Cosmic Acceleration
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Dates: February 17 - 19, 2020
Venue: Lecture Hall, Kavli IPMU, Kashiwa, Japan
Overview:
Because gravity is an attractive force, the expansion speed of the Universe should be decreasing. However, observational data accumulated over the years strongly support that the present Universe is in the phase of the accelerated expansion and there was also another phase of the accelerated expansion in the very early Universe. The physical echanism that makes the Universe undergo the ccelerated expansion is not known yet. Some “repulsive force” is necessary. The purpose of this innovative area is to clarify the origin of the accelerated expansion. In order to achieve this goal, it is necessary to investigate the interplay between the repulsive force causing the accelerated expansion and the attractive force sourced by dark matter which triggers the formation of the cosmic structures such as the galaxies and clusters of galaxies. In this innovative area, researchers from different fields join together and form nine sub-groups: inflation in the early Universe (A01), decelerated expansion by dark matter (A02), accelerated expansion by dark energy in the present Universe (A03), cosmic microwave background (B01), galaxy imaging (B02), galaxy spectroscopy (B03), direct measurement of the cosmic expansion (B04), ultimate data analysis (D01), and ultimate theory of the Universe (C01). Not only collaborations within each individual sub-group but also collaborations among the different sub-groups are essential to obtain scientific achievements we desire.
This symposium consists of reports of scientific results by representatives and members of each sub-group as well as researchers selected for public research.
Invited speakers:
Chihway Chang (KICP, U. Chicago)
Kyle Dawson (Utah)
Konstantinos Dimopoulos (Lancaster)
Elisa Ferreira (MPA)
Nicoletta Krachmalnicoff (SISSA)
Tom Melia (Kavli IPMU: TBC)
Marius Millea (BCCP, UC Berkeley)
Alexander Westphal (DESY)
Code of Conduct:
It is the policy of the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU) that all members and visitors will conduct themselves in a professional manner that is welcoming and free from any form of discrimination, harassment, or retaliation. Members and visitors will avoid any inappropriate actions or statements based on individual characteristics such as age, race, ethnicity, gender, sexual orientation, marital status, nationality, or political affiliation. Disruptive or harassing behavior of any kind will not be tolerated. Harassment includes but is not limited to inappropriate or intimidating behavior and language, unwelcome jokes or comments, unwanted touching or attention, offensive images, photography without permission, and stalking. Members and visitors will treat each other with respect to create a collegial, inclusive, and professional environment at the Kavli IPMU.
Organizers:
Masashi Hazumi (KEK/Kavli IPMU)
Eiichiro Komatsu (MPA/Kavli IPMU)
Ryu Makiya (Kavli IPMU)
Satoshi Miyazaki (NAOJ)
Hitoshi Murayama (Kavli IPMU/Berkeley)
Hirosi Ooguri (Caltech/Kavli IPMU)
Naoshi Sugiyama (Nagoya/Kavli IPMU)
Tomomi Sunayama (Kavli IPMU)
Masahiro Takada (Kavli IPMU)
Fuminobu Takahashi (Tohoku U.)
Tomonori Usuda (NAOJ)
Address:
Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU),
the University of Tokyo, 5-1-5 Kashiwa-no-ha, Kashiwa City, Chiba 277-8583, Japan
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Registration & coffee & snacks 30m Lecture Hall
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Fe 17 Morning session I Lecture Hall
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Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Masahiro Takada (Kavli IPMU)-
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logistics information 5m
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Accelerating Universe Overview 25mSpeaker: Hitoshi Murayama (Kavli IPMU/Berkeley)
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(Invited talk) From Quantum Gravity to Low Energy Physics 30mSpeaker: Yasunori Nomura (Berkeley/Kavli IPMU)
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Cross-correlation of the astrophysical gravitational-wave background with galaxy clustering 20mSpeaker: Valeri Vardanyan (Kavli IPMU)
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Coffee break 25m Lecture Hall
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Feb 17 Morning session IIConvener: Masahiro Takada
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Formations and clusterings of primordial black hole dark matter formed in the matter dominated Universe 20mSpeaker: Kaz Kohri (KEK)
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primordial black holes with primordial non-Gaussianity 20mSpeaker: Yokoyama Shuichiro (KMI, Nagoya University)
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Lunch break & Poster session 1h 35m Lecture Hall
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Feb 17 Afternoon session I Lecture Hall
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Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Fuminobu Takahashi (Tohoku U.)-
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(Invited talk) The light dark matter search— what’s going on at an MeV? 30mSpeaker: Tom Melia (Kavli IPMU)
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Searching for particle dark matter by cross-correlating gamma rays and large-scale structure 20mSpeaker: Shin'ichiro Ando (University of Amsterdam)
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Constraint on the nature of dark matter by high-resolution cosmological simulations and next generation spectroscopy observations 20mSpeaker: Tomoaki Ishiyama (Chiba University)
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The study on quantum gravity theory through polarization measurements of high energy gamma rays from gamma ray bursts 20mSpeaker: Shuichi Gunji (Yamagata University)
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IPMU Tea Time & Poster session 30m 3rd Floor, Fujiwara Hall
3rd Floor, Fujiwara Hall
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Feb 17 Afternoon session II Lecture Hall
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Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Eiichiro Komatsu (MPA/Kavli IPMU)-
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(Invited talk) Goals and challenges for next generation of CMB experiments 30mSpeaker: Nicoletta Krachmalnicoff (SISSA)
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Optical designs and performance of LiteBIRD 15mSpeaker: Hiroaki Imada (Université Paris-Saclay, CNRS/IN2P3, IJCLab)
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Development of LiteBIRD polarization modulator 15mSpeaker: Yuki Sakurai (Kavli IPMU)
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Cryogenics architecture for LiteBIRD satellite 15mSpeaker: Takashi Hasebe (JAXA/ISAS)
