Description |
The purpose of the School is to provide an introduction to the current state of research in cosmology and astroparticle physics. It is intended for beginning graduate students, as well as more senior non-expert researchers that are interested in these fields. Each course will be 3-4 days long, with lectures during the day and a tutorial session at the end of the day. More specialized seminars will also be scheduled. LECTURERS and TOPICS include: * Tom Abel (Stanford) - The dark ages * Alessandra Buonanno (Maryland) - Gravitational waves * Sean Carroll (Chicago) - Introduction to cosmology and dark energy * Andrea Ferrara (SISSA) - First light in the universe * Ariel Goodbar (Stockholm) - Observational cosmology * Renata Kallosh (Stanford) - String cosmology * Andrei Linde (Stanford) - Inflation * Ue-Li Pen (CITA) - Large scale structure in the universe * Antonio Riotto (Padova) - Early universe * Bernard Sadoulet (Berkeley) - Experimental astroparticle physics and dark matter searches * Max Tegmark (MIT) - Cosmic microwave background * Alexander Vilenkin (Tufts) - Topological defects |
Summer School in Cosmology and Astroparticle Physics (10-21 July) andWorkshop on Nongaussianity in Cosmology (24-28 July) | (smr 1761)
Go to day
-
-
09:30 - 09:45
Opening Address
Location: Main Building Main Lecture Hall -
09:30
Opening Address
15'
Speaker: U. Seljak (ICTP)
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09:30
Opening Address
15'
-
09:45 - 11:00
Formation of Large Scale Structure: Overview and Linear Theory - Lecture 1
Location: Main Building Lobby -
09:45
Formation of Large Scale Structure: Overview and Linear Theory - Lecture 1
1h15'
Speaker: U. Pen (University of Toronto, Canada)
-
09:45
Formation of Large Scale Structure: Overview and Linear Theory - Lecture 1
1h15'
-
11:15 - 12:30
Strategies for Dark Matter Detection - Lecture 1
Location: Main Building Lobby -
11:15
Strategies for Dark Matter Detection - Lecture 1
1h15'
Speaker: B. Sadoulet (University of California, USA) Material: lecture notes
-
11:15
Strategies for Dark Matter Detection - Lecture 1
1h15'
-
12:30 - 14:00
Lunch Break
Location: Main Building Lobby - 12:30 Lunch Break 1h30'
-
14:00 - 15:15
Introduction to Cosmology and the Early Universe - Lecture 1
Location: Main Building Lobby -
14:00
Introduction to Cosmology and the Early Universe - Lecture 1
1h15'
Speaker: S. Carroll (University of Chicago, USA) Material: lecture notes
-
14:00
Introduction to Cosmology and the Early Universe - Lecture 1
1h15'
-
15:30 - 16:45
Anthropic selection and the Landscape - Lecture 1
Location: Main Building Lobby -
15:30
Anthropic selection and the Landscape - Lecture 1
1h15'
Speaker: A. Vilenkin (Tufts University, USA)
-
15:30
Anthropic selection and the Landscape - Lecture 1
1h15'
-
09:30 - 09:45
Opening Address
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-
08:30 - 09:45
Anthropic selection and the Landscape - Lecture 2
-
08:30
Anthropic selection and the Landscape - Lecture 2
1h15'
Speaker: A. Vilenkin
-
08:30
Anthropic selection and the Landscape - Lecture 2
1h15'
-
10:00 - 11:15
Strategies for Dark Matter Detection - Lecture 2
-
10:00
Strategies for Dark Matter Detection - Lecture 2
1h15'
Speaker: B. Sadoulet Material: lecture notes
-
10:00
Strategies for Dark Matter Detection - Lecture 2
1h15'
-
11:30 - 12:45
