Theoretical Physics Division seminar
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Heavy H isotopes: theory ad experiments
2022.12.08 10:44 - Katarzyna KuźniarI will present an experimental and theoretical review of the H isotopic chain going from the simple deuteron to the observed, but highly contested, 7H which is probably the very last observable H state. The difficulties in defining and extracting the resonance parameters as well as the different theoretical approaches to compute them will be discussed.
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Ascribing quantum system to Schwarzschild spacetime with naked singularity
2022.12.01 10:38 - Katarzyna Kuźniar -
"Exact solutions of Einstein's equations and Relativistic Zel'dovich Approximation"
2021.12.09 15:10 - Katarzyna Kuźniar -
"Homogeneous-isotropic sector of loop quantum gravity: new approach"
2021.11.25 15:57 - Katarzyna Kuźniar -
Physical implications of a fundamental period of time
2021.10.22 12:36 - Katarzyna Kuźniar -
Hunting for FIMPs at particle colliders and in the sky
2021.06.07 11:20 - Anna RędaszekABSTRACT:
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A discussion on the flavor anomalies
2021.05.13 22:29 - Anna RędaszekIn this talk I will review the status of flavor physics after the first and second run of the LHC and in particular I will discuss recent results from the LHCb collaboration suggesting possible deviations from the SM predictions in semileptonic B-meson decays. I will also discuss possible interpretations of these anomalies in terms of New Physics.
Best regards,
T. Altinoluk, M. Kowal, P. Małkiewicz, E. Sessolo, P. Zin -
The de Broglie--Bohm Approach to Quantum Cosmology
2021.05.07 8:41 - Anna RędaszekWe review the de Broglie--Bohm quantum theory, an alternative description of quantum phenomena in accordance with all the quantum experiments already performed. It is a dynamical theory about objectively real trajectories in the configuration space of the physical system under investigation, where probabilities of outcomes are not essential. Hence, it can be applied to single closed systems, being suitable for Cosmology. The emerging cosmological models are usually free of singularities, with a bounce connecting a contracting era with an expanding phase, which we are now observing.