Conveners
Morning Session: Intro to Nuclear Physics, Nuclear Astrophysics
- Livius Trache (IFIN-HH)
Morning Session: Astroparticles
- Adam Maj (IFJ PAN)
Morning Session: Small Accelerators
- Razvan Lica
Morning Session: Nuclear Physics with lasers
- Olivier Sorlin (GANIL)
Morning Session: ELI-NP session
- Muhsin Harakeh (Univ. Groningen)
Morning Session: Outreach Session
- Timothy Jull (Univ. Arizona)
Morning Session: Nuclear Astrophysics (I)
- There are no conveners in this block
Morning Session: Nuclear Astrophysics (III)
- Bradley Meyer (Clemson University)
Morning Session
- There are no conveners in this block
Morning Session
- There are no conveners in this block
Morning Session
- There are no conveners in this block
We will introduce and review theoretical and phenomenological aspects on acceleration and propagation of ultra-high-energy cosmic rays, gamma-rays and neutrinos.
Model predictions for spectrum, composition and anisotropies of the ultra-high-energy multi-messenger sky will then be put in context with data from the Pierre Auger experiment.
We will review multi-messenger capabilities of the Pierre Auger
Observatory involving searches for high-energy neutrinos and photons from
transient events as well as searches for temporal and/or directional
correlations between different messengers including UHECR. Upper bounds on
the flux of up-going air showers – of the type that was reported by ANITA
- will be presented and used to...
We will review multi-messenger capabilities of the Pierre Auger
Observatory involving searches for high-energy neutrinos and photons from
transient events as well as searches for temporal and/or directional
correlations between different messengers including UHECR. Upper bounds on
the flux of up-going air showers – of the type that was reported by ANITA
- will be presented and used to...
The commissioning of the 1 PW experimental area has been successfully performed at ELI-NP with a TNSA experiment on proton acceleration and a LWFA experiment on electron acceleration. A brief introduction to the typical laser-driven acceleration mechanisms will be done, followed by the description of the typical laser parameters, setups, diagnostic and simulation tools and results obtained. In...
This talk will discuss the connection between nuclear and particle effects in supernovae and isotopic effects in planetary bodies in the Solar System.
I will discuss the longstanding puzzle of electron screening of nuclear reactions in the laboratory and within stars. A comparison between existing experimental data and multiple theories will be highlighted. I will focus on the modeling of nuclear/atomic reactions including (a) excitation, (b) ionization, (c) atomic transfer of electrons, (d) the role of stopping power at low energies and...
Rich experimental information obtained at AGS, RHIC and LHC in terms of
yield, average transverse momentum, transverse energy and suppression for light
flavor hadrons, is used to compare their dependence on the particle density per unit of
rapidity and unit of transverse overlapping area with predictions of phenomenological
models. At LHC energies such studies are extended to pp collisions...
Medium mass nuclei around the N = Z line offer new insights into the coexistence phenomena and the fundamental symmetries. The nuclei dominated by shape coexistence and mixing are of particular interest due to the open questions concerning the nature of the observed isomers, the irregularities in the excitation spectra, and their feeding by the β decay of the neighboring nuclei. On the...
In this talk I will discuss the evolution in the Nuclear Instrumentation (small scale experiments) over the last 20 years. I will start from the standard NIM detection system and evolve towards todays more and more digitized electronics and DAQ systems. The number of detectors and the size of the equipment has changed tremendously, but in partly in opposite direction to each other. However, in...
The aim of relativistic heavy ion accelerators is to study nuclear matter under extreme conditions. However, very strong electromagnetic fields for a very short time duration are present in distant collisions with no nuclear contact. Such strong fields can lead to nuclear fragmentation through the excitation of giant resonances or direct dissociation of light nuclei. This process can be used...
