2024 NCSRD - INPP Annual Meeting
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INPP Overview¶Speakers: Dr Christos Markou (Nat. Cent. for Sci. Res. Demokritos (GR)), Christos Markou (Institute of Nuclear Physics)
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ESI Overview¶Speaker: Aikaterini Tzamarioudaki (Nat. Cent. for Sci. Res. Demokritos (GR))
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CMS Activities 2024¶Speaker: Dr Aristoteles Kyriakis (Nat. Cent. for Sci. Res. Demokritos (GR))
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11:45
Coffee Break
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Two -Dimensional Mass Reconstruction in Top Pair Dilepton Topologies for High-Mass Resonance Searches Using CMS 2017 Dataset¶Speaker: Stelios Chistinakis
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2-Dimensional Mass Reconstruction in Asymmetric Topologies with Two Invisible Particles¶Speaker: Evdoxia Kalpakidou
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AILAB Activities 2024¶Speaker: Dr Aristoteles Kyriakis (Nat. Cent. for Sci. Res. Demokritos (GR))
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Semi-autonomous rover for Radiation Source Localization¶Speakers: Dr Aristoteles Kyriakis (Nat. Cent. for Sci. Res. Demokritos (GR)), John Karagiannis
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13:15
Lunch Break
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Overview of XRF Laboratory activities¶Speaker: Kalliopi Tsampa
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10
Chemical degradation of iron gall inks based on historical Byzantine recipes. Investigation of the role of metal ions by non-destructive analytical spectroscopic techniques¶Speaker: Ermioni Vassiou
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Study of the 11B(p,a0)8Be and 6Li(p,3He)4He reactions in the low energy range, suitable for NRA purposes¶Speaker: Evagelia Taimpiri
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Measurements of (p,γ) and (α,γ) reaction cross-sections for nuclear astrophysics purposes¶Speaker: Maria Peoviti
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16:00
Coffee Break
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14
ATLAS/Demokritos group research activities¶Speaker: Theodoros Geralis (Nat. Cent. for Sci. Res. Demokritos (GR))
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15
NSW Pad Trigger for the ATLAS experiment¶Speaker: Eleni Kanellaki (Nat. Cent. for Sci. Res. Demokritos (GR))
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ESSnuSB neutrino project at the European Spallation Source¶Speaker: Georgios Fanourakis (Nat. Cent. for Sci. Res. Demokritos (GR))
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KM3NET Overview¶Speakers: Evangelia Drakopoulou (N.C.S.R. DEMOKRITOS), Evangelia Drakopoulou (Nat. Cent. for Sci. Res. Demokritos (GR))
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18
Diffuse astrophysical neutrino flux searches with KM3NeT/ARCA¶Speaker: Vasileios Tsourapis
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KM3NeT/ARCA differential sensitivity studies¶Speaker: Lida Liogka
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20
Activities of the HEP-TH group¶Speakers: Giuseppe Bevilacqua (Istituto Nazionale Fisica Nucleare (IT)), Giuseppe Bevilacqua (NCSR Demokritos)
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11:30
Coffee Break
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Special Seminar: Forward Physics Facility @ CERN: The Astroparticle Connection¶
There is a renaissance of neutrino physics at CERN with the detection of TeV energy neutrinos from the colliding beams at the LHC by the FASER & SND detectors. There is much exciting physics that can be done at the proposed Forward Physics Facility of direct relevance to astroparticle physics experiments like cosmic neutrino telescopes and cosmic ray air shower arrays. I will discuss relevant topics such as neutrino interactions, forward charm & light hadron production and searches for new physics beyond-the-Standard-Model.
Speakers: Prof. Subir Sarkar (University of Oxford), Subir Sarkar (Saha Institute of Nuclear Physics (IN)) -
12:45
Lunch Break
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The hidden simplicity of complexity: Field theories of Arnol'd cats¶Speaker: Stam NICOLIS
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23
Landscape of the QCD Vacuum¶
We found new solutions of the sourceless Yang-Mills equation describing the superposition of chromomagnetic vortices of oppositely oriented magnetic fluxes. These gauge field configurations have constant energy densities and are separated by potential barriers forming a complicated landscape. It is suggested that the solutions describe the condensate of chromomagnetic vortices and represent a dual analog of the Cooper pairs condensate in a superconductor. In the presence of an Abelian field and in a particular limit the solutions reduce to flat connections of zero energy density and are forming a complicated potential landscape of the QCD vacuum. A possible tunnelling transition between these superfluxon flat configurations and the flat configurations with non-vanishing Chern-Pontryagin index will wash out the CP violating 𝜃 angle to zero, dynamically restoring CP symmetry.
Speakers: Prof. Georgios Savvidis (Nat. Cent. for Sci. Res. Demokritos (GR)), Georgios Savvidis (Nat. Cent. for Sci. Res. Demokritos (GR)) - 24
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KM3NeT/ARCA expectations for the diffuse astrophysical neutrino flux¶Speaker: Chrisovalantis Karagiannis
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