Gravitational Waves: Theory, Sources and Detectability - Lecture 1
-
11:30
Gravitational Waves: Theory, Sources and Detectability - Lecture 1
1h15'
Speaker: A. Buonanno (University of Maryland, USA) Material: lecture notes
-
11:30
Gravitational Waves: Theory, Sources and Detectability - Lecture 1
1h15'
-
12:45 - 14:00
Lunch Break
- 12:45 Lunch Break 1h15'
-
14:00 - 15:15
Large Scale Structure: Non-Linear regime, simulations - Lecture 2
-
14:00
Large Scale Structure: Non-Linear regime, simulations - Lecture 2
1h15'
Speaker: U. Pen
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14:00
Large Scale Structure: Non-Linear regime, simulations - Lecture 2
1h15'
-
15:30 - 16:45
The First Stars: Overview - Lecture 1
-
15:30
The First Stars: Overview - Lecture 1
1h15'
Speaker: T. Abel (Kavli Institute for Astro-Particle Physics, USA)
-
15:30
The First Stars: Overview - Lecture 1
1h15'
-
17:45 - 17:45
RECEPTION
Location: Main Building Terrace - 17:45 RECEPTION
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08:30 - 09:45
Anthropic selection and the Landscape - Lecture 2
-
-
08:30 - 09:45
Strategies for Dark Matter Detection - Lecture 3
Location: Main Building Main Lecture Hall -
08:30
Strategies for Dark Matter Detection - Lecture 3
1h15'
Speaker: B. Sadoulet Material: lecture notes
-
08:30
Strategies for Dark Matter Detection - Lecture 3
1h15'
-
10:00 - 11:15
Gravitational Waves: Theory, Sources and Detectability - Lecture 2
Location: Main Building Main Lecture Hall -
10:00
Gravitational Waves: Theory, Sources and Detectability - Lecture 2
1h15'
Speaker: A. Buonanno Material: lecture notes
-
10:00
Gravitational Waves: Theory, Sources and Detectability - Lecture 2
1h15'
-
11:30 - 12:45
The First Stars: Primordial Gas - Lecture 2
Location: Main Building Main Lecture Hall -
11:30
The First Stars: Primordial Gas - Lecture 2
1h15'
Speaker: T. Abel
-
11:30
The First Stars: Primordial Gas - Lecture 2
1h15'
-
12:45 - 14:00
Lunch Break
Location: Main Building Main Lecture Hall - 12:45 Lunch Break 1h15'
-
14:00 - 15:15
Introduction to Cosmology and the Early Universe - Lecture 2
Location: Main Building Main Lecture Hall -
14:00
Introduction to Cosmology and the Early Universe - Lecture 2
1h15'
Speaker: S. Carroll
-
14:00
Introduction to Cosmology and the Early Universe - Lecture 2
1h15'
-
15:30 - 16:45
DISCUSSION SESSION
Location: Main Building Main Lecture Hall -
15:30
DISCUSSION SESSION
1h15'
-
15:30
DISCUSSION SESSION
1h15'
-
08:30 - 09:45
Strategies for Dark Matter Detection - Lecture 3
-
-
08:30 - 09:45
Gravitational Waves: Theory, Sources and Detectability - Lecture 3
-
08:30
Gravitational Waves: Theory, Sources and Detectability - Lecture 3
1h15'
Speaker: A. Buonanno Material: lecture notes
-
08:30
Gravitational Waves: Theory, Sources and Detectability - Lecture 3
1h15'
-
10:00 - 11:15
Strategies for Dark Matter Detection - Lecture 4
-
10:00
Strategies for Dark Matter Detection - Lecture 4
1h15'
Speaker: B. Sadoulet Material: lecture notes
-
10:00
Strategies for Dark Matter Detection - Lecture 4
1h15'
-
11:30 - 12:45
The First Stars: Radiative Transfer - Lecture 3
-
11:30
The First Stars: Radiative Transfer - Lecture 3
1h15'
Speaker: T. Abel
-
11:30
The First Stars: Radiative Transfer - Lecture 3
1h15'
-
12:45 - 14:00
Lunch Break
- 12:45 Lunch Break 1h15'
-
14:00 - 15:15
