The lightest $Z_2$ odd particle in the scotogenic model, referred to as scotogenic dark matter (DM), is a widely studied candidate for DM. This scotogenic DM is generated through well-known thermal processes as well as via the evaporation of primordial black holes (PBHs). Recent reports suggested that the curvature fluctuations of PBHs during an epoch dominated by these entities in the early universe can serve as the source of so-called induced gravitational waves (GWs). In this study, we demonstrate that stringent constraints on the mass of scotogenic DM and PBHs can be obtained through the detection of induced GWs using future detectors.Comment: 8 pages, 4 figure
We investigate the impact of radiation from primordial black holes (PBHs), in the mass range of $10^...
Scalar perturbations in the early Universe create over-dense regions that can collapse into primordi...
With several dozen binary black hole events detected by LIGO/Virgo to date and many more expected in...
Dark Matter (DM) is omnipresent in our universe. Despite its abundance, the microscopic identity of ...
Primordial Black Holes (PBH) could dominate in the early universe and, evaporating before Big bang N...
Hawking evaporation of primordial black holes (PBHs) can facilitate the generation of matter-antimat...
We study the effect of an ultra-light primordial black hole (PBH) dominated phase on the gravitation...
The gravitational potential of initially Poisson distributed primordial black holes (PBH) can induce...
Because primordial black holes (PBHs) evaporate into all particle species in nature, PBHs may emit s...
Future ground-based gravitational wave observatories will be ideal probes of the environments surrou...
We study formation of primordial black holes and generation of gravitational waves in a class of cos...
To trace the particle nature of dark matter (DM) from cosmic microwave background observations, we s...
Axion-like particles (ALPs), a compelling candidate for dark matter (DM), are the pseudo Nambu-Golds...
We show that gravitational waves have the potential to unravel the microphysical properties of dark ...
Light primordial black holes (PBHs) with masses smaller than $10^9$ g ($10^{-24} M_\odot$) evaporate...
We investigate the impact of radiation from primordial black holes (PBHs), in the mass range of $10^...
Scalar perturbations in the early Universe create over-dense regions that can collapse into primordi...
With several dozen binary black hole events detected by LIGO/Virgo to date and many more expected in...
Dark Matter (DM) is omnipresent in our universe. Despite its abundance, the microscopic identity of ...
Primordial Black Holes (PBH) could dominate in the early universe and, evaporating before Big bang N...
Hawking evaporation of primordial black holes (PBHs) can facilitate the generation of matter-antimat...
We study the effect of an ultra-light primordial black hole (PBH) dominated phase on the gravitation...
The gravitational potential of initially Poisson distributed primordial black holes (PBH) can induce...
Because primordial black holes (PBHs) evaporate into all particle species in nature, PBHs may emit s...
Future ground-based gravitational wave observatories will be ideal probes of the environments surrou...
We study formation of primordial black holes and generation of gravitational waves in a class of cos...
To trace the particle nature of dark matter (DM) from cosmic microwave background observations, we s...
Axion-like particles (ALPs), a compelling candidate for dark matter (DM), are the pseudo Nambu-Golds...
We show that gravitational waves have the potential to unravel the microphysical properties of dark ...
Light primordial black holes (PBHs) with masses smaller than $10^9$ g ($10^{-24} M_\odot$) evaporate...
We investigate the impact of radiation from primordial black holes (PBHs), in the mass range of $10^...
Scalar perturbations in the early Universe create over-dense regions that can collapse into primordi...
With several dozen binary black hole events detected by LIGO/Virgo to date and many more expected in...