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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 | 2025/2026

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2026-05-28 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Andrzej Hryczuk (NCBJ)

Making Dark Matter Cool Again: dynamics of self-interacting dark sectors

Dark sectors generically contain particles with self-interactions, e.g. non-Abelian gauge fields or scalar fields not protected by any symmetry. In various models, these play crucial roles: either as mediators to the visible sector or the dark matter itself. The production dynamics of self-interacting, so-called cannibal states will be the focus of the talk. In particular, I will discuss the impact of solving the full system of coupled Boltzmann equations for the number densities and temperatures of all involved states, and describe three simple but phenomenologically rich scenarios. Finally, I will present a new mechanism for making dark matter cool again — how self-interactions can alleviate the Lyman-alpha limits, allowing for lighter DM states than usually expected.
2026-05-21 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Adam Gomułka (IFT UW)

Improved cosmological constraints on axion-lepton interactions

Axions appearing in extensions of the Standard Model can be produced thermally in the early universe through their couplings to leptons, leaving imprints on cosmological observables. Most existing analyses rely on the ΔN_eff approximation, which assumes ultra-relativistic axions and breaks down for axion masses above ~0.1 eV. I will present new model-independent constraints on both lepton-flavour-conserving and lepton-flavour-violating axion-lepton couplings, derived from Planck 2018 CMB and DESI DR2 BAO data, using the full phase-space Boltzmann equation for thermal axion production and including finite axion mass effects. The resulting bounds are significantly stronger than those from ΔN_eff across the mass range from 0.1 eV to 1 keV, with the most dramatic improvement for couplings involving the tau lepton, where our cosmological bounds surpass the most recent Belle-II limits on τ → ℓa decays. The results have direct implications for the QCD axion.
2026-05-14 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Mikołaj Marcinkowski (IFT UW)

A kinetically non-canonical scalar quantum field theory in cosmology

Typical field theories feature a kinetic term quadratic in field derivatives, like (∂φ)². Introducing a kinetic term that is a nonlinear function of (∂φ)² does not violate Lorentz covariance of the action (and in the case of gauge theories inherits their gauge invariance), making it a viable case to study. Such models were already investigated, for example k-inflation models by Armendáriz-Picón and Mukhanov. I describe some general properties of kinetically non-canonical theories, including challenges in quantizing them to make a quantum field theory (to my knowledge still an open problem). I focus on a scalar theory with a Dirac-Born-Infeld style kinetic term and analyse its behaviour in the early universe (during and after Inflation). I simulate the self-production of the particles of this field, with the intention of proposing them as a dark matter candidate.
2026-05-07 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Andrzej Wereszczyński (IFT UJ)

Dynamics of vortices: role of internal modes and false vacuum

I will show that dynamics of vortices (strings) is extremely sensitive to (1) existence of internal modes and (2) existence of a false point-like vacuum. The excitation of the modes is responsible for a complete breakdown of the geodesic dynamics  leading e.g., to chaotic, fractal-like pattern in scatterings of local vortices. The false vacuum radically changes the global vortex-antivortex annihilation. Specifically, despite the flat direction, it leads to appearance of very long-lived oscillons. This may change the abundance of axions if higher order operators are included.
2026-04-30 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Andrzej Czarnecki (University of Alberta)

Radiative effects in bound states

I will discuss two examples of determinations of bound-state properties. First, a rare decay of positronium: in QED, its spin-0 state annihilates only into an even number of photons, and spin-1 into an odd number. I will show how these rules are broken by weak interactions. Next, modifications of the muon decay by binding in an atom will be presented. This is of current interest because of experiments COMET (J-PARC, Japan) and Mu2e (Fermilab, USA) that will use muonic aluminium to search for the lepton-flavor violating process in which muon is converted into an electron. In both cases disagreements with previously published results will be pointed out and explained.
2026-04-23 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Kay Schönwald (CERN)