Introduction to Cosmology and the Early Universe - Lecture 3
-
14:00
Introduction to Cosmology and the Early Universe - Lecture 3
1h15'
Speaker: S. Carroll
-
14:00
Introduction to Cosmology and the Early Universe - Lecture 3
1h15'
-
15:30 - 16:45
The Cosmic Baryon Budget: distribution of Baryons - Lecture 3
-
15:30
The Cosmic Baryon Budget: distribution of Baryons - Lecture 3
1h15'
Speaker: U. Pen
-
15:30
The Cosmic Baryon Budget: distribution of Baryons - Lecture 3
1h15'
-
08:30 - 09:45
Gravitational Waves: Theory, Sources and Detectability - Lecture 3
-
-
08:30 - 09:45
The First Stars: Open Questions - Lecture 4
-
08:30
The First Stars: Open Questions - Lecture 4
1h15'
Speaker: T. Abel
-
08:30
The First Stars: Open Questions - Lecture 4
1h15'
-
10:00 - 11:15
Gravitational Waves: Theory, Sources and Detectability - Lecture 4
-
10:00
Gravitational Waves: Theory, Sources and Detectability - Lecture 4
1h15'
Speaker: A. Buonanno
-
10:00
Gravitational Waves: Theory, Sources and Detectability - Lecture 4
1h15'
-
11:30 - 12:45
Introduction to Cosmology and the Early Universe - Lecture 4
-
11:30
Introduction to Cosmology and the Early Universe - Lecture 4
1h15'
Speaker: S. Carroll
-
11:30
Introduction to Cosmology and the Early Universe - Lecture 4
1h15'
-
12:45 - 14:00
Lunch Break
- 12:45 Lunch Break 1h15'
-
14:00 - 15:15
Mapping of dark matter and dark baryons: lensing and CMB secondaries - Lecture 4
-
14:00
Mapping of dark matter and dark baryons: lensing and CMB secondaries - Lecture 4
1h15'
Speaker: U. Pen
-
14:00
Mapping of dark matter and dark baryons: lensing and CMB secondaries - Lecture 4
1h15'
-
15:30 - 16:45
DISCUSSION SESSION
-
15:30
DISCUSSION SESSION
1h15'
-
15:30
DISCUSSION SESSION
1h15'
-
08:30 - 09:45
The First Stars: Open Questions - Lecture 4
-
-
08:30 - 09:45
Observational cosmology: distant supernovae and dark energy - Lecture 1
-
08:30
Observational cosmology: distant supernovae and dark energy - Lecture 1
1h15'
Speaker: A. Goobar (University of Stockholm, Sweden)
-
08:30
Observational cosmology: distant supernovae and dark energy - Lecture 1
1h15'
-
10:00 - 11:15
String Cosmology - Lecture 1
-
10:00
String Cosmology - Lecture 1
1h15'
Speaker: R. Kallosh (Stanford University, USA) Material: lecture notes
-
10:00
String Cosmology - Lecture 1
1h15'
-
11:30 - 12:45
Cosmological Feedbacks from the First Stars - Lecture 1
-
11:30
Cosmological Feedbacks from the First Stars - Lecture 1
1h15'
Speaker: A. Ferrara (SISSA, Trieste) Material: lecture notes
-
11:30
Cosmological Feedbacks from the First Stars - Lecture 1
1h15'
-
12:45 - 14:00
Lunch Break
- 12:45 Lunch Break 1h15'
-
14:00 - 15:15
Cosmological Feedbacks from the First Stars - Lecture 2
-
14:00
Cosmological Feedbacks from the First Stars - Lecture 2
1h15'
Speaker: A. Ferrara
-
14:00
Cosmological Feedbacks from the First Stars - Lecture 2
1h15'
-
15:30 - 16:45
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 1
-
15:30
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 1
1h15'
Speaker: A. Riotto (INFN, Sezione di Padova, Italy)
-
15:30
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 1
1h15'
-
08:30 - 09:45
Observational cosmology: distant supernovae and dark energy - Lecture 1
-
-
08:30 - 09:45
Observational cosmology: distant supernovae and dark energy - Lecture 2
-
08:30
Observational cosmology: distant supernovae and dark energy - Lecture 2
