZQi9cxw7GVEpFFQ-Bpgtx7GjlDQOdjLw70kVBhamu-G9k-4RcolwgwBi-bRZvwFbUEB-jQyPyAyB5nHGRH78Zz8lZyHsADDFHGbk6sW1cVO3RvloU1dViDrne9VEvYvulP-MnlXfG39OTqxqgrn4nXPycb9-X23i7evD4-p2G-sk5X3MLVIBghdgMqssTRjahCtEVmpRlFRzKzKwJS8KzDUUFjjnQGnKtc4YhWROFtPdzruvwYRe7uugTdOo1rghSMwgQ2Bc4IguJ1R7F4I3Vna-3iv_LRHkoYicishDETkWGQ2YjDCSbWW83LnBt-M__yo_e0tgXw</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1808104671</pqid></control><display><type>article</type><title>Non-linear Higgs portal to Dark Matter</title><source>DOAJ Directory of Open Access Journals</source><source>Springer Nature OA Free Journals</source><source>EZB-FREE-00999 freely available EZB journals</source><source>Alma/SFX Local Collection</source><creator>Brivio, I. ; Gavela, M. B. ; Merlo, L. ; Mimasu, K. ; No, J. M. ; del Rey, R. ; Sanz, V.</creator><creatorcontrib>Brivio, I. ; Gavela, M. B. ; Merlo, L. ; Mimasu, K. ; No, J. M. ; del Rey, R. ; Sanz, V.</creatorcontrib><description>A
bstract
The Higgs portal to scalar Dark Matter is considered in the context of non-linearly realised electroweak symmetry breaking. We determine the dominant interactions of gauge bosons and the physical Higgs particle
h
to a scalar singlet Dark Matter candidate. Phenomenological consequences are also studied in detail, including the possibility of distinguishing this scenario from the standard Higgs portal in which the electroweak symmetry breaking is linearly realised. Two features of significant impact are: i) the connection between the electroweak scale
v
and the Higgs particle departs from the (
v
+
h
) functional dependence, as the Higgs field is not necessarily an exact electroweak doublet; ii) the presence of specific couplings that arise at different order in the non-linear and in the linear expansions. These facts deeply affect the Dark Matter relic abundance, as well as the expected signals in direct and indirect searches and collider phenomenology, where Dark Matter production rates are enhanced with respect to the standard portal.</description><identifier>ISSN: 1029-8479</identifier><identifier>EISSN: 1029-8479</identifier><identifier>DOI: 10.1007/JHEP04(2016)141</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Bosons ; Broken symmetry ; Classical and Quantum Gravitation ; Couplings ; Dark matter ; Elementary Particles ; Higgs particles ; Nonlinearity ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Quantum Physics ; Regular Article - Theoretical Physics ; Relativity Theory ; Scalars ; String Theory</subject><ispartof>The journal of high energy physics, 2016-04, Vol.2016 (4), p.1-35</ispartof><rights>The Author(s) 2016</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c356t-6f127076b0e8faf2341f36a114dc7bd2c6f780fd6bb19c0bf066602256cc84203</citedby><cites>FETCH-LOGICAL-c356t-6f127076b0e8faf2341f36a114dc7bd2c6f780fd6bb19c0bf066602256cc84203</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/JHEP04(2016)141$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://doi.org/10.1007/JHEP04(2016)141$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>314,777,781,861,27905,27906,41101,42170,51557</link.rule.ids></links><search><creatorcontrib>Brivio, I.</creatorcontrib><creatorcontrib>Gavela, M. B.</creatorcontrib><creatorcontrib>Merlo, L.</creatorcontrib><creatorcontrib>Mimasu, K.</creatorcontrib><creatorcontrib>No, J. M.</creatorcontrib><creatorcontrib>del Rey, R.</creatorcontrib><creatorcontrib>Sanz, V.</creatorcontrib><title>Non-linear Higgs portal to Dark Matter</title><title>The journal of high energy physics</title><addtitle>J. High Energ. Phys</addtitle><description>A
bstract
The Higgs portal to scalar Dark Matter is considered in the context of non-linearly realised electroweak symmetry breaking. We determine the dominant interactions of gauge bosons and the physical Higgs particle
h
to a scalar singlet Dark Matter candidate. Phenomenological consequences are also studied in detail, including the possibility of distinguishing this scenario from the standard Higgs portal in which the electroweak symmetry breaking is linearly realised. Two features of significant impact are: i) the connection between the electroweak scale
v
and the Higgs particle departs from the (
v
+
h
) functional dependence, as the Higgs field is not necessarily an exact electroweak doublet; ii) the presence of specific couplings that arise at different order in the non-linear and in the linear expansions. These facts deeply affect the Dark Matter relic abundance, as well as the expected signals in direct and indirect searches and collider phenomenology, where Dark Matter production rates are enhanced with respect to the standard portal.