Collider detection of dark matter electromagnetic anapole moments
Autor(a) principal: | |
---|---|
Data de Publicação: | 2018 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNIFESP |
Texto Completo: | https://repositorio.unifesp.br/handle/11600/55815 http://dx.doi.org/10.1103/PhysRevD.97.055023 |
Resumo: | Dark matter that interacts with the Standard Model by exchanging photons through higher multipole interactions occurs in a wide range of both strongly and weakly coupled hidden sector models. We study the collider detection prospects of these candidates, with a focus on Majorana dark matter that couples through the anapole moment. The study is conducted at the effective field theory level with the mono-Z signature incorporating varying levels of systematic uncertainties at the high-luminosity LHC. The projected collider reach on the anapole moment is then compared to the reach coming from direct detection experiments like LZ. Finally, the analysis is applied to a weakly coupled completion with leptophilic dark matter. |
id |
UFSP_d25614523c14e2ddb7a01788f29b4b06 |
---|---|
oai_identifier_str |
oai:repositorio.unifesp.br:11600/55815 |
network_acronym_str |
UFSP |
network_name_str |
Repositório Institucional da UNIFESP |
repository_id_str |
3465 |
spelling |
Alves, Alexandre [UNIFESP]Santos, A. C. O.Sinha, Kuver2020-07-20T16:31:15Z2020-07-20T16:31:15Z2018Physical Review D. College Pk, v. 97, n. 5, 2018.2470-0010https://repositorio.unifesp.br/handle/11600/55815http://dx.doi.org/10.1103/PhysRevD.97.055023WOS000427603400011.pdf10.1103/PhysRevD.97.055023WOS:000427603400011Dark matter that interacts with the Standard Model by exchanging photons through higher multipole interactions occurs in a wide range of both strongly and weakly coupled hidden sector models. We study the collider detection prospects of these candidates, with a focus on Majorana dark matter that couples through the anapole moment. The study is conducted at the effective field theory level with the mono-Z signature incorporating varying levels of systematic uncertainties at the high-luminosity LHC. The projected collider reach on the anapole moment is then compared to the reach coming from direct detection experiments like LZ. Finally, the analysis is applied to a weakly coupled completion with leptophilic dark matter.CNPqFundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP)Coordenacao de Aperfeicoamento de Pessoal de Nivel SuperiorUniv Fed Sao Paulo, Dept Fis, BR-09972270 Diadema, SP, BrazilUniv Fed Paraiba, Dept Fis, BR-58051970 Joao Pessoa, PB, BrazilUniv Catholic Louvain, Ctr Cosmol Particle Phys & Phenomenol CP3, B-1348 Louvain La Neuve, BelgiumUniv Oklahoma, Dept Phys & Astron, Norman, OK 73019 USAUniv Fed Sao Paulo, Dept Fis, BR-09972270 Diadema, SP, BrazilCNPq: 307098/2014-1FAPESP: 2013/22079-8CAPES: Capes-PDSE-88881.135139/2016-01Web of Science-engAmer Physical SocPhysical Review DCollider detection of dark matter electromagnetic anapole momentsinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleCollege Pkv. 975info:eu-repo/semantics/openAccessreponame:Repositório Institucional da UNIFESPinstname:Universidade Federal de São Paulo (UNIFESP)instacron:UNIFESPORIGINALWOS000427603400011.pdfapplication/pdf1202523${dspace.ui.url}/bitstream/11600/55815/1/WOS000427603400011.pdf148e1b323a34690f4dcc1c3b2e4c558bMD51open accessTEXTWOS000427603400011.pdf.txtWOS000427603400011.pdf.txtExtracted texttext/plain66270${dspace.ui.url}/bitstream/11600/55815/8/WOS000427603400011.pdf.txt85027019327fa8ffb3dc962cb4fa83adMD58open accessTHUMBNAILWOS000427603400011.pdf.jpgWOS000427603400011.pdf.jpgIM Thumbnailimage/jpeg6851${dspace.ui.url}/bitstream/11600/55815/10/WOS000427603400011.pdf.jpg8ac95e50511b282e9a1d947f9281f788MD510open access11600/558152023-06-05 19:22:51.146open accessoai:repositorio.unifesp.br:11600/55815Repositório InstitucionalPUBhttp://www.repositorio.unifesp.br/oai/requestopendoar:34652023-06-05T22:22:51Repositório Institucional da UNIFESP - Universidade Federal de São Paulo (UNIFESP)false |
