Dark-photon search using data from CRESST-II Phase 2
Identifying the nature and origin of dark matter is one of the major challenges for modern astro and particle physics. Direct dark-matter searches aim at an observation of dark-matter particles interacting within detectors. The focus of several such searches is on interactions with nuclei as provide...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Format: | Journal article |
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Springer
2017
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author | Angloher, G Bauer, P Bento, A Bucci, C Canonica, L Defay, X Erb, A v. Feilitzsch, F Ferreiro Iachellini, N Gorla, P Gütlein, A Hauff, D Jochum, J Kiefer, M Kluck, H Kraus, H Lanfranchi, J Loebell, J Mancuso, M Münster, A Pagliarone, C Petricca, F Potzel, W Pröbst, F Puig, R Reindl, F Schäffner, K Schieck, J Schönert, S Seidel, W Stodolsky, L Strandhagen, C Strauss, R Tanzke, A Tranh Thi, H Türkoǧlu, C Uffinger, M Ulrich, A Usherov, I Wawoczny, S Willers, M Wüstrich, M Zöller, A |
author_facet | Angloher, G Bauer, P Bento, A Bucci, C Canonica, L Defay, X Erb, A v. Feilitzsch, F Ferreiro Iachellini, N Gorla, P Gütlein, A Hauff, D Jochum, J Kiefer, M Kluck, H Kraus, H Lanfranchi, J Loebell, J Mancuso, M Münster, A Pagliarone, C Petricca, F Potzel, W Pröbst, F Puig, R Reindl, F Schäffner, K Schieck, J Schönert, S Seidel, W Stodolsky, L Strandhagen, C Strauss, R Tanzke, A Tranh Thi, H Türkoǧlu, C Uffinger, M Ulrich, A Usherov, I Wawoczny, S Willers, M Wüstrich, M Zöller, A |
author_sort | Angloher, G |
collection | OXFORD |
description | Identifying the nature and origin of dark matter is one of the major challenges for modern astro and particle physics. Direct dark-matter searches aim at an observation of dark-matter particles interacting within detectors. The focus of several such searches is on interactions with nuclei as provided e.g. byWeakly Interacting Massive Particles. However, there is a variety of dark-matter candidates favoring interactions with electrons rather than with nuclei. One example are dark photons, i.e., long-lived vector particles with a kinetic mixing to standard-model photons. In this work we present constraints on this kinetic mixing based on data from CRESST-II Phase 2 corresponding to an exposure before cuts of 52 kg-days. These constraints improve the existing ones for dark-photon masses between 0.3 and 0.7 keV/c2. |
first_indexed | 2024-03-06T19:23:38Z |
format | Journal article |
id | oxford-uuid:1af7f4ff-b43f-44e7-a0e3-c374c32a1c45 |
institution | University of Oxford |
last_indexed | 2024-03-06T19:23:38Z |
publishDate | 2017 |
publisher | Springer |
record_format | dspace |
spelling | oxford-uuid:1af7f4ff-b43f-44e7-a0e3-c374c32a1c452022-03-26T10:57:46ZDark-photon search using data from CRESST-II Phase 2Journal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:1af7f4ff-b43f-44e7-a0e3-c374c32a1c45Symplectic Elements at OxfordSpringer2017Angloher, GBauer, PBento, ABucci, CCanonica, LDefay, XErb, Av. Feilitzsch, FFerreiro Iachellini, NGorla, PGütlein, AHauff, DJochum, JKiefer, MKluck, HKraus, HLanfranchi, JLoebell, JMancuso, MMünster, APagliarone, CPetricca, FPotzel, WPröbst, FPuig, RReindl, FSchäffner, KSchieck, JSchönert, SSeidel, WStodolsky, LStrandhagen, CStrauss, RTanzke, ATranh Thi, HTürkoǧlu, CUffinger, MUlrich, AUsherov, IWawoczny, SWillers, MWüstrich, MZöller, AIdentifying the nature and origin of dark matter is one of the major challenges for modern astro and particle physics. Direct dark-matter searches aim at an observation of dark-matter particles interacting within detectors. The focus of several such searches is on interactions with nuclei as provided e.g. byWeakly Interacting Massive Particles. However, there is a variety of dark-matter candidates favoring interactions with electrons rather than with nuclei. One example are dark photons, i.e., long-lived vector particles with a kinetic mixing to standard-model photons. In this work we present constraints on this kinetic mixing based on data from CRESST-II Phase 2 corresponding to an exposure before cuts of 52 kg-days. These constraints improve the existing ones for dark-photon masses between 0.3 and 0.7 keV/c2. |
spellingShingle | Angloher, G Bauer, P Bento, A Bucci, C Canonica, L Defay, X Erb, A v. Feilitzsch, F Ferreiro Iachellini, N Gorla, P Gütlein, A Hauff, D Jochum, J Kiefer, M Kluck, H Kraus, H Lanfranchi, J Loebell, J Mancuso, M Münster, A Pagliarone, C Petricca, F Potzel, W Pröbst, F Puig, R Reindl, F Schäffner, K Schieck, J Schönert, S Seidel, W Stodolsky, L Strandhagen, C Strauss, R Tanzke, A Tranh Thi, H Türkoǧlu, C Uffinger, M Ulrich, A Usherov, I Wawoczny, S Willers, M Wüstrich, M Zöller, A Dark-photon search using data from CRESST-II Phase 2 |
title | Dark-photon search using data from CRESST-II Phase 2 |
title_full | Dark-photon search using data from CRESST-II Phase 2 |
title_fullStr | Dark-photon search using data from CRESST-II Phase 2 |
title_full_unstemmed | Dark-photon search using data from CRESST-II Phase 2 |
title_short | Dark-photon search using data from CRESST-II Phase 2 |
title_sort | dark photon search using data from cresst ii phase 2 |
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