Large fluctuations in the Sky
arXiv:2403.07343 · doi:10.1142/S0218271824410074
Abstract
Renormalization of quantum loop effects generated from large fluctuations is a hugely debatable topic of research these days which rules out the Primordial Black Hole (PBH) formation within the framework of single-field inflation. In this article, we briefly discuss that the correct implementation of regularization, renormalization, and resummation techniques in a setup described by an ultra-slow-roll phase sandwiched between two slow-roll phases in the presence of smooth or sharp transitions can lead to a stringent constraint on the PBH mass (i.e. )), which we advertise as a new No-go theorem. Finally, we will give some of the possible way-outs using which one can evade this proposed No-go theorem and produce solar/sub-solar mass PBHs.
15 pages (10 pages material + 5 pages references), Essay written and received honorable mention for the Gravity Research Foundation 2024 Awards for Essays on Gravitation, Comments are welcome, Accepted for publication in Int. J. Mod. Phys. D (for the special issue on Gravity Research Foundation 2024 Awards for Essays on Gravitation)
References in corpus (4)
Cited by in corpus (10)
- Primordial regular black holes as all the dark matter. II. Non-time-radial-symmetric and loop quantum gravity-inspired metrics
- Primordial regular black holes as all the dark matter. I. Time-radial-symmetric metrics
- Realisation of the ultra-slow roll phase in Galileon inflation and PBH overproduction
- Proving the absence of large one-loop corrections to the power spectrum of curvature perturbations in transient ultra-slow-roll inflation within the path-integral approach
- Obviating PBH overproduction for SIGWs generated by Pulsar Timing Arrays in loop corrected EFT of bounce
- Untangling PBH overproduction in -SIGWs generated by Pulsar Timing Arrays for MST-EFT of single field inflation
- Mechanisms for producing Primordial Black Holes from Inflationary Models Beyond Fine-Tuning
- Primordial regular black holes as all the dark matter. III. Covariant canonical quantum gravity models
- Negative non-Gaussianity as a salvager for PBHs with PTAs in bounce
- Stochastic origin of primordial fluctuations in the Sky