Sub-GeV dark matter and MeV gamma-ray detection with COSI

Abstract Sub-GeV dark matter (DM) has been attracting more attention due to the negative results searching for traditional weakly interacting massive particles (WIMPs). Such particles are expected to produce gamma rays from annihilation in the MeV energy region. Advancements in technology have opene...

وصف كامل

التفاصيل البيبلوغرافية
الحاوية / القاعدة:Journal of High Energy Physics
المؤلفون الرئيسيون: Yu Watanabe, Shigeki Matsumoto, Christopher M Karwin, Tom Melia, Michela Negro, Thomas Siegert, Yuki Watanabe, Hiroki Yoneda, Tadayuki Takahashi
التنسيق: مقال
اللغة:الإنجليزية
منشور في: SpringerOpen 2025-09-01
الموضوعات:
Models for Dark Matter
Particle Nature of Dark Matter
Cosmic Rays
New Light Particles
الوصول للمادة أونلاين:https://doi.org/10.1007/JHEP09(2025)078

الانترنت

https://doi.org/10.1007/JHEP09(2025)078

مواد مشابهة