Erratum: Directly Detecting MeV-Scale Dark Matter via Solar Reflection (Physical Review Letters (2018) 120 (141801) DOI: 10.1103/PhysRevLett.120.141801)

Haipeng An; Maxim Pospelov; Josef Pradler; Adam Ritz

doi:10.1103/PhysRevLett.121.259903

Erratum: Directly Detecting MeV-Scale Dark Matter via Solar Reflection (Physical Review Letters (2018) 120 (141801) DOI: 10.1103/PhysRevLett.120.141801)

Haipeng An
, Maxim Pospelov
, Josef Pradler
, Adam Ritz

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Comment/debate › peer-review

47 Scopus citations

Abstract

In this Letter, we pointed out that additional direct detection sensitivity to dark matter (DM) in the 10 keV10 MeV mass range is possible through consideration of reflected DM initially scattered by more energetic electrons in the Sun (or Earth) prior to scattering in the terrestrial underground detector. (Figure Presented).

Original language	English (US)
Article number	259903
Journal	Physical review letters
Volume	121
Issue number	25
DOIs	https://doi.org/10.1103/PhysRevLett.121.259903
State	Published - Dec 18 2018

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© 2018 American Physical Society.

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10.1103/PhysRevLett.121.259903

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abstract = "In this Letter, we pointed out that additional direct detection sensitivity to dark matter (DM) in the 10 keV10 MeV mass range is possible through consideration of reflected DM initially scattered by more energetic electrons in the Sun (or Earth) prior to scattering in the terrestrial underground detector. (Figure Presented).",

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AU - Ritz, Adam

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Erratum: Directly Detecting MeV-Scale Dark Matter via Solar Reflection (Physical Review Letters (2018) 120 (141801) DOI: 10.1103/PhysRevLett.120.141801)

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