Probing dark matter particles from evaporating primordial black holes via electron scattering in the CDEX-10 experiment
Dark matter (DM) is a major constituent of the Universe. However, no definite evidence of DM particles (denoted as “ χ ”) has been found in DM direct detection (DD) experiments to date. There is a novel concept of detecting χ from evaporating primordial black holes (PBHs). We search for χ emitted fr...
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Published in | Science China. Physics, mechanics & astronomy Vol. 67; no. 10; p. 101011 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Beijing
Science China Press
01.10.2024
Springer Nature B.V |
Subjects | |
Online Access | Get full text |
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Summary: | Dark matter (DM) is a major constituent of the Universe. However, no definite evidence of DM particles (denoted as “
χ
”) has been found in DM direct detection (DD) experiments to date. There is a novel concept of detecting
χ
from evaporating primordial black holes (PBHs). We search for
χ
emitted from PBHs by investigating their interaction with target electrons. The examined PBH masses range from 1 × 10
15
to 7
×
10
16
g under the current limits of PBH abundance
f
PBH
. Using 205.4 kg·day data obtained from the CDEX-10 experiment conducted in the China Jinping Underground Laboratory, we exclude the
χ
-electron (
χ
-
e
) elastic-scattering cross section
σ
χ
e
∼ 5 × 10
−29
cm
2
for
χ
with a mass
m
χ
≲ 0.1 keV from our results. With the higher radiation background but lower energy threshold (160 eV), CDEX-10 fills a part of the gap in the previous work. If (
m
χ
,
σ
χ
e
) can be determined in the future, DD experiments are expected to impose strong constraints on
f
PBH
for large
M
PBH
s. |
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ISSN: | 1674-7348 1869-1927 |
DOI: | 10.1007/s11433-024-2446-2 |