The swampland: introduction and review
E Palti - Fortschritte der Physik, 2019 - Wiley Online Library
The Swampland program aims to distinguish effective theories which can be completed into
quantum gravity in the ultraviolet from those which cannot. This article forms an introduction …
quantum gravity in the ultraviolet from those which cannot. This article forms an introduction …
[图书][B] Inflation and string theory
D Baumann, L McAllister - 2015 - books.google.com
The past two decades have seen transformative advances in cosmology and string theory.
Observations of the cosmic microwave background have revealed strong evidence for …
Observations of the cosmic microwave background have revealed strong evidence for …
New horizons in cosmology with spectral distortions of the cosmic microwave background
This Voyage 2050 paper highlights the unique science opportunities using spectral
distortions of the cosmic microwave background (CMB). CMB spectral distortions probe …
distortions of the cosmic microwave background (CMB). CMB spectral distortions probe …
CMB-S4 science book
This book lays out the scientific goals to be addressed by the next-generation ground-based
cosmic microwave background experiment, CMB-S4, envisioned to consist of dedicated …
cosmic microwave background experiment, CMB-S4, envisioned to consist of dedicated …
Probing the inflaton: Small-scale power spectrum constraints from measurements of the cosmic microwave background energy spectrum
In the early universe, energy stored in small-scale density perturbations is quickly dissipated
by Silk damping, a process that inevitably generates μ-and y-type spectral distortions of the …
by Silk damping, a process that inevitably generates μ-and y-type spectral distortions of the …
Inner cusps of the first dark matter haloes: formation and survival in a cosmological context
We use very high resolution cosmological zoom simulations to follow the early evolution of
12 first-generation haloes formed from gaussian initial conditions with scale-free power …
12 first-generation haloes formed from gaussian initial conditions with scale-free power …
CMB at 2× 2 order: the dissipation of primordial acoustic waves and the observable part of the associated energy release
Silk damping of primordial small-scale perturbations in the photon–baryon fluid due to
diffusion of photons inevitably creates spectral distortions in the cosmic microwave …
diffusion of photons inevitably creates spectral distortions in the cosmic microwave …
Spectral distortions of the CMB as a probe of inflation, recombination, structure formation and particle physics
Following the pioneering observations with COBE in the early 1990s, studies of the cosmic
microwave background (CMB) have focused on temperature and polarization anisotropies …
microwave background (CMB) have focused on temperature and polarization anisotropies …
[HTML][HTML] Higgs inflation at the critical point
F Bezrukov, M Shaposhnikov - Physics Letters B, 2014 - Elsevier
Higgs inflation can occur if the Standard Model (SM) is a self-consistent effective field theory
up to inflationary scale. This leads to an upper bound on the top Yukawa coupling, yt phys< …
up to inflationary scale. This leads to an upper bound on the top Yukawa coupling, yt phys< …
Primordial black holes dark matter from inflection point models of inflation and the effects of reheating
We study the generation of primordial black holes (PBH) in a single field inflection point
model of inflation wherein the effective potential is expanded up to the sextic order and the …
model of inflation wherein the effective potential is expanded up to the sextic order and the …