Season 6 Episode 4 PhD Seminar

Wednesday 22 Mar 2023, 18:15 → 19:45 Europe/Rome

Aula Conversi (VEF) and Zoom

28th meeting of physics PhD seminar series

If you want to attend in person, sign the doodle here:
https://doodle.com/meeting/participate/id/dGZQPMJb

https://uniroma1.zoom.us/skype/93015880584 or open Zoom and insert the Meeting ID
Meeting ID: 930 1588 0584

Passcode: 486750

 

Please sign up to the mailing list:
https://groups.google.com/u/1/a/uniroma1.it/g/phd-seminars

You can submit abstracts using the following link:

https://forms.gle/mgwxqH7dwPHT66gk7

1 Turbulence: an informal introduction

Did you know that one of the biggest present challenges in physics, mathematics and applied sciences deals with...classical mechanics? In fact the turbulent motion of fluids, despite centuries-long studies, still lacks fundamental mathematical proofs and a "unified" physical theory able to explain all the complicated features it presents. In this basic-level presentation I will introduce this fascinating subject, with the least possible number of formulas and many cool images and videos.

Speaker: Niccolò Cocciaglia

Cocciaglia PhD Seminar.pptx

2 Dicussion

3 Boson stars as targets of gravitational wave searches and probes of new fundamental fields

Gravitational astronomy provides a new, powerful tool to investigate the previously unexplored strong-field regime of gravity, in which compact bodies evolve and emits gravitational waves in a highly dynamical and non-linear evolution. A cornerstone of such research program is represented by the opportunity to test the nature of the most compact astrophysical objects known and to explore the possibility that compact sources other than black holes and neutron stars may exist in the Universe, leaving detectable signatures in the emitted gravitational signals. Within the variety of proposals, boson stars stand among the best motivated models, and can be interpreted as self-gravitating condensates of astronomical size, composed of either scalar or vector massive fields. During the talk I will discuss some of their main features and how these can be used to construct waveform templates in order to search for these objects and infer constraints on their fundamental properties with future observations by ground and space-based interferometers.

Speaker: Massimo Vaglio

PhDSem_S6Ep4_Vaglio.pdf

4 Discussion