2018
DOI: 10.1103/physrevlett.121.041802
|View full text |Cite
|
Sign up to set email alerts
|

Novel Way to Search for Light Dark Matter in Lepton Beam-Dump Experiments

Abstract: A novel mechanism to produce and detect light dark matter in experiments making use of GeV electrons (and positrons) impinging on a thick target (beam dump) is proposed. The positron-rich environment produced by the electromagnetic shower allows us to produce an A^{'} via nonresonant (e^{+}+e^{-}→γ+A^{'}) and resonant (e^{+}+e^{-}→A^{'}) annihilation on atomic electrons. The latter mechanism, for some selected kinematics, results in a larger sensitivity with respect to limits derived by the commonly used A^{'}… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

0
62
0

Year Published

2019
2019
2024
2024

Publication Types

Select...
8
1
1

Relationship

1
9

Authors

Journals

citations
Cited by 65 publications
(62 citation statements)
references
References 29 publications
(31 reference statements)
0
62
0
Order By: Relevance
“…The NA64 Collaboration has recently published very strong limits for DP masses below 150 MeV [45] via a missing energy analysis. For large α D , experiments looking at electron-DM scattering such as LSND [46,47], MiniBooNE [20,21], E137 [48][49][50], and NOνA [25] and capable of competing with NA64 for dark matter masses below few tens of MeV. (ii) Direct detection: In the region where the χ relic abundance corresponds to the observed DM abundance and for large values of α D , CRESST-II and III place strong constraints on m χ > 500 MeV [51][52][53][54].…”
Section: Vector Portalmentioning
confidence: 99%
“…The NA64 Collaboration has recently published very strong limits for DP masses below 150 MeV [45] via a missing energy analysis. For large α D , experiments looking at electron-DM scattering such as LSND [46,47], MiniBooNE [20,21], E137 [48][49][50], and NOνA [25] and capable of competing with NA64 for dark matter masses below few tens of MeV. (ii) Direct detection: In the region where the χ relic abundance corresponds to the observed DM abundance and for large values of α D , CRESST-II and III place strong constraints on m χ > 500 MeV [51][52][53][54].…”
Section: Vector Portalmentioning
confidence: 99%
“…The mass splitting between Dirac fermion component states δ and DM mass M χ are indicated. Constraints on dark photons are shown [60][61][62][63][64][65] (gray) alongside CRESST DM-nucleon scattering bounds [58] (blue), and SuperCDMS Ge/Si projections [66] (dotted).…”
mentioning
confidence: 99%
“…Such a beam intensity will allow BDX to collect ∼10 22 electron-on-target (EOT) in 285 days, in full parasitic runs. The interaction between the energetic electrons and the atoms of the dump leads to the production of Dark Photons through a Bremsstrahlung-like radiative process (A − strahlung, Figure 1, left) [10] and e + e − annihilations [13,14]. The A could then decay into forward-boosted DM particles (χ) (Figure 1, left).…”
Section: Bdx Overviewmentioning
confidence: 99%