Format results
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PSI 2017/2018 - Cosmology - Lecture 1
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 2
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 3
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 4
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 5
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 6
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 7
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 8
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 9
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 10
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 11
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 12
David Kubiznak - Charles University
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PSI 2017/2018 - Cosmology - Lecture 1
David Kubiznak - Charles University
Why to study cosmology? Some observational facts, Maximally symmetric spaces -
PSI 2017/2018 - Cosmology - Lecture 2
David Kubiznak - Charles University
FRW spacetime: coordinate systems, Hubble drag, cosmological redshift -
PSI 2017/2018 - Cosmology - Lecture 3
David Kubiznak - Charles University
FRW spacetime: horizons, Friedmann equations, cosmological inventory -
PSI 2017/2018 - Cosmology - Lecture 4
David Kubiznak - Charles University
FRW spacetime: dynamics of scale factor, local thermal equilibrium -
PSI 2017/2018 - Cosmology - Lecture 5
David Kubiznak - Charles University
Thermodynamics in expanding Universe: adiabatic expansion, freeze out, brief thermal history -
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PSI 2017/2018 - Cosmology - Lecture 8
David Kubiznak - Charles University
Dark matter candidates, Evidence for dark energy: supernovae Ia observations -
PSI 2017/2018 - Cosmology - Lecture 9
David Kubiznak - Charles University
Cosmological constant problems, Inflation paradigm, 3 puzzles -
PSI 2017/2018 - Cosmology - Lecture 10
David Kubiznak - Charles University
Physics of inflation: single field slow roll inflation -
PSI 2017/2018 - Cosmology - Lecture 11
David Kubiznak - Charles University
CMB again: ensemble of Universes, cosmic variance, E- and B-modes -
PSI 2017/2018 - Cosmology - Lecture 12
David Kubiznak - Charles University
BICEP 2, Inflation as a generator of perturbations, Time dependent harmonic oscillator