Loading…

Perspectives of direct detection of supersymmetric dark matter in the NMSSM

In the Next-to-Minimal-Supersymmetric-Standard-Model (NMSSM) the lightest supersymmetric particle (LSP) is a candidate for the dark matter (DM) in the universe. It is a mixture from the various gauginos and Higgsinos and can be bino-, Higgsino- or singlino-dominated. Singlino-dominated LSPs can have...

Full description

Saved in:
Bibliographic Details
Published in:Physics letters. B 2017-08, Vol.771, p.611-618
Main Authors: Beskidt, C., de Boer, W., Kazakov, D.I., Wayand, S.
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c426t-1be507e26a1457ec020698f0039865d6b820fe1ec0533f55f704b0be4e5df9093
cites cdi_FETCH-LOGICAL-c426t-1be507e26a1457ec020698f0039865d6b820fe1ec0533f55f704b0be4e5df9093
container_end_page 618
container_issue
container_start_page 611
container_title Physics letters. B
container_volume 771
creator Beskidt, C.
de Boer, W.
Kazakov, D.I.
Wayand, S.
description In the Next-to-Minimal-Supersymmetric-Standard-Model (NMSSM) the lightest supersymmetric particle (LSP) is a candidate for the dark matter (DM) in the universe. It is a mixture from the various gauginos and Higgsinos and can be bino-, Higgsino- or singlino-dominated. Singlino-dominated LSPs can have very low cross sections below the neutrino background from coherent neutrino scattering which is limiting the sensitivity of future direct DM search experiments. However, previous studies suggested that the combination of both, the spin-dependent (SD) and spin-independent (SI) searches are sensitive in complementary regions of parameter space, so considering both searches will allow to explore practically the whole parameter space of the NMSSM. In this letter, the different scenarios are investigated with a new scanning technique, which reveals that significant regions of the NMSSM parameter space cannot be explored, even if one considers both, SI and SD, searches.
doi_str_mv 10.1016/j.physletb.2017.06.016
format article
fullrecord <record><control><sourceid>elsevier_doaj_</sourceid><recordid>TN_cdi_doaj_primary_oai_doaj_org_article_37a12b79cb3c4a5cb5fd162b4e07810a</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S0370269317304835</els_id><doaj_id>oai_doaj_org_article_37a12b79cb3c4a5cb5fd162b4e07810a</doaj_id><sourcerecordid>S0370269317304835</sourcerecordid><originalsourceid>FETCH-LOGICAL-c426t-1be507e26a1457ec020698f0039865d6b820fe1ec0533f55f704b0be4e5df9093</originalsourceid><addsrcrecordid>eNqFkNtOAyEQhonRxHp4BbMvsOsAC-zeaYyHxmOiXhNgB6W23QbQpG8vtcZbrwgfM98wPyEnFBoKVJ7OmtX7Os0x24YBVQ3IpuAdMqGd4jVrW7FLJsAV1Ez2fJ8cpDQDACpATsjtE8a0QpfDF6Zq9NUQYrlVA-YNHJcblj5XpWq9WGCOwVWDiR_VwuSMsQrLKr9j9XD__Hx_RPa8mSc8_j0PyevV5cvFTX33eD29OL-rXctkrqlFAQqZNLQVCh0wkH3nAXjfSTFI2zHwSMuD4NwL4RW0Fiy2KAbfQ88PyXTrHUYz06sYFiau9WiC_gFjfNMm5uDmqLkylFnVO8tda4Szwg9UMtsiqI6CKS65dbk4phTR__ko6E28ukz4jVdv4tUgdcGl8WzbiGXTr4BRJxdw6XAbYPlK-E_xDQkAhws</addsrcrecordid><sourcetype>Open Website</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Perspectives of direct detection of supersymmetric dark matter in the NMSSM</title><source>Elsevier</source><source>Elsevier ScienceDirect Journals</source><creator>Beskidt, C. ; de Boer, W. ; Kazakov, D.I. ; Wayand, S.</creator><creatorcontrib>Beskidt, C. ; de Boer, W. ; Kazakov, D.I. ; Wayand, S.</creatorcontrib><description>In the Next-to-Minimal-Supersymmetric-Standard-Model (NMSSM) the lightest supersymmetric particle (LSP) is a candidate for the dark matter (DM) in the universe. It is a mixture from the various gauginos and Higgsinos and can be bino-, Higgsino- or singlino-dominated. Singlino-dominated LSPs can have very low cross sections below the neutrino background from coherent neutrino scattering which is limiting the sensitivity of future direct DM search experiments. However, previous studies suggested that the combination of both, the spin-dependent (SD) and spin-independent (SI) searches are sensitive in complementary regions of parameter space, so considering both searches will allow to explore practically the whole parameter space of the NMSSM. In this letter, the different scenarios are investigated with a new scanning technique, which reveals that significant regions of the NMSSM parameter space cannot be explored, even if one considers both, SI and SD, searches.