From elia.battistelli at roma1.infn.it  Mon Mar  6 15:30:54 2017
From: elia.battistelli at roma1.infn.it (Elia Battistelli)
Date: Mon, 06 Mar 2017 15:30:54 +0100
Subject: [astroseminar@Sapienza] today at 16:30: Daniele Fargion
Message-ID: <cc95a5c8f5d77f40266919ae8e5b1f06@roma1.infn.it>

Title: Introduzione alle recenti scoperte dell' Astrofisica
Speaker:   Daniele Fargion
Institute: Sapienza Universit? di Roma e INFN, Sezione di Roma
Date: Monday, 6 March 2017
Time: 4:30pm
Location: Aula Conversi, Marconi Building, Dept. of Physics, Sapienza 
University

Abstract:
Da 70 anni l'astronomia ottica e' stata estesa all'astrofisica radio, 
poi X e quind gamma,  rivoluzionando  il cielo e le nuove sorgenti.
30 anni fa una Supernova vicina,  la 1987A, ci illuminava per la prima 
volta di neutrini, aprendo,( con il Sole), una nuova finestra nel cielo.
Da pochi anni nuovi rivelatori vedono, energetici neutrini e 
potentissimi raggi cosmici, da sorgenti violente.
Infine da un anno si possono udire ultimi sussulti gravitazionali di 
unioni e collassi di buchi neri.
Nuovissime finestre su astronomie quasi invisibili ma di
massima potenza.

web: https://agenda.infn.it/conferenceDisplay.py?confId=12859


From elia.battistelli at roma1.infn.it  Fri Mar 10 18:13:41 2017
From: elia.battistelli at roma1.infn.it (Elia Battistelli)
Date: Fri, 10 Mar 2017 18:13:41 +0100
Subject: [astroseminar@Sapienza] =?utf-8?q?15/03/2017_at_16=3A00=3A_=C3=81?=
	=?utf-8?q?ngeles_Molin=C3=A9?=
Message-ID: <a302c45c42c88aeeb412534bc17a8a73@roma1.infn.it>

Title: Indirect DM searches and DM halo models
Speaker:   Prof. ?ngeles Molin?
Institute: Instituto de Astrof?sica e Ci?ncias do Espa?o, Departamento 
de F?sica da FCUL, Lisboa, Portugal
Date: Wednesday, 15 March 2017
Time: 4:00pm
Location: Aula 4, Fermi Building, Dept. of Physics, Sapienza University

Abstract:
Today there exists a strong evidence to believe that most of the matter 
in our Universe is made of dark matter (DM). In the last years, a huge 
effort has been focused on understanding its nature as well as its 
detection. The indirect detection of DM, namely, the detection of the 
annihilation or decay products of DM particles, is a useful and 
important tool. First, in this talk I will focus on the contribution to 
the diffuse neutrino and gamma-ray background from DM annihilations in 
halos at several redshifts and the role of subhalos on such searches. 
Finally, I will briefly present the guidelines for a project that will 
be carried out with Dr. Carlos Arguelles and other members of ICRANet 
and UNLP-CONICET, about the emission in the X-ray background that would 
be produced by decay of sterile neutrino DM from the galactic center. 
This study will be performed assuming the Ruffini-Arguelles-Rueda (RAR) 
model, for the distribution of DM in galaxies.

web: https://agenda.infn.it/conferenceDisplay.py?confId=13138


From elia.battistelli at roma1.infn.it  Tue Mar 14 15:16:35 2017
From: elia.battistelli at roma1.infn.it (Elia Battistelli)
Date: Tue, 14 Mar 2017 15:16:35 +0100
Subject: [astroseminar@Sapienza] =?utf-8?q?15/03/2017_at_16=3A00=3A_=C3=81?=
 =?utf-8?q?ngeles_Molin=C3=A9=3A_CANCELLED?=
Message-ID: <de9246fd40bcf4b4a1087cbe9fbad5eb@roma1.infn.it>


THIS IS TO INFORM THAT DUE TO PERSONAL REASONS Prof. ?ngeles MOLIN? HAD 
TO CANCEL HER SEMINAR


Title: Indirect DM searches and DM halo models
Speaker:   Prof. ?ngeles Molin?
Institute: Instituto de Astrof?sica e Ci?ncias do Espa?o, Departamento 
de F?sica da FCUL, Lisboa, Portugal
Date: Wednesday, 15 March 2017
Time: 4:00pm
Location: Aula 4, Fermi Building, Dept. of Physics, Sapienza University

Abstract:
Today there exists a strong evidence to believe that most of the matter 
in our Universe is made of dark matter (DM). In the last years, a huge 
effort has been focused on understanding its nature as well as its 
detection. The indirect detection of DM, namely, the detection of the 
annihilation or decay products of DM particles, is a useful and 
important tool. First, in this talk I will focus on the contribution to 
the diffuse neutrino and gamma-ray background from DM annihilations in 
halos at several redshifts and the role of subhalos on such searches. 
Finally, I will briefly present the guidelines for a project that will 
be carried out with Dr. Carlos Arguelles and other members of ICRANet 
and UNLP-CONICET, about the emission in the X-ray background that would 
be produced by decay of sterile neutrino DM from the galactic center. 
This study will be performed assuming the Ruffini-Arguelles-Rueda (RAR) 
model, for the distribution of DM in galaxies.

web: https://agenda.infn.it/conferenceDisplay.py?confId=13138


