Program

To see the talk file , please click the speaker name.

2/19 (Thu) 2/20 (Fri) 2/21 (Sat)
9:00 - 9:30 Registration    

Morning Session

9:30 - 12:00

C. Baccigalupi (Planck exp. and foregrounds for CMB B-mode)

M. Hazumi & A. Lee (CMB experiments: present and future)

M. Kawasaki (QCD axion)

     
X. Chen (Primordial feature and
non-Gaussianity)
M. Cicoli (String cosmology) K. Nakayama (Primordial GW)
Lunch      

Afternoon Session I

13:00 - 15:00

F. Takahashi ( Influm: review)

G. Shiu (Inflation in string theory)

J. Soda (Form field inflation)

Discussion Session
(J. Yokoyama, K. Kohri)
T. Kobayashi (String pheno, inflation)

Y. Oyama
N. Kitajima
H. Yoshino

Break Photo  

Afternoon Session II

15:30 - 18:15

K. Kohri
M. Karciauskas
J. White

H. Kodama
T. Terada
Y. Yamada

15:45 Closing
     

K. Bamba
S. Kawai

N. Yamanaka
T. Matsuda
 
Poster (all day)

Y. Hamada
S. Ichinose
Y. Watanabe

Bus departs at 18:40
  Reception (18:30 - 20:00) Banquet (19:00 - 21:00)

Last Update: 23 February, 2015

February 19 (Thursday)

Morning Session

[chair: Masashi Hazumi]

Carlo Baccigalupi (SISSA):

Recent measurements of contaminants to cosmological B-modes

Xingang Chen (Texas U, Dallas)

High energy physics in the primordial density perturbations

Afternoon Session I

[chair Hideo Kodama]

Fuminobu Takahashi (Tohoku U)

High and intermediate-scale inflation

Discussion Session

Kazunori Kohri (KEK)

Jun'ichi Yokoyama (RESCEU, U Tokyo)

Afternoon Session II

[chair: Fuminobu Takahashi]

Kazunori Kohri (KEK)

Large and small field conformal inflation models

Mindaugas Karciauskas (KEK)

The effects of radiative corrections on inflation observables

Jonathan White (RESCEU, U Tokyo)

Open inflation and scalar suppression on large scales

[chair: Shun'ya Mizoguchi]

Kazuharu Bambda (Ochanomizu U)

Large-scale magnetic fields, non-Gaussianity, and primordial gravitational waves from inflation

Shinsuke Kawai (Sugnkyunkwan U)

Testing supersymmetric Higgs inflation with non-Gaussianity

Reception 18:30 - 20:30

February 20 (Friday)

Morning Session

[chair: Jiro Soda]

Masashi Hazumi (KEK) & Adrian Lee (UC Berkeley)

TBA

Michele Cicoli (Bologna U)

Pre- and post-inflationary string cosmology

Afternoon Session I

[chair: Yoske Sumitomo]

Gary Shiu (Wisconsin U/HKUST)

Inflation, B-mode, and string theory

Tatsuo Kobayashi (Hokkaido U)

Towards natural inflation in string theory

Afternoon Session II

[chair: Tetsutaro Higaki]

Hideo Kodama (KEK)

Multi-dimensional Starobinsky-type inflation in gauged maximal supergravity

Takahiro Terada (U Tokyo)

MSSM Higgs inflation - an application of inflation without the stabilizer superfield -

Yusuke Yamada (Waseda U)

Inflation in supergravity without Kaehler potential

[chair: Tatsuo Kobayashi]

Nodoka Yamanaka (Riken)

Dark matter in the hidden gauge theory and Higgs mini-inflation

Tomohiro Matsuda (Saitama Inst. Tech.)

Scale dependence from additional degree of freedom during inflation

Banquet 19:00 - 21:00 at Japanese Restaurant "Sasanoya"

February 21 (Saturday)

Morning Session

[chair: Kazunori Kohri]

Masahiro Kawasaki (ICRR, U Tokyo)

Cosmological aspect of QCD axion

Kazunori Nakayama (U Tokyo)

Inflationary gravitational waves as a probe of the early universe

Afternoon Session

[chair: Kazunori Nakayama]

Jiro Soda (Kobe U)

Impact of form fields on primordial gravitational waves

Yoshihiko Oyama

Constraints on the neutrino mass by future precise CMB polarization and 21cm line observations

Naoya Kitajima

Gravitational waves from Higgs domain walls

Hirotaka Yoshino

Axion bosenova

Closing 15:45

 

Poster

Yuta Hamada (Kyoto U)

TBA

Shoichi Ichinose (Shizuoka U)

New approach to cosmological fluctuation and CMB power spectrum

Yuki Watanabe (RESCEU, U Tokyo)

Self-unitarization of new Higgs inflation and compatibility with Planck and BICEP2 data

 

Sponsor

    This workshop is supported by the KEK Theory Center and the JSPS Grant-in-Aid for Scientific Research (A) 26247042
    "Quest for the Ultimate Theory in terms of rich cosmophysical phenomena caused by fields and particles in the hidden sector".