</description><subject>Bosons</subject><subject>Broken symmetry</subject><subject>Classical and Quantum Gravitation</subject><subject>Couplings</subject><subject>Dark matter</subject><subject>Elementary Particles</subject><subject>Higgs particles</subject><subject>Nonlinearity</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Regular Article - Theoretical Physics</subject><subject>Relativity Theory</subject><subject>Scalars</subject><subject>String Theory</subject><issn>1029-8479</issn><issn>1029-8479</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><recordid>eNp1kD1PwzAQQC0EEqUws2ZCZQi9cxw7GVEpFFQ-Bpgtx7GjlDQOdjLw70kVBhamu-G9k-4RcolwgwBi-bRZvwFbUEB-jQyPyAyB5nHGRH78Zz8lZyHsADDFHGbk6sW1cVO3RvloU1dViDrne9VEvYvulP-MnlXfG39OTqxqgrn4nXPycb9-X23i7evD4-p2G-sk5X3MLVIBghdgMqssTRjahCtEVmpRlFRzKzKwJS8KzDUUFjjnQGnKtc4YhWROFtPdzruvwYRe7uugTdOo1rghSMwgQ2Bc4IguJ1R7F4I3Vna-3iv_LRHkoYicishDETkWGQ2YjDCSbWW83LnBt-M__yo_e0tgXw</recordid><startdate>20160401</startdate><enddate>20160401</enddate><creator>Brivio, I.</creator><creator>Gavela, M. B.</creator><creator>Merlo, L.</creator><creator>Mimasu, K.</creator><creator>No, J. M.</creator><creator>del Rey, R.</creator><creator>Sanz, V.</creator><general>Springer Berlin Heidelberg</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20160401</creationdate><title>Non-linear Higgs portal to Dark Matter</title><author>Brivio, I. ; Gavela, M. B. ; Merlo, L. ; Mimasu, K. ; No, J. M. ; del Rey, R. ; Sanz, V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c356t-6f127076b0e8faf2341f36a114dc7bd2c6f780fd6bb19c0bf066602256cc84203</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Bosons</topic><topic>Broken symmetry</topic><topic>Classical and Quantum Gravitation</topic><topic>Couplings</topic><topic>Dark matter</topic><topic>Elementary Particles</topic><topic>Higgs particles</topic><topic>Nonlinearity</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Quantum Physics</topic><topic>Regular Article - Theoretical Physics</topic><topic>Relativity Theory</topic><topic>Scalars</topic><topic>String Theory</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Brivio, I.</creatorcontrib><creatorcontrib>Gavela, M. B.</creatorcontrib><creatorcontrib>Merlo, L.</creatorcontrib><creatorcontrib>Mimasu, K.</creatorcontrib><creatorcontrib>No, J. M.</creatorcontrib><creatorcontrib>del Rey, R.</creatorcontrib><creatorcontrib>Sanz, V.</creatorcontrib><collection>Springer Nature OA Free Journals</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>The journal of high energy physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Brivio, I.</au><au>Gavela, M. B.</au><au>Merlo, L.</au><au>Mimasu, K.</au><au>No, J. M.</au><au>del Rey, R.</au><au>Sanz, V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Non-linear Higgs portal to Dark Matter</atitle><jtitle>The journal of high energy physics</jtitle><stitle>J. High Energ. Phys</stitle><date>2016-04-01</date><risdate>2016</risdate><volume>2016</volume><issue>4</issue><spage>1</spage><epage>35</epage><pages>1-35</pages><issn>1029-8479</issn><eissn>1029-8479</eissn><abstract>A
bstract
The Higgs portal to scalar Dark Matter is considered in the context of non-linearly realised electroweak symmetry breaking. We determine the dominant interactions of gauge bosons and the physical Higgs particle
h
to a scalar singlet Dark Matter candidate. Phenomenological consequences are also studied in detail, including the possibility of distinguishing this scenario from the standard Higgs portal in which the electroweak symmetry breaking is linearly realised. Two features of significant impact are: i) the connection between the electroweak scale
v
and the Higgs particle departs from the (
v
+
h
) functional dependence, as the Higgs field is not necessarily an exact electroweak doublet; ii) the presence of specific couplings that arise at different order in the non-linear and in the linear expansions. These facts deeply affect the Dark Matter relic abundance, as well as the expected signals in direct and indirect searches and collider phenomenology, where Dark Matter production rates are enhanced with respect to the standard portal.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1007/JHEP04(2016)141</doi><tpages>35</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1029-8479 |
ispartof | The journal of high energy physics, 2016-04, Vol.2016 (4), p.1-35 |
issn | 1029-8479 1029-8479 |
language | eng |
recordid | cdi_proquest_miscellaneous_1808104671 |
source | DOAJ Directory of Open Access Journals; Springer Nature OA Free Journals; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection |
subjects | Bosons Broken symmetry Classical and Quantum Gravitation Couplings Dark matter Elementary Particles Higgs particles Nonlinearity Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Quantum Physics Regular Article - Theoretical Physics Relativity Theory Scalars String Theory |
title | Non-linear Higgs portal to Dark Matter |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-21T07%3A27%3A56IST&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=Non-linear%20Higgs%20portal%20to%20Dark%20Matter&rft.jtitle=The%20journal%20of%20high%20energy%20physics&rft.au=Brivio,%20I.&rft.date=2016-04-01&rft.volume=2016&rft.issue=4&rft.spage=1&rft.epage=35&rft.pages=1-35&rft.issn=1029-8479&rft.eissn=1029-8479&rft_id=info:doi/10.1007/JHEP04(2016)141&rft_dat=%3Cproquest_cross%3E1808104671%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=1808104671&rft_id=info:pmid/&rfr_iscdi=true |