Physics Beyond the Standard Model in Leptonic & Hadronic Processes and Relevant Computing Tools

Session

Research Talks of “Session 5”

27 Feb 2024, 11:00

Amphitheater "Alkis Argyriades" ( University of Athens, Greece )

39. Bound-spectra predictions in exotic muonic atoms through advanced numerical solutions of the Dirac Equations

Prof. Theocharis Kosmas (University of Ioannina)

Recently, appreciably sensitive experiments operating in frontier muon facilities at J-PARC in Tokio, PSI in Switzerland, Fermilab in USA, RCNP in Osaka, etc., provide ultra-high-precision measurements in muon physics for open problems in muon-nucleus processes and purely leptonic atomic systems [1,2]. A plethora of such processes are well analyzed and described by theories falling within (SM)...

30. Charged-current neutrino scattering off I-127 and Cs-133 and the effect of quenching and two-body currents.

Matti Hellgren

The stable iodine and caesium isotopes are the primary constituents of several
detectors including the CsI[Na] neutrino detector operational from 2015 to 2019
at the SNS. Theoretically computed cross sections for these nuclei are therefore
of considerable interest. The goal of the research outlined in this abstract was to
obtain accurate theoretical scattering cross sections for stopped...

11. Deformed shell model applications to weak interaction processes

Rankanidhi Sahu (National Institute of Sciene and Technology)

R. Sahu,1 V.K.B. Kota,2 and T.S. Kosmas3
1 National Institute of Science and Technology,
Palur Hills, Berhampur 761 008, Odisha, India
2 Physical Research Laboratory, Ahmedabad 380 009, India
3 Division of Theoretical Physics, University of Ioannina, GR 45110 Ioannina, Greece

The deformed shell model (DSM) was successful in describing many spectroscopic prop-
erties of medium maas...

8. Probing new physics with DUNE, CEvNS and dark matter direct detection experiments

Dr Dimitrios Papoulias (National and Kapodistrian University of Athens)

Intense neutrino beams with keV-GeV energies produce sizeable event rates through the elastic neutrino-electron scattering (EvES) and coherent elastic neutrino-nucleus scattering (CEvNS) chanels. In this talk, I will focus on solar as well as accelerator neutrinos from the Spallation Neutron Source at Oak Ridge and the Long Baseline Neutrino Facility (LBNF) at Fermilab. I will present recent...