Majorana-Raychaudhuri Seminars
Welcome to Majorana-Raychaudhuri Seminars. We organise seminars in the field of Quantum Field Theory, Gravitation, Cosmology and Particle Physics on Fridays at 16.30 - 18.00 (IST*) / 12.00 - 13.00 (CET*) as a joint venture of INFN & University Salerno, Italy & PAMU, Indian Statistical Institute, Kolkata, India.
Please use this link to join the seminar.
Seminars This Week:
November 15, 2024: (12:00 - 12:45 CET/ 16:30 - 17:15 IST)
Title: Some properties of Gravitational Waves in Modified Theories of Gravity
Abstract: In this talk, at first, I'll briefly discuss polarisation modes of Gravitational Waves (GWs) in modified theories of gravity mainly focusing on f(R) gravity metric formalism and Palatini formalism. After that I'll discuss quasinormal modes of black holes or ring-down GWs in some selected modified theories of gravity. These two properties may be helpful in the near future to constrain different modified theories of gravity.
November 15, 2024: (12:45 - 13:30 CET/ 17:15 - 18:00 IST)
Title: Smooth reheating via non-Abelian dark sector
Abstract: We consider a model, where a single inflaton interacts weakly as an axion with Yang-Mills gauge bosons. As these rapidly thermalize, the friction felt by the inflaton field is increased, leading to a self-amplifying process. If the gauge bosons of the thermal bath represent a dark sector, the reheating of the Standard Model is then realised through portal interactions. The dark relic abundance in this scenario depends mostly on the departure from equilibrium after the universe cools down below the critical temperature, when the dark vectors confine into composite states. This constrains the confinement scale of the dark sector. Moreover, indirect detection and Big-Bang nucleosynthesis set bounds on the portal interactions, revealing a predictive parameter space.
November 15, 2024: (13:30 - 14:15 CET/ 18:00 - 18:45 IST)
Title: Gravitational Waves from Stochastic Scalar Fluctuations
Abstract: In this talk, we will present a novel mechanism for gravitational wave generation in the early Universe. Light spectator scalar fields during inflation can acquire a blue-tilted power spectrum due to stochastic effects. We show that this effect can lead to large curvature perturbations at small scales (induced by the spectator field fluctuations) while maintaining the observed, slightly red-tilted curvature perturbations at large cosmological scales (induced by inflaton fluctuations). Along with other observational signatures, such as enhanced dark matter substructure, large curvature perturbations can induce a stochastic gravitational wave background (SGWB). We will discuss this mechanism in detail and present several benchmark scenarios that result in gravitational wave strengths visible to near-future detectors.
Organisers:
Gaetano Lambiase (University & INFN Salerno, Italy)
Supratik Pal (PAMU - ISI, Kolkata, India)
Anish Ghoshal (University of Warsaw, Poland)
Arnab Paul (Indian Institute of Technology Madras, India)
Shiladitya Porey (Novosibirsk State University, Russia)