Pages that link to "Item:Q5026110"
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The following pages link to Reconstruction of primordial power spectrum of curvature perturbation from the merger rate of primordial black hole binaries (Q5026110):
Displaying 10 items.
- Feasibility of primordial black hole Remnants as dark matter in view of Hawking radiation recoil (Q5029554) (← links)
- Primordial black holes in peak theory with a non-Gaussian tail (Q5061935) (← links)
- Primordial black holes ensued from exponential potential and coupling parameter in nonminimal derivative inflation model (Q5099200) (← links)
- Constraints on the primordial curvature power spectrum by pulsar timing array data: a polynomial parameterization approach (Q6497845) (← links)
- An exact model for enhancing/suppressing primordial fluctuations (Q6558392) (← links)
- Realisation of the ultra-slow roll phase in Galileon inflation and PBH overproduction (Q6585226) (← links)
- Enhanced curvature perturbation and primordial black hole formation in two-stage inflation with a break (Q6589401) (← links)
- Primordial non-Gaussianity as a saviour for PBH overproduction in SIGWs generated by pulsar timing arrays for Galileon inflation (Q6598595) (← links)
- Generic predictions for primordial perturbations and their implications (Q6598615) (← links)
- Comparing sharp and smooth transitions of the second slow-roll parameter in single-field inflation (Q6623760) (← links)