</description><identifier>ISSN: 0370-2693</identifier><identifier>EISSN: 1873-2445</identifier><identifier>DOI: 10.1016/j.physletb.2017.06.016</identifier><language>eng</language><publisher>Elsevier B.V</publisher><subject>Dark matter ; Direct dark matter searches ; NMSSM ; Spin dependent dark matter cross section ; Spin independent dark matter cross section ; Supersymmetry</subject><ispartof>Physics letters. B, 2017-08, Vol.771, p.611-618</ispartof><rights>2017 The Authors</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c426t-1be507e26a1457ec020698f0039865d6b820fe1ec0533f55f704b0be4e5df9093</citedby><cites>FETCH-LOGICAL-c426t-1be507e26a1457ec020698f0039865d6b820fe1ec0533f55f704b0be4e5df9093</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/S0370269317304835$$EHTML$$P50$$Gelsevier$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,3549,27924,27925,45780</link.rule.ids></links><search><creatorcontrib>Beskidt, C.</creatorcontrib><creatorcontrib>de Boer, W.</creatorcontrib><creatorcontrib>Kazakov, D.I.</creatorcontrib><creatorcontrib>Wayand, S.</creatorcontrib><title>Perspectives of direct detection of supersymmetric dark matter in the NMSSM</title><title>Physics letters. B</title><description>In the Next-to-Minimal-Supersymmetric-Standard-Model (NMSSM) the lightest supersymmetric particle (LSP) is a candidate for the dark matter (DM) in the universe. It is a mixture from the various gauginos and Higgsinos and can be bino-, Higgsino- or singlino-dominated. Singlino-dominated LSPs can have very low cross sections below the neutrino background from coherent neutrino scattering which is limiting the sensitivity of future direct DM search experiments. However, previous studies suggested that the combination of both, the spin-dependent (SD) and spin-independent (SI) searches are sensitive in complementary regions of parameter space, so considering both searches will allow to explore practically the whole parameter space of the NMSSM. In this letter, the different scenarios are investigated with a new scanning technique, which reveals that significant regions of the NMSSM parameter space cannot be explored, even if one considers both, SI and SD, searches.</description><subject>Dark matter</subject><subject>Direct dark matter searches</subject><subject>NMSSM</subject><subject>Spin dependent dark matter cross section</subject><subject>Spin independent dark matter cross section</subject><subject>Supersymmetry</subject><issn>0370-2693</issn><issn>1873-2445</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><sourceid>DOA</sourceid><recordid>eNqFkNtOAyEQhonRxHp4BbMvsOsAC-zeaYyHxmOiXhNgB6W23QbQpG8vtcZbrwgfM98wPyEnFBoKVJ7OmtX7Os0x24YBVQ3IpuAdMqGd4jVrW7FLJsAV1Ez2fJ8cpDQDACpATsjtE8a0QpfDF6Zq9NUQYrlVA-YNHJcblj5XpWq9WGCOwVWDiR_VwuSMsQrLKr9j9XD__Hx_RPa8mSc8_j0PyevV5cvFTX33eD29OL-rXctkrqlFAQqZNLQVCh0wkH3nAXjfSTFI2zHwSMuD4NwL4RW0Fiy2KAbfQ88PyXTrHUYz06sYFiau9WiC_gFjfNMm5uDmqLkylFnVO8tda4Szwg9UMtsiqI6CKS65dbk4phTR__ko6E28ukz4jVdv4tUgdcGl8WzbiGXTr4BRJxdw6XAbYPlK-E_xDQkAhws</recordid><startdate>20170810</startdate><enddate>20170810</enddate><creator>Beskidt, C.</creator><creator>de Boer, W.</creator><creator>Kazakov, D.I.</creator><creator>Wayand, S.</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>6I.