RubricaRubrica Cerca nel sitoCerca nel sito ModulisticaModulistica WebmailWebmail
Il Dipartimento sui social: Seguici su Facebook Seguici su Facebook Seguici su Youtube

Contenuti pagina [0] | Menù [1] | Copyright e credits [2]

Dipartimento di Fisica

Sei in »» The first detection of gravitational waves produced by colliding neutron stars by LIGO and Virgo and the starting gun of the multi-messenger... » Seminari Pubblici » Leggi

The first detection of gravitational waves produced by colliding neutron stars by LIGO and Virgo and the starting gun of the multi-messenger...
Speaker Speaker: Luciano Nicastro e Eliana Palazzi
Affiliato Affiliato: INAF Bologna
Data Evento Martedì 07 Novembre 2017, alle ore 15.00 - Aula Seminari
The first detection of gravitational waves produced by colliding neutron stars by LIGO and Virgo and the starting gun of the multi-messenger astronomy era

In September 2015, the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) detected, for the first time, gravitational waves (GWs) from the merging of two black holes (BHs) of stellar origin, at an approximate distance of 1.4 billion light years. In August 2017, the same international collaboration, which now could use data from the Virgo interferometer in Cascina (near Pisa), detected the GW signal originating from the merging of two neutron stars. The two bodies are less massive and closer than previous LIGO/Virgo discoveries. Moreover, in this last case, the very exceptional result was that scientists were able to subsequently identify the electromagnetic emission (using both space and ground-based telescopes) of the transient event, which obviously was not possible with BH mergers. We will give an overview of the global effort that led to the discovery of the source, named GW170817, and its scientific implications which marked the beginning of the era of multi-messenger astronomy.