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Daniel Litim (University of Sussex)16/12/2024, 13:45
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Andreas Ringwald16/12/2024, 14:00
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Roberto Percacci16/12/2024, 14:45
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Kai Jรผrgen Spychala16/12/2024, 15:45
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Gabriel Picanco Costa16/12/2024, 16:30
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Latham Boyle (Higgs Centre for Theoretical Physics, University of Edinburgh)16/12/2024, 17:00
I will present the idea that the big bang is a type of mirror -- in particular a "CPT mirror". I will review the evidence for this idea, its explanatory power, and its predictions. Recently, we have come to think this idea is closely tied to the asymptotic safety idea, and I will present a new result to this effect (in collaboration with Neil Turok and Vatsalya Vaibhav -- to appear soon).
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16/12/2024, 17:45
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Christopher Herzog17/12/2024, 09:30
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Max Uetrecht (TU Dortmund University)17/12/2024, 10:15
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Charlie Cresswell-Hogg17/12/2024, 11:15
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Mireia Tolosa Simeon (Ruhr-Universitรคt Bochum), Mireia Tolosa Simeรณn17/12/2024, 12:00
The chiral Ising-, XY-, and Heisenberg models serve as effective descriptions of Dirac semimetals undergoing a quantum phase transition into a symmetry-broken ordered state. Interestingly, their quantum critical points govern the physical behavior of the system in the vicinity of the transition even at finite temperatures. In this contribution, we explore the chiral models at zero and finite...
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Mr Yannick Kluth (University of Manchester)17/12/2024, 14:00
We investigate $\beta$-functions of quantum gravity using dimensional regularisation. In contrast to minimal subtraction, a non-minimal renormalisation scheme is employed which is sensitive to power-law divergences from mass terms or dimensionful couplings. By construction, this setup respects global and gauge symmetries, including diffeomorphisms, and allows for systematic extensions to...
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Renata Ferrero17/12/2024, 14:45
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Marc Schiffer (Radboud University Nijmegen)17/12/2024, 16:00
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Riccardo Martini (UniBo and INFN - Bologna)17/12/2024, 16:45
I will introduce the concept of restricted Weyl invariances and discuss their advantages for matter fields in curved space and their disadvantages for quantum gravity.
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17/12/2024, 17:30
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Dr Simone Blasi (DESY)18/12/2024, 09:30
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Bilal Hawashin (RUB)18/12/2024, 10:15
Spontaneous symmetry breaking can persist at all temperatures in certain biconical $\mathrm{O}(N)\times \mathbb{Z}_2$ vector models when the underlying field theories are ultraviolet complete. So far, the existence of such theories has been established in fractional dimensions for local but nonunitary models or in 2+1 dimensions but for nonlocal models. Here, we study local models at zero and...
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Joรฃo Viana (Faculdade de Ciรชncias da Universidade de Lisboa), Joรฃo Viana18/12/2024, 11:15
Strong first-order phase transitions (SFOPT) during the evolution of the Higgs potential in the early universe not only allow for the dynamical generation of the observed matter-antimatter asymmetry, they can also source a stochastic gravitational wave (GW) background possibly detectable with future space-based gravitational waves interferometers. As SFOPTs are phenomenologically incompatible...
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Moritz Bosse (TU Dortmund)18/12/2024, 12:00
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Enrico Maria Sessolo18/12/2024, 14:00
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Joachim Brod (University of Cincinnati)18/12/2024, 14:45
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Tania Natalie Robens (Rudjer Boskovic Institute (HR))18/12/2024, 15:45
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Diego Buccio (SISSA)18/12/2024, 16:30
Running coupling were introduced in quantum filed theory in order to preserve perturbativity in scattering amplitudes, despite the appearance of large logs of external momenta. It is commonly believed that these logarithms are directly related to UV divergencies in one-loop perturbation theory, however this is not completely true in higher derivative theories. On one hand, large logs can...
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Gabriel Assant18/12/2024, 17:00
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18/12/2024, 17:30
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Tom Steudtner19/12/2024, 09:30
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Katerina Lipka (Deutsches Elektronen-Synchrotron (DE))19/12/2024, 10:00
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Geraldine Servant (Deutsches Elektronen-Synchrotron (DE))19/12/2024, 11:15
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Juri Smirnov19/12/2024, 12:00
An ultra-light axion with CP violating interactions with a dark sector and CP preserving interac- tions with the visible sector can act as a novel portal between dark matter and the Standard Model. In such theories, dark matter sources an axion field extending over the entire galaxy, the gradient of which can be searched for with precise spin precession experiments. A reinterpretation of...
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19/12/2024, 12:30
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