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Dark-photon search using data from CRESST-II Phase 2

Authors :
Angloher, G
Bauer, P
Bento, A
Bucci, C
Canonica, L
Defay, X
Erb, A
von Feilitzsch, F
Iachellini, N
Gorla, P
Gutlein, A
Hauff, D
Jochum, J
Kiefer, M
Kluck, H
Kraus, H
Lanfranchi, J
Loebell, J
Mancuso, M
Munster, A
Pagliarone, C
Petricca, F
Potzel, W
Probst, F
Puig, R
Reindl, F
Schaffner, K
Schieck, J
Schonert, S
Seidel, W
Stodolsky, L
Strandhagen, C
Strauss, R
Tanzke, A
Thi, H
Turkoglu, C
Uffinger, M
Ulrich, A
Usherov, I
Wawoczny, S
Willers, M
Wustrich, M
Zoller, A
Angloher G
Bauer P
Bento A
Bucci C
Canonica L
Defay X
Erb A
von Feilitzsch F
Iachellini NF
Gorla P
Gutlein A
Hauff D
Jochum J
Kiefer M
Kluck H
Kraus H
Lanfranchi JC
Loebell J
Mancuso M
Munster A
Pagliarone C
Petricca F
Potzel W
Probst F
Puig R
Reindl F
Schaffner K
Schieck J
Schonert S
Seidel W
Stodolsky L
Strandhagen C
Strauss R
Tanzke A
Thi HHT
Turkoglu C
Uffinger M
Ulrich A
Usherov I
Wawoczny S
Willers M
Wustrich M
Zoller A
Angloher, G
Bauer, P
Bento, A
Bucci, C
Canonica, L
Defay, X
Erb, A
von Feilitzsch, F
Iachellini, N
Gorla, P
Gutlein, A
Hauff, D
Jochum, J
Kiefer, M
Kluck, H
Kraus, H
Lanfranchi, J
Loebell, J
Mancuso, M
Munster, A
Pagliarone, C
Petricca, F
Potzel, W
Probst, F
Puig, R
Reindl, F
Schaffner, K
Schieck, J
Schonert, S
Seidel, W
Stodolsky, L
Strandhagen, C
Strauss, R
Tanzke, A
Thi, H
Turkoglu, C
Uffinger, M
Ulrich, A
Usherov, I
Wawoczny, S
Willers, M
Wustrich, M
Zoller, A
Angloher G
Bauer P
Bento A
Bucci C
Canonica L
Defay X
Erb A
von Feilitzsch F
Iachellini NF
Gorla P
Gutlein A
Hauff D
Jochum J
Kiefer M
Kluck H
Kraus H
Lanfranchi JC
Loebell J
Mancuso M
Munster A
Pagliarone C
Petricca F
Potzel W
Probst F
Puig R
Reindl F
Schaffner K
Schieck J
Schonert S
Seidel W
Stodolsky L
Strandhagen C
Strauss R
Tanzke A
Thi HHT
Turkoglu C
Uffinger M
Ulrich A
Usherov I
Wawoczny S
Willers M
Wustrich M
Zoller A
Publication Year :
2017

Abstract

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. by weakly 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.

Details

Database :
OAIster
Notes :
STAMPA, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1434548712
Document Type :
Electronic Resource