Primordial black holes and scotogenic dark matter

نویسندگان

چکیده

We study the effect of scotogenic dark matter on primordial black holes (PBHs) and vice versa. show that if PBHs evaporate in radiation dominant era, upper limit initial mass $M_{\rm in}$ should be constrained as $10^4 \lesssim M_{\rm in}/M_{\rm Pl} 10^{10}$ for $\mathcal{O}$(1) TeV ($\mathcal{O}$(1) is most appropriate energy scale model). On other hand, PBH dominated a quite heavy ($m_{/rm DM} /gtrsim 10^9$ GeV) $M_{/rm in}/M_{/rm /sim 10^{13}$ may allowed.

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ژورنال

عنوان ژورنال: International Journal of Modern Physics A

سال: 2021

ISSN: ['0217-751X', '1793-656X']

DOI: https://doi.org/10.1142/s0217751x21501396