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53. International Winter Meeting on Nuclear Physics

26–30 Jan 2015
Bormio, Italy
Europe/Berlin timezone

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Session

Thursday Morning

29 Jan 2015, 09:00
Bormio, Italy

Bormio, Italy

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  1. 62. Dark Matter Search with CREST
    Dr Jean-Come Lanfranchi (TU-Muenchen)
    29/01/2015, 09:00
    Overview Talk
    Dark Matter Search with CREST
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  2. 67. Super Heavy Elements
    Dr Michael Block (GSI)
    29/01/2015, 09:40
    Nuclear Structure and Astrophysics
    Overview Talk
    Super Heavy Elements
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  3. 2. Muons: civil applications
    Germano Bonomi (Department of Mechanical and Industrial Engineering - University of Brescia)
    29/01/2015, 10:50
    Applications and Instrumentations
    Extended Contribution
    Cosmic radiation has been known since the first decades of the 20th century: it has been considered for many years, the best source of projectiles to investigate the core of matter, from nuclei to elementary particles. Nowadays, cosmic ray muons are very important in particle and nuclear physics, because they are used for detector testing and calibration, and for detector alignment in complex...
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  4. 8. Hadron physics from Dyson-Schwinger equations
    Prof. Christian Fischer (JLU Giessen)
    29/01/2015, 11:20
    Hadron Physics
    Extended Contribution
    We summarise recent results on spectra and electromagnetic properties of ground and excited hadronic states determined in the framework of Dyson-Schwinger, Bethe-Salpeter and Faddeev-equations. We discuss the effects of dynamical quark mass generation and dynamically generated pion cloud contributions to the spectra of mesons and baryons. Also we plan to discuss first results for...
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  5. 20. Looking the Universe from Deep Underground
    Dr Davide Trezzi (Università degli Studi di Milano / INFN)
    29/01/2015, 12:00
    Extended Contribution
    The abundance of primordial light nuclei at the beginning of the Universe, during the so called Big Bang Nucleosynthesis era (BBN), can be estimated by means of Cosmology, Particle and Nuclear Physics. The first two give the environmental conditions and information about nucleons present at that time. The last one describes how those primordial nucleons fused themselves in order to produce the...
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