Precise predictions for gluon fusion induced ZH production at the LHC

The associated production of a Higgs boson with a vector boson, W or Z, provides the third-largest cross section for Higgs boson production at the LHC. Furthermore, it is an important process for the measurement of the Higgs coupling to bottom quarks, which is difficult in other Higgs production processes due to large backgrounds. The process of ZH production receives contributions from a gluon-initiated subprocess, which formally enters at higher orders in QCD, but is enhanced due to the large gluon luminosity at a hadron collider.  In this talk, I will present recent calculations for the 2-loop virtual amplitudes for this process valid in general kinematics, as well as the calculation of the associated 3-loop virtual amplitudes in the large top mass expansion. Afterwards, I present the public C++ library ggxy, where these corrections are implemented and which allows to freely modify all input parameters, such as the top-quark mass and its renormalization scheme and the masses of the external Z and Higgs bosons.  In addition, ggxy has been interfaced to Powheg and Herwig, which allows the matching to parton showers.
2026-04-16 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Ignacy Nałęcz (IFT UW)

From Hydrodynamics to Bubble Wall Velocity

Cosmological scalar phase transitions are ubiquitous in particle physics models. If they are first-order, they can be tested with gravitational-wave signal and baryon asymmetry they produce. These however, crucially depend on the velocity that nucleated new-phase bubbles reached. In my talk I will present generalized description which builds a bridge between numerical simulations, often use within the community, and the analytical estimates of this parameter. Our method allows one to determine the wall velocity without the necessity of performing full real-time simulations. Moreover, I will explain why some stationary solutions discussed in the literature are not dynamically realized, and provide a selection rule determining their fate.
2026-04-09 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Piotr Chankowski (IFT UW)

Effective quantum field theory approach to the ferromagnetic phase transition in a gas of fermions

I will summarize our recent effective quantum field theory computations of the free energy of a gas of spin-1/2 fermions interacting through a short-range spin-independent repulsive potential. The result is used to study the impact that higher-order corrections can have on the characteristics of a phase transition to the ordered phase, namely on the emergence of itinerant ferromagnetism. I will also comment on the relation of our computations to experimental searches for the ferromagnetic transition in cold gases of fermionic atoms.
2026-03-26 (Czwartek)
Zapraszamy na spotkanie o godzinie 12:15  Calendar icon
Zahra Tabrizi (University of Pittsburgh)

[ON-LINE] Neutrino-Collider Synergy for Beyond the Standard Model Searches

Neutrinos were discovered more than 60 years ago, yet they are the most mysterious particles of the Standard Model (SM) of particle physics. In order to further explore the neutrino sector, next-generation, long-baseline neutrino oscillation experiments are being built, including the DUNE and Hyper-K experiments. Given the intense neutrino beam, the massive fardetector, and the envisaged scale of the near detector, these experiments will certainly offer a rich physics program.  In this seminar I aim to explain how we can search for physics beyond the Standard Model (BSM) at neutrino experiments and unify neutrino and collider information in new physics searches within single, quantitative frameworks. I will first give a general introduction on the current status of neutrino physics. Then I will discuss how we can search for new particles and/or interactions at neutrino experiments with the goal of combining the results with the ones of colliders. I will explain how this can be done via two complementary approaches, 1) Direct search of dark sectors, where I will use these experiments for searches of specific new particles, including light dark matter or axion-like particles, etc; 2) Indirect search of new physics, where I will demonstrate how to use the systematic framework of Effective Field Theory at neutrino experiments, where the results can be combined with the results of other low or high energy experiments, such as the LHC. Finally, I will discuss future collider prospects, such as neutrino physics at a muon collider.
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2026-03-19 (Czwartek)
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 12:15  Calendar icon
Patrick Foldenauer (IFT-UAM CSIC, Madrid)

Testing New Physics with Neutrinos at Dark Matter experiments

In this talk, I will present a new avenue of how to test new physics with neutrinos - the observation of (solar) neutrino scattering in dark matter direct detection experiments.  It will be the first time coherent elastic neutrino-nucleus scattering (CEvNS) will be detected from astrophysical neutrinos, as opposed to reactors or spallation sources. Simultaneously, it will provide a complementary measurement of solar neutrinos via elastic neutrino-electron scattering. I will review the implications of this novel signal both for neutrino physics within and beyond the Standard Model. In this context, I will also discuss the prospects of observing solar neutrino scattering with RES-NOVA, a novel cryogenic bolometer experiment designed to observe CEvNS of astrophysical neutrino sources.
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