</scope><scope>AAFTH</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>DOA</scope></search><sort><creationdate>20170810</creationdate><title>Perspectives of direct detection of supersymmetric dark matter in the NMSSM</title><author>Beskidt, C. ; de Boer, W. ; Kazakov, D.I. ; Wayand, S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c426t-1be507e26a1457ec020698f0039865d6b820fe1ec0533f55f704b0be4e5df9093</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Dark matter</topic><topic>Direct dark matter searches</topic><topic>NMSSM</topic><topic>Spin dependent dark matter cross section</topic><topic>Spin independent dark matter cross section</topic><topic>Supersymmetry</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Beskidt, C.</creatorcontrib><creatorcontrib>de Boer, W.</creatorcontrib><creatorcontrib>Kazakov, D.I.</creatorcontrib><creatorcontrib>Wayand, S.</creatorcontrib><collection>ScienceDirect Open Access Titles</collection><collection>Elsevier:ScienceDirect:Open Access</collection><collection>CrossRef</collection><collection>Directory of Open Access Journals</collection><jtitle>Physics letters. B</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Beskidt, C.</au><au>de Boer, W.</au><au>Kazakov, D.I.</au><au>Wayand, S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Perspectives of direct detection of supersymmetric dark matter in the NMSSM</atitle><jtitle>Physics letters. B</jtitle><date>2017-08-10</date><risdate>2017</risdate><volume>771</volume><spage>611</spage><epage>618</epage><pages>611-618</pages><issn>0370-2693</issn><eissn>1873-2445</eissn><abstract>In the Next-to-Minimal-Supersymmetric-Standard-Model (NMSSM) the lightest supersymmetric particle (LSP) is a candidate for the dark matter (DM) in the universe. It is a mixture from the various gauginos and Higgsinos and can be bino-, Higgsino- or singlino-dominated. Singlino-dominated LSPs can have very low cross sections below the neutrino background from coherent neutrino scattering which is limiting the sensitivity of future direct DM search experiments. However, previous studies suggested that the combination of both, the spin-dependent (SD) and spin-independent (SI) searches are sensitive in complementary regions of parameter space, so considering both searches will allow to explore practically the whole parameter space of the NMSSM. In this letter, the different scenarios are investigated with a new scanning technique, which reveals that significant regions of the NMSSM parameter space cannot be explored, even if one considers both, SI and SD, searches.</abstract><pub>Elsevier B.V</pub><doi>10.1016/j.physletb.2017.06.016</doi><tpages>8</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0370-2693
ispartof Physics letters. B, 2017-08, Vol.771, p.611-618
issn 0370-2693
1873-2445
language eng
recordid cdi_doaj_primary_oai_doaj_org_article_37a12b79cb3c4a5cb5fd162b4e07810a
source Elsevier; Elsevier ScienceDirect Journals
subjects Dark matter
Direct dark matter searches
NMSSM
Spin dependent dark matter cross section
Spin independent dark matter cross section
Supersymmetry
title Perspectives of direct detection of supersymmetric dark matter in the NMSSM
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-07T13%3A27%3A38IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-elsevier_doaj_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Perspectives%20of%20direct%20detection%20of%20supersymmetric%20dark%20matter%20in%20the%20NMSSM&rft.jtitle=Physics%20letters.%20B&rft.au=Beskidt,%20C.&rft.date=2017-08-10&rft.volume=771&rft.spage=611&rft.epage=618&rft.pages=611-618&rft.issn=0370-2693&rft.eissn=1873-2445&rft_id=info:doi/10.1016/j.physletb.2017.06.016&rft_dat=%3Celsevier_doaj_%3ES0370269317304835%3C/elsevier_doaj_%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c426t-1be507e26a1457ec020698f0039865d6b820fe1ec0533f55f704b0be4e5df9093%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true