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Wydział Fizyki UW > Badania > Seminaria i konwersatoria > Seminarium Kosmologia i Fizyka Cząstek

Seminarium Kosmologia i Fizyka Cząstek

2006/2007 | 2007/2008 | 2008/2009 | 2009/2010 | 2010/2011 | 2011/2012 | 2012/2013 | 2013/2014 | 2014/2015 | 2015/2016 | 2016/2017

2011-01-18 (Wtorek)
Zapraszamy do Sali Dużej Teoretycznej (229), ul. Hoża 69 o godzinie 13:15  Calendar icon
Aleksandra Piórkowska (IF UŚ)

The impact of cosmological model on testing theories of fundamental interactions

2011-01-11 (Wtorek)
Zapraszamy do Sali Dużej Teoretycznej (229), ul. Hoża 69 o godzinie 13:15  Calendar icon
Luis Alvarez-Gaume (CERN TH)

Further thoughts on Supersymmetry and Inflation: An update

2010-12-21 (Wtorek)
Zapraszamy do Sali Dużej Teoretycznej (229), ul. Hoża 69 o godzinie 13:15  Calendar icon
Mariusz Dąbrowski (Uniwersytet Szczeciński)

Własności i klasyfikacja egzotycznych osobliwości w kosmologii

2010-12-07 (Wtorek)
Zapraszamy do Sali Dużej Teoretycznej (229), ul. Hoża 69 o godzinie 13:15  Calendar icon
Alexander Belyaev (U. of Southampton)

Distinguishing Z' Physics with early LHC data

What is a Z' Physics and why it can be appealing at the LHC now?This is the subject of this talk where LHC potential to test anddistinguish some promising models with spin-1 Z' bosons isdiscussed. If a Z' is discovered then measurement of the mass andcross-section will provide a powerful discriminator between thebenchmark models. This discrimination can be further improved byZ' width measurement. Comparison between Tevatron and LHCpotentials to test Z' models is performed.http://arxiv.org/pdf/1010.6058
2010-11-30 (Wtorek)
Zapraszamy do Sali Dużej Teoretycznej (229), ul. Hoża 69 o godzinie 13:15  Calendar icon
Stephan Huber (U. of Sussex)

The electroweak phase transition and baryogenesis in the Two Higgs doublet model

2010-11-23 (Wtorek)
Zapraszamy do Sali Dużej Teoretycznej (229), ul. Hoża 69 o godzinie 13:15  Calendar icon
Jakub Mielczarek (OA UJ)

Loop quantum cosmology and the CMB observations

We present a possible way of indirect probing of thePlanck scale effects by the cosmological observations.Our considerations base on loop quantum cosmology (LQC) which is the symmetry reduced model of loop quantum gravity. We show how the standard phase of cosmic inflation is naturally realized within LQC. We consider generation of gravitational waves in this model. Based on this, we present the way to relate LQC effects with observations of the cosmic microwave background radiation (CMB). In particular, we investigate the possible LQC effects on the B-type polarization of the CMB. We confront the theoretical predictions with the available observational data and indicate the possible constraints on the Planck scale physics. We discuss perspectives and limitations of the proposed approach.
2010-11-16 (Wtorek)
Zapraszamy do Sali Dużej Teoretycznej (229), ul. Hoża 69 o godzinie 13:15  Calendar icon
Piotr Korcyl (UJ)

Supersymmetric Yang-Mills quantum mechanics and their Witten index

A class of supersymmetric quantum systems called supersymmetric Yang-Mills quantum mechanics will be presented. After a brief description of their relevance to theoretical physics, emphasis will be put on a subset of these models, namely the D=2 models with a general SU(N) gauge symmetry. The derivation of their spectra and eigenstates using the cut Fock base approach will be discussed. The evaluation of their Witten index will be presented as well.
2010-10-26 (Wtorek)
Zapraszamy do Sali Dużej Teoretycznej (229), ul. Hoża 69 o godzinie 13:15  Calendar icon
Michał Artymowski (IFT UW)

Cosmology and Loop Quantum Cosmology with vector fields

2010-10-12 (Wtorek)
Zapraszamy do Sali Dużej Teoretycznej (229), ul. Hoża 69 o godzinie 13:15  Calendar icon
Dorota Sokołowska (IFT UW)

Cosmological evolution towards the present Inert Phase in 2HDM

2010-10-05 (Wtorek)
Zapraszamy do Sali Dużej Teoretycznej (229), ul. Hoża 69 o godzinie 13:15  Calendar icon
Jan Sobczyk (IFT UWr)

Neutrino Interactions in 1 GeV Energy Region

All the current and planned neutrino osillation experiments use/will use fluxes of neutrinos of energies of the order of 1 GeV. Precise measurements of oscillation parameters require better knowledge of neutrino interactions in this energy region. There is a lot of both experimental and theoretical activity in the field and the purpose of the seminar is to present a review of this activity.
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