After reviewing the motivations for cosmological inflation formulated in the formalism of
supersymmetry, we argue that the appropriate framework is that of no-scale supergravity …

We investigate the power spectrum of Non-Cold Dark Matter (NCDM) produced in a state out
of thermal equilibrium. We consider dark matter production from the decay of scalar …

Recent BICEP/Keck data on the cosmic microwave background, in combination with
previous WMAP and Planck data, impose strong new constraints on the tilt in the scalar …

We compute the density of a spin-3 2 particle, the raritron, produced at the end of inflation
due to gravitational interactions. We consider a background inflaton condensate as the …

We argue that accidental approximate scaling symmetries are robust predictions of weakly
coupled string vacua, and show that their interplay with supersymmetry and other …

It has been argued that supergravity models of inflation with vanishing sound speeds, cs,
lead to an unbounded growth in the production rate of gravitinos. We consider several …

A bstract A discrepancy between the measured anomalous magnetic moment of the muon
(g− 2) μ and computed Standard Model value now stands at a combined 4. 2σ following …

We explore various aspects concerning the role of vector bosons during the reheating
process. Generally, reheating occurs during the period of oscillations of the inflaton …

We propose a non-oscillatory no-scale supergravity model of inflation (NO-NO inflation) in
which the inflaton does not oscillate at the end of the inflationary era. Instead, the Universe is …

We explore various aspects concerning the role of vector bosons during the reheating
process. Generally, reheating occurs during the period of oscillations of the inflaton …