1h15'
Speaker: A. Goobar
-
08:30
Observational cosmology: distant supernovae and dark energy - Lecture 2
1h15'
-
10:00 - 11:15
String Cosmology - Lecture 2
-
10:00
String Cosmology - Lecture 2
1h15'
Speaker: R. Kallosh Material: lecture notes
-
10:00
String Cosmology - Lecture 2
1h15'
-
11:30 - 12:45
Inflation - Lecture 1
-
11:30
Inflation - Lecture 1
1h15'
Speaker: A. Linde (Stanford University, USA) Material: lecture notes
-
11:30
Inflation - Lecture 1
1h15'
-
12:45 - 14:00
Lunch Break
- 12:45 Lunch Break 1h15'
-
14:00 - 15:15
Cosmological Feedbacks from the First Stars - Lecture 3
-
14:00
Cosmological Feedbacks from the First Stars - Lecture 3
1h15'
Speaker: A. Ferrara
-
14:00
Cosmological Feedbacks from the First Stars - Lecture 3
1h15'
-
15:30 - 16:45
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 2
-
15:30
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 2
1h15'
Speaker: A. Riotto
-
15:30
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 2
1h15'
-
08:30 - 09:45
Observational cosmology: distant supernovae and dark energy - Lecture 2
-
-
08:30 - 09:45
Observational cosmology: distant supernovae and dark energy - Lecture 3
-
08:30
Observational cosmology: distant supernovae and dark energy - Lecture 3
1h15'
Speaker: A. Goobar
-
08:30
Observational cosmology: distant supernovae and dark energy - Lecture 3
1h15'
-
10:00 - 11:15
String Cosmology - Lecture 3
-
10:00
String Cosmology - Lecture 3
1h15'
Speaker: R. Kallosh Material: lecture notes
-
10:00
String Cosmology - Lecture 3
1h15'
-
11:30 - 12:45
Inflation - Lecture 2
-
11:30
Inflation - Lecture 2
1h15'
Speaker: A. Linde
-
11:30
Inflation - Lecture 2
1h15'
-
12:45 - 14:00
Lunch Break
- 12:45 Lunch Break 1h15'
-
14:00 - 15:15
Cosmological Feedbacks from the First Stars - Lecture 4
-
14:00
Cosmological Feedbacks from the First Stars - Lecture 4
1h15'
Speaker: A. Ferrara
-
14:00
Cosmological Feedbacks from the First Stars - Lecture 4
1h15'
-
15:30 - 16:45
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 1
-
15:30
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 1
1h15'
Speaker: M. Tegmark (MIT, USA)
-
15:30
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 1
1h15'
-
08:30 - 09:45
Observational cosmology: distant supernovae and dark energy - Lecture 3
-
-
08:30 - 09:45
Inflation - Lecture 3
-
08:30
Inflation - Lecture 3
1h15'
Speaker: A. Linde
-
08:30
Inflation - Lecture 3
1h15'
-
10:00 - 11:15
Observational cosmology: distant supernovae and dark energy - Lecture 4
-
10:00
Observational cosmology: distant supernovae and dark energy - Lecture 4
1h15'
Speaker: A. Goobar
-
10:00
Observational cosmology: distant supernovae and dark energy - Lecture 4
1h15'
-
11:30 - 12:45
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 2
-
11:30
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 2
1h15'
Speaker: M. Tegmark
-
11:30
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 2
1h15'
-
12:45 - 14:00
Lunch Break
- 12:45 Lunch Break 1h15'
-
14:00 - 15:15
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 3
-
14:00
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 3
1h15'
Speaker: A. Riotto
-
14:00
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 3
1h15'
-
15:30 - 16:45
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 3
-
15:30
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 3