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Simultaneous determination of the cosmic birefringence and miscalibrated polarisation angles from LiteBIRD 15mSpeaker: Yuto Minami (KEK)
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Poster machine-gun talks Lecture Hall
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Kashiwa, Japan
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Coffee & snacks 30m Lecture Hall
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Feb 18 Morning session I Lecture Hall
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Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Masashi Hazumi (KEK/Kavli IPMU)- 09:00
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Supersymmetric model for dark matter and muon g-2 20mSpeaker: Norimi Yokozaki (Tohoku University)
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New Insights in to the Stellar Components and Dark Halo in the Milky Way 20mSpeaker: Chiba Masashi (Tohoku University)
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Diversity of the central dark matter densities in the Galactic dwarf spheroidals 20mSpeaker: Kohei Hayashi (ICRR, U. Tokyo)
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Coffee break 15m Lecture Hall
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Feb 18 Morning session II Lecture Hall
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Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Masashi Hazumi-
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(Invited talk) UV-IR Bottlenecks for Inflation and the Higgs 30mSpeaker: Alexander Westphal (DESY)
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Revisiting slow-roll dynamics and the tensor tilt in general single-field inflation 20mSpeaker: Tsutomu Kobayashi (Rikkyo University)
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Group Photo 5m Lecture Hall
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Lunch break & Poster session 1h 20m
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Feb 18 Afternoon session I Lecture Hall
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Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Satoshi Miyazaki-
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(Invited talk) eBOSS: Cosmology with Baryon Acoustic Oscillations and Redshift Space Distortions 30mSpeaker: Kyle Dawson (The University of Utah)
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The impact of projection effects on cluster observables 20mSpeaker: Tomomi Sunayama (Kavli IPMU)
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Cosmological constraints from galaxy-galaxy lensing and clustering with the Subaru HSC and SDSS BOSS data 20mSpeaker: Hironao Miyatake (Nagoya University)
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IPMU Tea Time & Poster session 50m 3rd Floor, Fujiwara Hall
3rd Floor, Fujiwara Hall
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Feb 18 Afternoon session II Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Misao Sasaki- 16:00
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Initial density field reconstructions from high redshift galaxy surveys 20mSpeaker: Metin Ata (Kavli IPMU)
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Computations of quantities characterizing PBHs formed from primordial perturbations 20mSpeaker: Teruaki Suyama (Tokyo Institute of Technology)
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Banquet @ The Meat Dutch; 19:00 - 2h Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, Japan30min from IPMU (by walk), 5min from Mitsui-Garden Hotel or Kashiwa-no-Ha Campus station
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Coffee & snacks 30m Lecture Hall
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Feb 19 Morning session I Lecture Hall
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Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Tomonori Usuda-
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B02 30mSpeaker: Satoshi Miyazaki (NAOJ)
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Splashback radius of clusters in the HSC survey 20mSpeaker: Masamune Oguri (U. Tokyo/Kavli IPMU)
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(invited talk) Cosmology in the Era of Galaxy Surveys -- from DES to LSST 30m
We are at an exciting time of cosmology with a number of Stage III galaxy surveys finishing up and Stage IV experiments on the horizon. In this talk I will summarize some of the first year DES cosmology results, focusing on the 3x2pt and 5x2pt analysis which probes the large-scale structure through the galaxy and weak lensing fields. I will point out some of the challenges going forward with DES and LSST, as well as some new exciting directions that the new data allows us to explore.
Speaker: Chihway Chang (University of Chicago)
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Coffee break 20m Lecture Hall
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Feb 19 Morning session II Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Tomonori Usuda-
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Laboratory searches for pseudo Nambu-Goldstone bosons with stimulated photon-photon colliders 20mSpeaker: Kensuke Homma (Hiroshima U.)
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Measurement of expansion of the Universe using high-z type Ia supernovae 20mSpeaker: Naoki Yasuda (Kavli IPMU)
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Structure of subhalos around Milky Way-mass galaxies in CDM and SIDM universe 20mSpeaker: Takashi Okamoto (Hokkaido Uniersity)
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Lunch break & Poster session 1h 15m Lecture Hall
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Kavli IPMU, Kashiwa, Japan
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Feb 19 Afternoon session I Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Masahiro Takada- 13:15
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Development of laser comb to calibrate high dispersion spectrograph for radial velocity measurement 20mSpeaker: Hajime Inaba (National Institute of Advanced Industrial Science and Technology (AIST))
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First Stability Results of our Second Gen. Astro-Comb 20mSpeaker: Malte Schramm (NAOJ)
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HSC-PFS cross-correlation simulated by the “lognormal_lens” code 25mSpeaker: Issha Kayo (Tokyo University of Technology)
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Thermal history of the universe probed by a joint analysis of the thermal Sunyaev–Zeldovich effect and galaxy surveys 25mSpeaker: Ryu Makiya (Kavli IPMU)
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Closing remark 5mSpeaker: Hitoshi Murayama (Kavli IPMU/Berkeley)
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