scholarly journals First demonstration of a sub-keV electron recoil energy threshold in a liquid argon ionization chamber

Author(s):  
S. Sangiorgio ◽  
T.H. Joshi ◽  
A. Bernstein ◽  
J. Coleman ◽  
M. Foxe ◽  
...  
2013 ◽  
Author(s):  
S Sangiorgio ◽  
A Bernstein ◽  
J Colomean ◽  
M Foxe ◽  
C Hagmann ◽  
...  

2021 ◽  
Vol 2021 (1) ◽  
Author(s):  
Hyun Min Lee

Abstract Motivated by the recent excess in the electron recoil from XENON1T experiment, we consider the possibility of exothermic dark matter, which is composed of two states with mass splitting. The heavier state down-scatters off the electron into the lighter state, making an appropriate recoil energy required for the Xenon excess even for the standard Maxwellian velocity distribution of dark matter. Accordingly, we determine the mass difference between two component states of dark matter to the peak electron recoil energy at about 2.5 keV up to the detector resolution, accounting for the recoil events over ER = 2 − 3 keV, which are most significant. We include the effects of the phase-space enhancement and the atomic excitation factor to calculate the required scattering cross section for the Xenon excess. We discuss the implications of dark matter interactions in the effective theory for exothermic dark matter and a massive Z′ mediator and provide microscopic models realizing the required dark matter and electron couplings to Z′.


1994 ◽  
Vol 35 ◽  
pp. 384-385 ◽  
Author(s):  
A.S. Barabash ◽  
G. Carugno ◽  
S.I. Konovalov ◽  
P.A. Polozov ◽  
R.R. Saakyan ◽  
...  

1999 ◽  
Vol 38 (Part 1, No. 11) ◽  
pp. 6491-6497 ◽  
Author(s):  
Akira Yunoki ◽  
Tadayoshi Doke ◽  
Masayuki Kase ◽  
Toshisuke Kashiwagi ◽  
Toshiyuki Kato ◽  
...  

1976 ◽  
Vol 135 (1) ◽  
pp. 151-156 ◽  
Author(s):  
W. Hofmann ◽  
U. Klein ◽  
M. Schulz ◽  
J. Spengler ◽  
D. Wegener

1979 ◽  
Vol 166 (2) ◽  
pp. 169-170 ◽  
Author(s):  
A.S. Barabash ◽  
A.A. Golubev ◽  
O.V. Kazachenko ◽  
B.M. Ovchinnikov

1999 ◽  
Vol 70 (1-3) ◽  
pp. 233-235 ◽  
Author(s):  
V.D. Ashitkov ◽  
A.S. Barabash ◽  
S.G. Belogurov ◽  
G. Carugno ◽  
S.I. Konovalov ◽  
...  

2020 ◽  
Vol 2020 (12) ◽  
Author(s):  
Masahiro Ibe ◽  
Shin Kobayashi ◽  
Yuhei Nakayama ◽  
Satoshi Shirai

Abstract Recently, the XENON1T collaboration reported an excess in the electron recoil energy spectrum. One of the simplest new physics interpretation is a new neutrino-electron interaction mediated by a light vector particle. However, for the parameter region favored by this excess, the constraints from the stellar cooling are severe. Still, there are astrophysical uncertainties on those constraints. In this paper, we discuss the constraint on the light mediator from the effective number of neutrino Neff in the CMB era, which provides an independent constraint. We show that Neff is significantly enhanced and exceeds the current constraint in the parameter region favored for the XENON1T excess. As a result, the interpretation by a light mediator heavier than about 1 eV is excluded by the Neff constraint.


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