1h15'
Speaker: M. Tegmark
-
15:30
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 3
1h15'
-
08:30 - 09:45
Inflation - Lecture 3
-
-
08:30 - 09:45
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 4
-
08:30
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 4
1h15'
Speaker: M. Tegmark
-
08:30
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 4
1h15'
-
10:00 - 11:15
Inflation - Lecture 4
-
10:00
Inflation - Lecture 4
1h15'
Speaker: A. Linde
-
10:00
Inflation - Lecture 4
1h15'
-
11:30 - 12:45
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 4
-
11:30
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 4
1h15'
Speaker: A. Riotto
-
11:30
Inflation, Cosmological perturbations from inflation & baryon asymmetry - Lecture 4
1h15'
-
12:45 - 14:00
Lunch Break
- 12:45 Lunch Break 1h15'
-
14:00 - 15:15
String Cosmology - Lecture 4
-
14:00
String Cosmology - Lecture 4
1h15'
Speaker: R. Kallosh Material: lecture notes
-
14:00
String Cosmology - Lecture 4
1h15'
-
15:30 - 16:30
DISCUSSION SESSION & CLOSING REMARKS
-
15:30
DISCUSSION SESSION & CLOSING REMARKS
1h0'
-
15:30
DISCUSSION SESSION & CLOSING REMARKS
1h0'
-
08:30 - 09:45
Cosmic Conundrums: Dark Energy, Dark Matter & Inflation - Lecture 4
-
-
10:00 - 10:30
Setting the stage: Gaussian concordance cosmology and its parameters
Location: Adriatico Guest House (Lower Level 1) -
10:00
Setting the stage: Gaussian concordance cosmology and its parameters
30'
Speaker: Max Tegmark (MIT, USA)
-
10:00
Setting the stage: Gaussian concordance cosmology and its parameters
30'
-
10:30 - 11:30
Coffee Break
Location: Adriatico Guest House (Terrace) - 10:30 Coffee Break 1h0'
-
11:30 - 12:00
Testing Lorentz invariance violation through electromagnetic wave propagation in the universe
Location: Adriatico Guest House (Lower Level 1) -
11:30
Testing Lorentz invariance violation through electromagnetic wave propagation in the universe
30'
Speaker: Tina Kahniashvili (Abastunami Astrophysical Observatory, Georgia)
-
11:30
Testing Lorentz invariance violation through electromagnetic wave propagation in the universe
30'
-
12:00 - 12:30
Non-Gaussian anomalies in the WMAP
Location: Adriatico Guest House (Lower Level 1) -
12:00
Non-Gaussian anomalies in the WMAP
30'
Speaker: Joao Magueijo (Imperial College, UK)
-
12:00
Non-Gaussian anomalies in the WMAP
30'
-
12:30 - 14:30
Lunch Break
Location: Adriatico Guest House (Lower Level 1) - 12:30 Lunch Break 2h0'
-
14:30 - 15:00
Evil axes and evil foreground
Location: Adriatico Guest House (Lower Level 1) -
14:30
Evil axes and evil foreground
30'
Speaker: Angelica De Oliveira-Costa (MIT, USA)
-
14:30
Evil axes and evil foreground
30'
-
15:00 - 15:30
Mysteries on Universe's largest Observable Scales
Location: Adriatico Guest House (Lower Level 1) -
15:00
Mysteries on Universe's largest Observable Scales
30'
Speaker: Dragan Huterer (University of Chicago, USA)
-
15:00
Mysteries on Universe's largest Observable Scales
30'
-
15:30 - 16:00
Are non-Gaussianities responsible for excess small-scale anisotropy in the CMB?
Location: Adriatico Guest House (Lower Level 1) -
15:30
Are non-Gaussianities responsible for excess small-scale anisotropy in the CMB?
30'
Speaker: Asantha Cooray (University of California, USA)
-
15:30
Are non-Gaussianities responsible for excess small-scale anisotropy in the CMB?
