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Wydział Fizyki UW > Badania > Seminaria i konwersatoria > Seminarium "Teoria cząstek elementarnych i kosmologia"

Seminarium "Teoria cząstek elementarnych i kosmologia"

2017/2018 | 2018/2019 | 2019/2020 | 2020/2021 | 2021/2022 | 2022/2023 | 2023/2024 | 2024/2025

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2025-01-23 (Czwartek)
Zapraszamy na spotkanie o godzinie 12:15  Calendar icon
Viatcheslav Mukhanov (Ludwig Maximilian University, Munich)

Gravitationally dominated instantons

We study the decay of the false vacuum in the regime where the quantum field theory analysis is not valid, since gravitational effects become important. This happens when the height of the barrier separating the false and the true vacuum is large, and it has implications for the instability of de Sitter, Minkowski and anti-de Sitter vacua. We carry out the calculations for a scalar field with a potential coupled to gravity, and work within the thin-wall approximation, where the bubble wall is thin compared to the size of the bubble. We show that the false de Sitter vacuum is unstable, independently of the height of the potential and the relative depth of the true vacuum compared to the false vacuum. The false Minkowski and anti-de Sitter vacua can be stable despite the existence of a lower energy true vacuum. However, when the relative depth of the true and false vacua exceeds a critical value, which depends on the potential of the false vacuum and the height of the barrier, then the false Minkowski and anti-de Sitter vacua become unstable. We calculate the probability for the decay of the false de Sitter, Minkowski and anti-de Sitter vacua, as a function of the parameters characterizing the field potential.
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2025-01-16 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Daniele Perri (IFT UW)

Magnetic monopoles in cosmic magnetic fields: acceleration and constraints

Magnetic monopoles are intriguing hypothetical particles and inevitable predictions of theories of Grand Unification. They should be produced during phase transitions in the early universe, but mechanisms like the Schwinger effect in strong magnetic fields could also contribute to the monopole number density. I will show how we can infer additional bounds on the magnetic monopole flux from detecting intergalactic magnetic fields, and how even well-established limits, such as Parker bounds and limits from terrestrial experiments, strongly depend on the acceleration in cosmic magnetic fields. I will also discuss the implications of these bounds for minicharged monopoles and magnetic black holes as dark matter candidates. Finally, we apply our primordial bounds to monopoles produced by the primordial magnetic fields themselves through the Schwinger effect, deriving necessary conditions for the survival of the primordial fields.
2024-12-19 (Czwartek)
Zapraszamy na spotkanie o godzinie 12:15  Calendar icon
Oleg Lebedev (Helsinki U.)

Predictive freeze-in

Non-thermal dark matter models suffer from the ever-presentgravitational particle production background, which marspredictivity of the framework altogether. I will discuss a classof freeze-in dark matter models with a low reheating temperaturethat are free of such problems and are directly testable.
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2024-12-12 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Theodoros Papanikolaou (SSM & INFN Napoli)

Primordial black holes and induced gravitational waves

Primordial black holes (PBHs) can generically form through the collapse of enhanced cosmological perturbations, constituting in some specific mass ranges a viable candidate for dark matter. Interestingly enough, the enhanced cosmological perturbations which collapse to form PBHs as well as the PBH energy density perturbations themselves can produce a stochastic gravitational-wave (GW) background induced by second-ordergravitational interactions, which can be detectable in GW observatories. In this talk, afterintroducing initially the motivation for the physics of PBHs and the associated to them GWsignals I will focus afterwards on the ultra-light PBH mass range and its induced GWsignatures through which one can probe the physics of the primordial Universe, theunderlying gravity theory testing as well fundamental high-energy physics theories.
2024-12-05 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Maxim Laletin (IFT UW)

Revisited axion contribution to dark radiation using momentum-dependent evolution

Axions can be produced via the interactions in the thermal plasma of the early Universe and their contribution to dark radiation can modify the cosmological observables and constrain the axion couplings to SM particles. In my talk I am going to outline an approach to calculate the axion cosmological abundance that goes beyond the approximations widely used in the literature on the topic and demonstrate how it affects the bounds on axion couplings on the example of axion interactions with leptons.
2024-11-28 (Czwartek)
Zapraszamy na spotkanie o godzinie 12:15  Calendar icon
Pedro Schwaller (University of Mainz)

Gravitational wave probes of dark sectors

Gravitational waves offer a new window into the early and dark universe. I will review sources of gravitational waves that can be searched for with current and future GW experiments, discuss interpretations of the recent observation of a stochastic GW background with PTAs, and explore new ideas for GW searches at utra-high frequencies using microwave cavities.
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2024-11-21 (Czwartek)
Zapraszamy na spotkanie o godzinie 12:15  Calendar icon
Kai Schmitz (Münster U.)

Gravitational waves from low-scale cosmic strings

(on-line)

Cosmic strings are a common prediction in many grand unified theories and a promising source of stochastic gravitational waves (GWs) from the early Universe. If strings are produced at a comparatively low energy scale, v ≲ 10^9 GeV, their GW signal exhibits, as I will discuss in this talk, several novel features that are not present in the case of high-scale cosmic strings, including: (i) a sharp cutoff frequency f_cut in the GW spectrum from the fundamental oscillation mode on closed string loops and (ii) an oscillating pattern in the total GW spectrum from all oscillation modes whose local minima are located at integer multiples of f_cut. I will explain the physical origin of these features and illustrate how they can be leveraged to directly probe the discrete spectrum of oscillation modes on closed string loops with future GW observatories such as BBO and DECIGO.
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2024-11-14 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Anish Ghoshal (IFT UW)

Cancelled

2024-11-07 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Michał Ryczkowski (IFT UW & Padua U.)

Theoretical constraints on models with vector-like fermions

In this talk, based on our recent work (Phys. Rev. D 110 (2024) 7, 075029, [2406.16050]), we explore theoretical constraints on models in which the Standard Model field content is extended by vector-like fermions and, in some cases, a real scalar singlet. Our approach focuses on the requirements of electroweak vacuum stability, perturbativity of model couplings, and gauge coupling unification, utilizing renormalization group equations. We show that a careful analysis of these factors leads to stringent constraints on the parameter space of the considered models. This, in turn, has significant implications for phenomenology, as we illustrate through examples of the double Higgs boson production, electroweak precision observables, and the electroweak phase transition.
2024-10-31 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
André Sopczak (IEAP CTU in Prague)

ATLAS forward proton detectors: status, performance and physics results

A key focus of the physics program at the LHC is the study of head-on proton-proton collisions. However, an important class of physics can be studied for cases where the protons narrowly miss one another and remain intact. In such cases, the electromagnetic fields surrounding the protons can interact producing high-energy photon-photon collisions. Alternatively, interactions mediated by the strong force can also result in intact forward scattered protons, providing probes of quantum chromodynamics (QCD). In order to aid identification and provide unique information about these rare interactions, instrumentation to detect and measure protons scattered through very small angles is installed in the beam pipe far downstream of the interaction point. We describe the ATLAS Forward Proton “Roman Pot” detectors (AFP and ALFA), their performance of Tracking and Time-of-Flight detectors. Results from ATLAS and AFP/ALFA photoproduction in proton-proton and heavy ion collisions are reviewed.
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