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Common Trends in Cosmology and Particle Physics
is an Eötvös Graduate Course and Workshop in Physics.
The lecture series covered the latest developments at the interface of
particle physics and cosmology and the most important astrophysical projects
exploring the evolution of the Universe. The course consisted of a
a four-day lecture series followed by a two-day workshop,
open to doctoral students and young postdoctoral
fellows. During the workshop, the participants had the
opportunity to present their contributions.
Organising Committee:
Zsolt Frei (Eötvös University Budapest)
Wolfgang Kummer (TU Wien)
András Patkós (Eötvös University Budapest)
Dominik J. Schwarz (CERN)
Sponsored by Aktion Österreich-Ungarn, the Hungarian
Academy of Sciences, the Hungarian Research Fund (OTKA) and the
Doctoral School of Eötvös University.
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Monday, 23 June 2003
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09:00
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Particle Physics I
(50')
transparencies
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Csaba Csáki (Cornell University, USA)
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10:10
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Cosmology with the Cosmic Microwave Background I
(50')
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Pedro G. Ferreira (Oxford University, UK)
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11:10
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CDM Simulations and the Formation of Galaxies I
(50')
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Guinevere Kauffmann (MPA Garching, Germany)
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16:00
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17:10
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Cosmology with the Cosmic Microwave Background II
(50')
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Pedro G. Ferreira
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18:10
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CDM Simulations and the Formation of Galaxies II
(50')
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Guinevere Kauffmann
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Tuesday, 24 June 2003
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09:00
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10:10
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Cosmology with the Cosmic Microwave Background III
(50')
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Pedro G. Ferreira
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11:10
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Cosmological Perturbations I
(50')
proceedings
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Robert Brandenberger (Brown University, USA)
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16:00
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CDM Simulations and the Formation of Galaxies III
(50')
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Guinevere Kauffmann
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17:10
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Cosmological Perturbations II
(50')
proceedings
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Robert Brandenberger
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18:10
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Large Scale Structure I
(50')
transparencies
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Alex Szalay (Johns Hopkins University, USA & Eötvös University, Hungary)
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Wednesday, 25 June 2003
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09:00
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Cosmological Perturbations III
(50')
proceedings
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Robert Brandenberger
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10:00
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11:10
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12:10
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Cosmological Inflation I
(50')
transparencies
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Igor Tkachev (CERN, Switzerland)
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Thursday, 26 June 2003
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09:00
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10:10
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Dark Energy I
(50')
transparencies
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Luca Amendola (Rome University, Italy)
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11:10
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16:00
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17:10
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18:10
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Friday, 27 June 2003
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09:00
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Galaxy Clusters I
(50')
transparencies
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Sabine Schindler (Innsbruck University, Austria)
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10:10
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11:10
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George Marx Memorial Lecture
(50')
transparencies
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Subir Sarkar (Oxford University, UK)
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16:00
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Back Reaction of Cosmological Perturbations
(30')
proceedings
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Robert Brandenberger (Brown University, USA)
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16:30
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Backreaction Problem for Pure de Sitter
(20')
transparencies
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Bojan Losic (University of British Columbia, Canada)
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16:50
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Cosmological Perturbation Theory and Wave Mechanics
(30')
transparencies
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István Szapudi (University of Hawaii, USA)
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17:40
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The CDM Power Spectrum on Smallest Scales
(20')
transparencies
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Stefan Hofmann (Stockholm University, Sweden)
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18:00
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Three-Point-Correlation Function for the SDSS-EDR
(20')
transparencies
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Christian Maulbetsch (Astrophysikalisches Institut Potsdam, Germany)
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18:20
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Bosonic D-Branes at Finite Temperature in TFD Approach
(20')
proceedings
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Ion Vancea (University of Sao Paulo, Brazil)
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18:40
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Gravitational Radiation Reaction in Compact Binary Systems
(20')
transparencies
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Zoltán Keresztes (University of Szeged, Hungary)
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Saturday, 28 June 2003
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09:00
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Results From the Mainz Neutrino Mass Experiment
(20')
transparencies
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Christine Kraus (University of Mainz, Germany)
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09:20
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Recent Progress in QCD at High Temperature
(30')
transparencies
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Anton Rebhan (TU Wien, Austria)
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09:50
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HTL Quasiparticle Models of Deconfined QCD at Finite Chemical Potential
(20')
transparencies
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Paul Romatschke (TU Wien, Austria)
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10:30
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Non-equilibrium Dynamics of Phi**4 Theory in the 2PPI Formalism
(20')
transparencies
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Andreas Heinen (University of Dortmund, Germany)
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10:50
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Thermalisation of Quantum Fields
(20')
transparencies
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Szabolcs Borsányi (Eötvös University, Hungary)
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11:10
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Phase Transition of a Scalar Field Theory in the Early Universe
(20')
transparencies
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Andreas Ipp (TU Wien, Austria)
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11:30
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The First Nonlinear Structures and the Reionization History of the Universe: Implications of the recent WMAP Results
(30')
transparencies
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Zoltán Haiman (Columbia University, USA)
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