30'
-
16:00 - 16:30
Statistical isotropy of CMB temperature and polarization
Location: Adriatico Guest House (Lower Level 1) -
16:00
Statistical isotropy of CMB temperature and polarization
30'
Speaker: Tarun Souradeep (IUCAA, Pune, India)
-
16:00
Statistical isotropy of CMB temperature and polarization
30'
-
10:00 - 10:30
Setting the stage: Gaussian concordance cosmology and its parameters
-
-
09:30 - 10:00
A non-Gaussian cold spot in the CMB sky
Location: Adriatico Guest House Kastler Lecture Hall -
09:30
A non-Gaussian cold spot in the CMB sky
30'
Speaker: Marcos Cruz (Universidad de Cantabria, Spain)
-
09:30
A non-Gaussian cold spot in the CMB sky
30'
-
10:00 - 10:30
Anomalous large-scale angular correlations in CMB maps
Location: Adriatico Guest House Kastler Lecture Hall -
10:00
Anomalous large-scale angular correlations in CMB maps
30'
Speaker: Armando Bernui (INPE, San Jose dos Campos, Brazil)
-
10:00
Anomalous large-scale angular correlations in CMB maps
30'
-
10:30 - 11:30
Coffee Break
Location: Adriatico Guest House (Terrace) - 10:30 Coffee Break 1h0'
-
11:30 - 12:00
Local voids as the origin of the large-angle CMB anomalies
Location: Adriatico Guest House Kastler Lecture Hall -
11:30
Local voids as the origin of the large-angle CMB anomalies
30'
Speaker: Kaiko Taro Inoue (Kinki University, Osaka, Japan)
-
11:30
Local voids as the origin of the large-angle CMB anomalies
30'
-
12:00 - 12:30
Non-standard Non-Gaussianity
Location: Adriatico Guest House Kastler Lecture Hall -
12:00
Non-standard Non-Gaussianity
30'
Speaker: Alejandro Gangui (IAFE, Buenos Aires, Argentina)
-
12:00
Non-standard Non-Gaussianity
30'
-
12:30 - 14:30
Lunch Break
Location: Adriatico Guest House Kastler Lecture Hall - 12:30 Lunch Break 2h0'
-
14:30 - 15:00
Non-Gaussian CMB maps from cosmic strings
Location: Adriatico Guest House Kastler Lecture Hall -
14:30
Non-Gaussian CMB maps from cosmic strings
30'
Speaker: Paul Shellard (D.A.M.T.P., Cambridge, UK)
-
14:30
Non-Gaussian CMB maps from cosmic strings
30'
-
15:00 - 15:30
Non-Gaussianities in two field inflation
Location: Adriatico Guest House Kastler Lecture Hall -
15:00
Non-Gaussianities in two field inflation
30'
Speaker: Filippo Vernizzi (University of Helsinki, Finland)
-
15:00
Non-Gaussianities in two field inflation
30'
-
15:30 - 16:00
Non-linear evolution of inhomogeneities during multi-field inflation
Location: Adriatico Guest House Kastler Lecture Hall -
15:30
Non-linear evolution of inhomogeneities during multi-field inflation
30'
Speaker: Gerasimos Rigopoulos (Utrecht University, Netherlands)
-
15:30
Non-linear evolution of inhomogeneities during multi-field inflation
30'
-
16:00 - 16:30
Non-Gaussianity in multiple-field inflation
Location: Adriatico Guest House Kastler Lecture Hall -
16:00
Non-Gaussianity in multiple-field inflation
30'
Speaker: Bartjan VanTent (D.A.M.T.P., Cambridge, UK)
-
16:00
Non-Gaussianity in multiple-field inflation
30'
-
18:30 - 20:30
RECEPTION
Location: Adriatico Guest House (Terrace) - 18:30 RECEPTION 2h0'
-
09:30 - 10:00
A non-Gaussian cold spot in the CMB sky
-
-
09:30 - 10:00
Relic Anisotropy as the source of all evil?
Location: Adriatico Guest House Kastler Lecture Hall -
09:30
Relic Anisotropy as the source of all evil?
30'
Speaker: Carlo Contaldi (Imperial College, London, UK)
-
09:30
Relic Anisotropy as the source of all evil?
