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Search for Light Dark Matter with NA64 at CERN
by
Gertsenberger, S V
, Salamatin, K M
, Kravchuk, L V
, Sieber, H
, Cooke, D
, Girod, S
, Mena Yanssen, R G
, Gardikiotis, A
, Kolosov, V N
, V Yu Volkov
, Tlisova, I V
, Voronchikhin, I V
, Zamora-Saa, J
, Lysan, V
, Lyubovitskij, V E
, Soto, O
, Volkov, P V
, Karneyeu, A E
, Dermenev, A V
, Kasianova, E A
, Ketzer, B
, Toropin, A N
, Charitonidis, N
, M H"osgen
, Frolov, V N
, Peshekhonov, D V
, L Molina Bueno
, Bisio, P
, Galleguillos Silva, R B
, Zhevlakov, A S
, Kambar, Y
, Polyakov, V A
, A Yu Trifonov
, Radics, B
, Banerjee, D
, Depero, E
, Matveev, V A
, Crivelli, P
, Tuzi, M
, Kirpichnikov, D V
, Mongillo, M
, R Mena Fredes
, Donskov, S V
, Gninenko, S N
, Kuleshov, S V
, Kachanov, V A
, Kramarenko, V A
, Bernhard, J
, Celentano, A
, Andreev, Yu M
, Samoylenko, V D
, Tikhomirov, V O
, Oberhauser, B Banto
, Dusaev, R R
, Shchukin, D
, Enik, T
, Kekelidze, G D
, Chumakov, A G
, Marsicano, L
, Vasilishin, B I
, Krasnikov, N V
, Kirsanov, M M
, Marini, A
in
CERN
/ Couplings
/ Dark matter
/ Electrons
/ Electroweak model
/ Photons
/ Synchrotrons
2023
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Search for Light Dark Matter with NA64 at CERN
by
Gertsenberger, S V
, Salamatin, K M
, Kravchuk, L V
, Sieber, H
, Cooke, D
, Girod, S
, Mena Yanssen, R G
, Gardikiotis, A
, Kolosov, V N
, V Yu Volkov
, Tlisova, I V
, Voronchikhin, I V
, Zamora-Saa, J
, Lysan, V
, Lyubovitskij, V E
, Soto, O
, Volkov, P V
, Karneyeu, A E
, Dermenev, A V
, Kasianova, E A
, Ketzer, B
, Toropin, A N
, Charitonidis, N
, M H"osgen
, Frolov, V N
, Peshekhonov, D V
, L Molina Bueno
, Bisio, P
, Galleguillos Silva, R B
, Zhevlakov, A S
, Kambar, Y
, Polyakov, V A
, A Yu Trifonov
, Radics, B
, Banerjee, D
, Depero, E
, Matveev, V A
, Crivelli, P
, Tuzi, M
, Kirpichnikov, D V
, Mongillo, M
, R Mena Fredes
, Donskov, S V
, Gninenko, S N
, Kuleshov, S V
, Kachanov, V A
, Kramarenko, V A
, Bernhard, J
, Celentano, A
, Andreev, Yu M
, Samoylenko, V D
, Tikhomirov, V O
, Oberhauser, B Banto
, Dusaev, R R
, Shchukin, D
, Enik, T
, Kekelidze, G D
, Chumakov, A G
, Marsicano, L
, Vasilishin, B I
, Krasnikov, N V
, Kirsanov, M M
, Marini, A
in
CERN
/ Couplings
/ Dark matter
/ Electrons
/ Electroweak model
/ Photons
/ Synchrotrons
2023
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Do you wish to request the book?
Search for Light Dark Matter with NA64 at CERN
by
Gertsenberger, S V
, Salamatin, K M
, Kravchuk, L V
, Sieber, H
, Cooke, D
, Girod, S
, Mena Yanssen, R G
, Gardikiotis, A
, Kolosov, V N
, V Yu Volkov
, Tlisova, I V
, Voronchikhin, I V
, Zamora-Saa, J
, Lysan, V
, Lyubovitskij, V E
, Soto, O
, Volkov, P V
, Karneyeu, A E
, Dermenev, A V
, Kasianova, E A
, Ketzer, B
, Toropin, A N
, Charitonidis, N
, M H"osgen
, Frolov, V N
, Peshekhonov, D V
, L Molina Bueno
, Bisio, P
, Galleguillos Silva, R B
, Zhevlakov, A S
, Kambar, Y
, Polyakov, V A
, A Yu Trifonov
, Radics, B
, Banerjee, D
, Depero, E
, Matveev, V A
, Crivelli, P
, Tuzi, M
, Kirpichnikov, D V
, Mongillo, M
, R Mena Fredes
, Donskov, S V
, Gninenko, S N
, Kuleshov, S V
, Kachanov, V A
, Kramarenko, V A
, Bernhard, J
, Celentano, A
, Andreev, Yu M
, Samoylenko, V D
, Tikhomirov, V O
, Oberhauser, B Banto
, Dusaev, R R
, Shchukin, D
, Enik, T
, Kekelidze, G D
, Chumakov, A G
, Marsicano, L
, Vasilishin, B I
, Krasnikov, N V
, Kirsanov, M M
, Marini, A
in
CERN
/ Couplings
/ Dark matter
/ Electrons
/ Electroweak model
/ Photons
/ Synchrotrons
2023
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Paper
Search for Light Dark Matter with NA64 at CERN
2023
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Overview
Thermal dark matter models with particle \\(\\) masses below the electroweak scale can provide an explanation for the observed relic dark matter density. This would imply the existence of a new feeble interaction between the dark and ordinary matter. We report on a new search for the sub-GeV \\(\\) production through the interaction mediated by a new vector boson, called the dark photon \\(A'\\), in collisions of 100 GeV electrons with the active target of the NA64 experiment at the CERN SPS. With \\(9.3710^11\\) electrons on target collected during 2016-2022 runs NA64 probes for the first time the well-motivated region of parameter space of benchmark thermal scalar and fermionic dark matter models. No evidence for dark matter production has been found. This allows us to set the most sensitive limits on the \\(A'\\) couplings to photons for masses \\(m_A' 0.35\\) GeV, and to exclude scalar and Majorana dark matter with the \\(-A'\\) coupling \\(_D 0.1\\) for masses \\(0.001 m_ 0.1\\) GeV and \\(3m_ m_A'\\).
Publisher
Cornell University Library, arXiv.org
Subject
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