Conveners
Early Universe
- Mar Bastero Gil (University of Granada)
Early Universe
- Mar Bastero Gil (University of Granada)
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Juraj Klaric (Universiteit van Amsterdam, Nikhef)15/05/2024, 09:30early universe cosmology
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Dr Alexander Jenkins (University College London)15/05/2024, 10:00
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Mathias Pierre15/05/2024, 11:15
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Jesus Gambin Egea (Instituto de Fisica Teorica, UAM - CSIC)15/05/2024, 11:47early universe cosmology
A possible way to generate primordial black holes as candidates for the entirety of dark matter is a large power spectrum of inflationary curvature fluctuations. Recently, questions have been raised regarding the validity of perturbation theory in this context. We compute the one-loop power spectrum in ultra-slow roll inflation, including all relevant interactions for such analysis, along with...
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Oksana Iarygina (Nordita)15/05/2024, 11:54early universe cosmology
Nowadays, the search for primordial gravitational waves is mainly focused on the parity-odd polarization pattern in the CMB - the B-modes. A correct interpretation of B-mode measurements strongly relies on understanding their production mechanism. One intriguing scenario is gravitational waves generation by gauge fields. The tachyonic amplification of the gauge fields modes during inflation...
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Chiara Cecchini (University of Trento, TIFPA-INFN)15/05/2024, 12:01early universe cosmology
Fundamental scale invariance has been proposed as a new theoretical principle beyond renormalizability. Besides its highly predictive power, a scale-invariant formulation of gravity could provide a natural explanation for the long-standing hierarchy problem and interesting applications in cosmology.
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We present a globally scale-invariant model of quadratic gravity and study its solutions in a... -
Piotr Toczek (University of Warsaw)15/05/2024, 12:08early universe cosmology
Slow first-order phase transitions generate large inhomogeneities that can lead to the formation of primordial black holes (PBHs). We show that the gravitational wave (GW) spectrum then consists of a primary component sourced by bubble collisions and a secondary one induced by large perturbations. The latter gives the dominant peak if $\beta/H_0 < 10$, impacting, in particular, the...
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Ansh Bhatnagar (IPPP, Durham University)15/05/2024, 12:15early universe cosmology
In standard leptogenesis models, the baryon asymmetry is initially produced as a lepton asymmetry via the out of equilibrium decays of the lightest right handed neutrino (RHN).
There are however constraints on the RHN mass that are in tension; the naturalness constraint on the Higgs mass from RHN loop corrections, i.e. the Vissani bound, puts a limit on the RHN mass which is lower than is...
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Nicklas Ramberg (Johannes gutenberg universität Mainz)15/05/2024, 12:22early universe cosmology
We introduce a novel approach to investigate sectors solely gravitationally coupled, characterized by significant anisotropies. These anisotropies undergo damping through gravitational interactions with the baryon-photon fluid, inducing heating in the process. The resultant injected heat leads to observable distortions in the cosmic microwave background spectrum. We provide analytic estimates...
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