30'
-
10:00 - 10:30
On the effective field theory approach to cosmological initial conditions
Location: Adriatico Guest House Kastler Lecture Hall -
10:00
On the effective field theory approach to cosmological initial conditions
30'
Speaker: Massimo Porrati (New York University, USA)
-
10:00
On the effective field theory approach to cosmological initial conditions
30'
-
10:30 - 11:30
Coffee Break
Location: Adriatico Guest House (Terrace) - 10:30 Coffee Break 1h0'
-
11:30 - 12:00
Right-handed neutrinos as the source of density perturbations
Location: Adriatico Guest House Kastler Lecture Hall -
11:30
Right-handed neutrinos as the source of density perturbations
30'
Speaker: Lotfi Boubekeur (ICTP)
-
11:30
Right-handed neutrinos as the source of density perturbations
30'
-
12:00 - 12:30
Nongaussianity from Tachyonic Preheating in Hybrid Inflation
Location: Adriatico Guest House Kastler Lecture Hall -
12:00
Nongaussianity from Tachyonic Preheating in Hybrid Inflation
30'
Speaker: Neil Barnaby (McGill University, Montreal, Canada)
-
12:00
Nongaussianity from Tachyonic Preheating in Hybrid Inflation
30'
-
12:30 - 13:00
Atacama Cosmology Telescope
Location: Adriatico Guest House Kastler Lecture Hall -
12:30
Atacama Cosmology Telescope
30'
Speaker: Raul Jimenez
-
12:30
Atacama Cosmology Telescope
30'
-
12:30 - 14:30
Lunch Break
Location: Adriatico Guest House Kastler Lecture Hall - 12:30 Lunch Break 2h0'
-
14:30 - 15:00
Second order gauge-invariant perturbations during inflation
Location: Adriatico Guest House Kastler Lecture Hall -
14:30
Second order gauge-invariant perturbations during inflation
30'
Speaker: Giovanni Marozzi (University of Bologna, Italy)
-
14:30
Second order gauge-invariant perturbations during inflation
30'
-
15:00 - 15:30
Colored noise induced low L moments and non-Gaussianity in cosmology
Location: Adriatico Guest House Kastler Lecture Hall -
15:00
Colored noise induced low L moments and non-Gaussianity in cosmology
30'
Speaker: Kin-Wang Ng (Academia Sinica, Taiwan, ROC)
-
15:00
Colored noise induced low L moments and non-Gaussianity in cosmology
30'
-
15:30 - 16:00
High order correction terms for the peak-peak correlation function in nearly-Gaussian models
Location: Adriatico Guest House Kastler Lecture Hall -
15:30
High order correction terms for the peak-peak correlation function in nearly-Gaussian models
30'
Speaker: Ana Paula Andrade (Univ. Estadual de Santa Cruz, Bahia, Brazil)
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15:30
High order correction terms for the peak-peak correlation function in nearly-Gaussian models
30'
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16:00 - 16:30
Non-Gaussian signatures in the large-scale power spectrum
Location: Adriatico Guest House Kastler Lecture Hall -
16:00
Non-Gaussian signatures in the large-scale power spectrum
30'
Speaker: Alex Szalay (The John Hopkins University, Baltimore, USA)
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16:00
Non-Gaussian signatures in the large-scale power spectrum
30'
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09:30 - 10:00
Relic Anisotropy as the source of all evil?
-
-
09:30 - 10:00
Testing primordial non-Gaussianity in CMB Anisotropies
Location: Adriatico Guest House Kastler Lecture Hall -
09:30
Testing primordial non-Gaussianity in CMB Anisotropies
30'
Speaker: Michele Liguori (University of Padova, Italy)
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09:30
Testing primordial non-Gaussianity in CMB Anisotropies
30'
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10:00 - 10:30
Non-Gaussianity detection and discrimination using several multiscale transforms
Location: Adriatico Guest House Kastler Lecture Hall -
10:00
Non-Gaussianity detection and discrimination using several multiscale transforms
30'
Speaker: Jean-Luc Starck (CEA, Gif-sur-Yvette, France)
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10:00
Non-Gaussianity detection and discrimination using several multiscale transforms
30'
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10:30 - 11:30
Coffee Break
Location: Adriatico Guest House (Terrace) - 10:30 Coffee Break 1h0'
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11:30 - 12:00
Efficiency of non-Gaussian estimators
Location: Adriatico Guest House Kastler Lecture Hall -
11:30
Efficiency of non-Gaussian estimators
30'
Speaker: Daniel Babich (Harvard University, Cambridge, USA)
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11:30
Efficiency of non-Gaussian estimators
30'
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12:00 - 12:30
Nongaussianity anomalies in WMAP
Location: Adriatico Guest House Kastler Lecture Hall -
12:00
Nongaussianity anomalies in WMAP
30'
Speaker: Olivier P. Dore (University of Toronto, Canada)
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12:00
Nongaussianity anomalies in WMAP
30'
