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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08:30
Registration & coffee & snacks Lecture Hall
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Kavli IPMU, Kashiwa, Japan
Kashiwa, Japan -
Fe 17 Morning session I Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Masahiro Takada (Kavli IPMU)-
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logistics information
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Accelerating Universe OverviewSpeaker: Hitoshi Murayama (Kavli IPMU/Berkeley)
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(Invited talk) From Quantum Gravity to Low Energy PhysicsSpeaker: Yasunori Nomura (Berkeley/Kavli IPMU)
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Cross-correlation of the astrophysical gravitational-wave background with galaxy clusteringSpeaker: Valeri Vardanyan (Kavli IPMU)
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10:20
Coffee break 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 UniverseSpeaker: Kaz Kohri (KEK)
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primordial black holes with primordial non-GaussianitySpeaker: Yokoyama Shuichiro (KMI, Nagoya University)
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11:55
Lunch break & Poster session Lecture Hall
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Kavli IPMU, Kashiwa, Japan
Kashiwa, Japan -
Feb 17 Afternoon session I Lecture Hall
Lecture Hall
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?Speaker: Tom Melia (Kavli IPMU)
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Searching for particle dark matter by cross-correlating gamma rays and large-scale structureSpeaker: 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 observationsSpeaker: 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 burstsSpeaker: Shuichi Gunji (Yamagata University)
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15:00
IPMU Tea Time & Poster session 3rd Floor, Fujiwara Hall
3rd Floor, Fujiwara Hall
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Feb 17 Afternoon session II Lecture Hall
Lecture Hall
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 experimentsSpeaker: Nicoletta Krachmalnicoff (SISSA)
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Optical designs and performance of LiteBIRDSpeaker: Hiroaki Imada (Université Paris-Saclay, CNRS/IN2P3, IJCLab)
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Cryogenics architecture for LiteBIRD satelliteSpeaker: Takashi Hasebe (JAXA/ISAS)
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Simultaneous determination of the cosmic birefringence and miscalibrated polarisation angles from LiteBIRDSpeaker: Yuto Minami (KEK)
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Poster machine-gun talks Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, Japan
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Coffee & snacks Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, Japan -
Feb 18 Morning session I Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Masashi Hazumi (KEK/Kavli IPMU)- 19
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Supersymmetric model for dark matter and muon g-2Speaker: Norimi Yokozaki (Tohoku University)
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New Insights in to the Stellar Components and Dark Halo in the Milky WaySpeaker: Chiba Masashi (Tohoku University)
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Diversity of the central dark matter densities in the Galactic dwarf spheroidalsSpeaker: Kohei Hayashi (ICRR, U. Tokyo)
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10:30
Coffee break Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, Japan -
Feb 18 Morning session II Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Masashi Hazumi-
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(Invited talk) UV-IR Bottlenecks for Inflation and the HiggsSpeaker: Alexander Westphal (DESY)
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Revisiting slow-roll dynamics and the tensor tilt in general single-field inflationSpeaker: Tsutomu Kobayashi (Rikkyo University)
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12:05
Group Photo Lecture Hall
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Kavli IPMU, Kashiwa, Japan
Kashiwa, Japan -
12:10
Lunch break & Poster session
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Feb 18 Afternoon session I Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Satoshi Miyazaki-
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(Invited talk) eBOSS: Cosmology with Baryon Acoustic Oscillations and Redshift Space DistortionsSpeaker: Kyle Dawson (The University of Utah)
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The impact of projection effects on cluster observablesSpeaker: Tomomi Sunayama (Kavli IPMU)
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Cosmological constraints from galaxy-galaxy lensing and clustering with the Subaru HSC and SDSS BOSS dataSpeaker: Hironao Miyatake (Nagoya University)
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15:10
IPMU Tea Time & Poster session 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- 30
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Initial density field reconstructions from high redshift galaxy surveysSpeaker: Metin Ata (Kavli IPMU)
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Computations of quantities characterizing PBHs formed from primordial perturbationsSpeaker: Teruaki Suyama (Tokyo Institute of Technology)
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19:00
Banquet @ The Meat Dutch; 19:00 - 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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08:30
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08:30
Coffee & snacks Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, Japan -
Feb 19 Morning session I Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Tomonori Usuda-
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B02Speaker: Satoshi Miyazaki (NAOJ)
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Splashback radius of clusters in the HSC surveySpeaker: Masamune Oguri (U. Tokyo/Kavli IPMU)
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(invited talk) Cosmology in the Era of Galaxy Surveys -- from DES to LSST
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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10:40
Coffee break Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, Japan -
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 collidersSpeaker: Kensuke Homma (Hiroshima U.)
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Measurement of expansion of the Universe using high-z type Ia supernovaeSpeaker: Naoki Yasuda (Kavli IPMU)
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Structure of subhalos around Milky Way-mass galaxies in CDM and SIDM universeSpeaker: Takashi Okamoto (Hokkaido Uniersity)
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12:00
Lunch break & Poster session Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, Japan -
Feb 19 Afternoon session I Lecture Hall
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, JapanConvener: Masahiro Takada- 42
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Development of laser comb to calibrate high dispersion spectrograph for radial velocity measurementSpeaker: Hajime Inaba (National Institute of Advanced Industrial Science and Technology (AIST))
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First Stability Results of our Second Gen. Astro-CombSpeaker: Malte Schramm (NAOJ)
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HSC-PFS cross-correlation simulated by the “lognormal_lens” codeSpeaker: 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 surveysSpeaker: Ryu Makiya (Kavli IPMU)
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Closing remarkSpeaker: Hitoshi Murayama (Kavli IPMU/Berkeley)
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