SUSYDM-PHEN

Supersymmetric Dark Matter and Collider Phenomenology

 Coordinatore "NATIONAL CENTER FOR SCIENTIFIC RESEARCH ""DEMOKRITOS""" 

 Organization address address: Patriarchou Gregoriou Str.
city: AGHIA PARASKEVI
postcode: 15310

contact info
Titolo: Ms.
Nome: Styliani
Cognome: Martaki
Email: send email
Telefono: +30 210 6503039
Fax: +30 210 65 24 965

 Nazionalità Coordinatore Greece [EL]
 Totale costo 100˙000 €
 EC contributo 100˙000 €
 Programma FP7-PEOPLE
Specific programme "People" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call FP7-PEOPLE-2007-4-3-IRG
 Funding Scheme MC-IRG
 Anno di inizio 2007
 Periodo (anno-mese-giorno) 2007-09-01   -   2011-08-31

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    "NATIONAL CENTER FOR SCIENTIFIC RESEARCH ""DEMOKRITOS"""

 Organization address address: Patriarchou Gregoriou Str.
city: AGHIA PARASKEVI
postcode: 15310

contact info
Titolo: Ms.
Nome: Styliani
Cognome: Martaki
Email: send email
Telefono: +30 210 6503039
Fax: +30 210 65 24 965

EL (AGHIA PARASKEVI) coordinator 0.00
2    UNIVERSITY OF PATRAS

 Organization address address: UNIVERSITY CAMPUS RIO PATRAS
city: RIO PATRAS
postcode: 26500

contact info
Titolo: Ms.
Nome: Styliani
Cognome: Martaki
Email: send email
Telefono: +30 210 6503039
Fax: +30 210 6524965

EL (RIO PATRAS) participant 0.00

Mappa


 Word cloud

Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.

satellite    physics    experiments    models    standard    lsp    model    relic    baryonic    dm    density    dark    possibility    years    supersymmetric    particle    explore    energy    context    collider    cosmological   

 Obiettivo del progetto (Objective)

'The compilation of the recent cosmological data from experiments in cosmology and astrophysics, and in particular of those of the WMAP satellite, confirm with greater accuracy the standard cosmological model. According to them the current energy density of the Universe is comprised by about 70% of dark energy and 30% of matter, most of which is in the form of non-baryonic dark matter (DM). It has been appreciated for some time that the lightest supersymmetric particle (LSP) is a suitable candidate for this non-baryonic cold dark matter. The LSP is stable in supersymmetric models where R-parity is conserved, and its relic density falls naturally within the favoured range if it weighs less than 1 TeV. In this case the most of the parameter space of the supersymmetric models can be explored by the future high energy experiments, like these that will be performed at LHC collider at CERN after about two years and at the International Linear Collider some years later. This, in conjunction with the upcoming information from projects like the PLANCK satellite and the various neutrinos telescopes, will provide us with the unique opportunity to comprehend the fundamental physics beyond the Standard Model of the particle physics. We will study the effect of the presence of CP violating phases on direct and indirect DM experiments, in the context of variants of the Minimal Supersymmetric Standard Model (MSSM), and we will impose the cosmological constraints by estimating precisely the neutralino relic density. In doing so, we will explore the complementarity between the accelerator and DM searches. In addition, we will investigate the possibility of baryogenesis through leptogenesis in this framework. On the other hand, we will study the possibility that the LSP is the gravitino, the supersymmetric partner of the graviton, and we will explore the interplay between the DM and the Dark Energy, in the context of grand unified and string models.'

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