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12:30 - 14:30
Lunch Break
Location: Adriatico Guest House Kastler Lecture Hall - 12:30 Lunch Break 2h0'
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14:30 - 15:00
New approaches for detecting non-Gaussianity in the CMB
Location: Adriatico Guest House Kastler Lecture Hall -
14:30
New approaches for detecting non-Gaussianity in the CMB
30'
Speaker: Kristofer Jennings (Purdue University, USA)
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14:30
New approaches for detecting non-Gaussianity in the CMB
30'
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15:00 - 15:30
Inflationary non-Gaussianity and the present Universe
Location: Adriatico Guest House Kastler Lecture Hall -
15:00
Inflationary non-Gaussianity and the present Universe
30'
Speaker: Sabino Matarrese (University of Padova, Italy)
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15:00
Inflationary non-Gaussianity and the present Universe
30'
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15:30 - 16:00
Nongaussianity from higher derivative interactions
Location: Adriatico Guest House Kastler Lecture Hall -
15:30
Nongaussianity from higher derivative interactions
30'
Speaker: Paolo Creminelli (ICTP)
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15:30
Nongaussianity from higher derivative interactions
30'
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16:00 - 16:30
Statistical reconstruction of non-Gaussian PDF's
Location: Adriatico Guest House Kastler Lecture Hall -
16:00
Statistical reconstruction of non-Gaussian PDF's
30'
Speaker: Ue-Li Pen (University of Toronto, Canada)
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16:00
Statistical reconstruction of non-Gaussian PDF's
30'
-
16:30 - 17:00
Statistical analysis of undetected point sources in cosmic microwave background maps
Location: Adriatico Guest House Kastler Lecture Hall -
16:30
Statistical analysis of undetected point sources in cosmic microwave background maps
30'
Speaker: Rita Belen Barreiro (Universidad de Cantabria, Spain)
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16:30
Statistical analysis of undetected point sources in cosmic microwave background maps
30'
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19:00 - 19:00
CONFERENCE DINNER
Location: Adriatico Guest House Kastler Lecture Hall - 19:00 CONFERENCE DINNER
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09:30 - 10:00
Testing primordial non-Gaussianity in CMB Anisotropies
-
-
09:30 - 10:00
Non-Gaussianity in the 21 cm background
Location: Adriatico Guest House Kastler Lecture Hall -
09:30
Non-Gaussianity in the 21 cm background
30'
Speaker: Annalisa Pillepich (ETH, Zurich, Switzerland)
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09:30
Non-Gaussianity in the 21 cm background
30'
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10:00 - 10:30
How optical imaging surveys can constrain cosmology
Location: Adriatico Guest House Kastler Lecture Hall -
10:00
How optical imaging surveys can constrain cosmology
30'
Speaker: Lloyd Knox (University of California at Davis, USA)
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10:00
How optical imaging surveys can constrain cosmology
30'
-
10:30 - 11:30
Coffee Break
Location: Adriatico Guest House (Terrace) - 10:30 Coffee Break 1h0'
-
11:30 - 12:00
Impact of primordial non-Gaussianity on dark energy constraints from clusters observations
Location: Adriatico Guest House Kastler Lecture Hall -
11:30
Impact of primordial non-Gaussianity on dark energy constraints from clusters observations
30'
Speaker: Emiliano Sefusatti (Fermilab, Batavia, USA)
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11:30
Impact of primordial non-Gaussianity on dark energy constraints from clusters observations
30'
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12:00 - 12:30
Newtonian correspondence and pure general relativistic correction terms from the relativistic non-linear cosmological perturbation theory
Location: Adriatico Guest House Kastler Lecture Hall -
12:00
Newtonian correspondence and pure general relativistic correction terms from the relativistic non-linear cosmological perturbation theory
30'
Speaker: Jai-Chan Hwang (Kyungpook National University, Taegu, ROC)
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12:00
Newtonian correspondence and pure general relativistic correction terms from the relativistic non-linear cosmological perturbation theory
30'
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12:30 - 13:00
Non-Gaussian statistics of galactic dust
Location: Adriatico Guest House Kastler Lecture Hall -
12:30
Non-Gaussian statistics of galactic dust
30'
Speaker: Emory F. Bunn (University of Richmond, USA)
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12:30
Non-Gaussian statistics of galactic dust
30'
-
09:30 - 10:00
Non-Gaussianity in the 21 cm background