dc.title.en.fl_str_mv |
Collider detection of dark matter electromagnetic anapole moments |
title |
Collider detection of dark matter electromagnetic anapole moments |
spellingShingle |
Collider detection of dark matter electromagnetic anapole moments Alves, Alexandre [UNIFESP] |
title_short |
Collider detection of dark matter electromagnetic anapole moments |
title_full |
Collider detection of dark matter electromagnetic anapole moments |
title_fullStr |
Collider detection of dark matter electromagnetic anapole moments |
title_full_unstemmed |
Collider detection of dark matter electromagnetic anapole moments |
title_sort |
Collider detection of dark matter electromagnetic anapole moments |
author |
Alves, Alexandre [UNIFESP] |
author_facet |
Alves, Alexandre [UNIFESP] Santos, A. C. O. Sinha, Kuver |
author_role |
author |
author2 |
Santos, A. C. O. Sinha, Kuver |
author2_role |
author author |
dc.contributor.author.fl_str_mv |
Alves, Alexandre [UNIFESP] Santos, A. C. O. Sinha, Kuver |
description |
Dark matter that interacts with the Standard Model by exchanging photons through higher multipole interactions occurs in a wide range of both strongly and weakly coupled hidden sector models. We study the collider detection prospects of these candidates, with a focus on Majorana dark matter that couples through the anapole moment. The study is conducted at the effective field theory level with the mono-Z signature incorporating varying levels of systematic uncertainties at the high-luminosity LHC. The projected collider reach on the anapole moment is then compared to the reach coming from direct detection experiments like LZ. Finally, the analysis is applied to a weakly coupled completion with leptophilic dark matter. |
publishDate |
2018 |
dc.date.issued.fl_str_mv |
2018 |
dc.date.accessioned.fl_str_mv |
2020-07-20T16:31:15Z |
dc.date.available.fl_str_mv |
2020-07-20T16:31:15Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.citation.fl_str_mv |
Physical Review D. College Pk, v. 97, n. 5, 2018. |
dc.identifier.uri.fl_str_mv |
https://repositorio.unifesp.br/handle/11600/55815 http://dx.doi.org/10.1103/PhysRevD.97.055023 |
dc.identifier.issn.none.fl_str_mv |
2470-0010 |
dc.identifier.file.none.fl_str_mv |
WOS000427603400011.pdf |
dc.identifier.doi.none.fl_str_mv |
10.1103/PhysRevD.97.055023 |
dc.identifier.wos.none.fl_str_mv |
WOS:000427603400011 |
identifier_str_mv |
Physical Review D. College Pk, v. 97, n. 5, 2018. 2470-0010 WOS000427603400011.pdf 10.1103/PhysRevD.97.055023 WOS:000427603400011 |
url |
https://repositorio.unifesp.br/handle/11600/55815 http://dx.doi.org/10.1103/PhysRevD.97.055023 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.none.fl_str_mv |
Physical Review D |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
- |
dc.coverage.none.fl_str_mv |
College Pk |
dc.publisher.none.fl_str_mv |
Amer Physical Soc |
publisher.none.fl_str_mv |
Amer Physical Soc |
dc.source.none.fl_str_mv |
reponame:Repositório Institucional da UNIFESP instname:Universidade Federal de São Paulo (UNIFESP) instacron:UNIFESP |
instname_str |
Universidade Federal de São Paulo (UNIFESP) |
instacron_str |
UNIFESP |
institution |
UNIFESP |
reponame_str |
Repositório Institucional da UNIFESP |
collection |
Repositório Institucional da UNIFESP |
bitstream.url.fl_str_mv |
${dspace.ui.url}/bitstream/11600/55815/1/WOS000427603400011.pdf ${dspace.ui.url}/bitstream/11600/55815/8/WOS000427603400011.pdf.txt ${dspace.ui.url}/bitstream/11600/55815/10/WOS000427603400011.pdf.jpg |
bitstream.checksum.fl_str_mv |
148e1b323a34690f4dcc1c3b2e4c558b 85027019327fa8ffb3dc962cb4fa83ad 8ac95e50511b282e9a1d947f9281f788 |
bitstream.checksumAlgorithm.fl_str_mv |
MD5 MD5 MD5 |
repository.name.fl_str_mv |
Repositório Institucional da UNIFESP - Universidade Federal de São Paulo (UNIFESP) |
repository.mail.fl_str_mv |
|
_version_ |
1802764167389642752 |