-
Dr Catalina Oana Curceanu (LNF), Mr Kristian Piscicchia (LNF)11/27/15, 9:30 AM
-
Dr Catalina Oana Curceanu (LNF)11/27/15, 9:45 AM
-
Dr Stefano Campion (Universita' La Sapienza, Roma)11/27/15, 10:15 AM
-
Prof. Marco Merafina (University of Rome La Sapienza)11/27/15, 10:30 AMA new family of nonrelativistic, Newtonian non quantum equilibrium configurations describing galactic halos is introduced taking into account a new possibility to identify particles with masses larger than 1 GeV as components of the dark matter. This possibility may have important implications on the formation of very massive particles during the big bang. The obtained results are in...Go to contribution page
-
Oscar Straniero (N)11/27/15, 11:30 AM
-
Dr Martina Donnari (Università di Roma "Sapienza")11/27/15, 12:00 PMThe role of Dark Energy (DE) in the long term evolution of galaxy clusters is the main topic of this talk. Recently, observational data of the outflow of galaxies in the Virgo cluster, suggest that DE can also act on a small cosmic scales, like a single galaxy cluster. By means of direct N-body we performed several simulations in which a galaxy cluster is undergo to the action of the DE force...Go to contribution page
-
Alessandro Scordo (LNF)11/27/15, 12:30 PM
-
Dr Francesco Gabriele Saturni (Dip. di Fisica - Universita' degli Studi di Roma "La Sapienza")11/27/15, 1:00 PMArrays of Cherenkov telescopes constitute the instrumental frontier for the ground-based gamma-ray astronomy. Their activity has presently led to great improvements in high-energy imaging and source discovery, also providing new tools to study cosmic rays, photon propagation in the Universe and dark matter (DM). In particular, the indirect search for DM through the detection of gamma rays...Go to contribution page
-
Prof. Damir Bosnar (Department of Physics, Faculty of Science, University of Zagreb)11/27/15, 2:30 PMThe structure of nuclei can be well described by independent particle models assuming movement of nucleons in nuclear mean field. However, some basic properties of nuclei such as nuclear binding energies cannot be reproduced without introduction of mechanisms beyond this assumption, such as nucleon-nucleon correlations. The same phenomena are responsible for the existence of the nuclear states...Go to contribution page
-
Dr Raffaele Del Grande (LNF-INFN)11/27/15, 3:00 PM
-
Mr Kristian Piscicchia (LNF)11/27/15, 3:30 PMThe AMADEUS experiment deals with the investigation of the low-energy kaon-nuclei hadronic interaction at the DAΦNE collider at LNF-INFN, trying to answer pending questions in the non-perturbative strangeness QCD sector. AMADEUS step 0 consisted in the reanalysis of 2004/2005 KLOE data, exploiting $K^−$ absorptions in H, ${}^4$He, ${}^9$Be and ${}^{12}$C, leading to the first invariant mass...Go to contribution page
-
Domenico Logoteta (PI)11/27/15, 4:30 PMWe calculate the energy per particle of symmetric nuclear matter and pure neutron matter using the many Brueckner-Hartree-Fock approach and employing the Chiral Next-to-next-to next-to leading order (N3LO) nucleon-nucleon (NN) potential, supplemented with various parametrizations of the Chiral Next-to-next-to lead-ing order (N2LO) three-nucleon force. Such combination is able to reproduce...Go to contribution page
-
Alessandro Drago (FE)11/27/15, 5:00 PMWe propose a model for short duration gamma-ray bursts (sGRBs) based on the formation of a quark star after the merger of two neutron stars. We assume that the sGRB central engine is a proto-magnetar, which has been previously invoked to explain the plateau-like X-ray emission observed following both long and short GRBs. Here, we show that: i) a few milliseconds after the merger it is possible...Go to contribution page
-
11/27/15, 5:30 PM
Choose timezone
Your profile timezone: