STOchastic LAttice Simulation of hybrid inflation
Tomoaki Murata and Yuichiro Tada
arXiv:
2603.04850
[astro-ph.CO].
Calculating the power spectrum in stochastic inflation by Monte Carlo simulation and least squares curve fitting
Koichi Miyamoto and Yuichiro Tada
arXiv:
2508.17654
[astro-ph.CO].
I'm a theoretical scientist in Rikkyo University, Japan. I'm working to elucidate inflation, dark matter, and dark energy, a.k.a. the three mysteries of the universe, combining theory, observation, and numerical simulation. I have developed a computer simulator of inflation, STOchastic LAttice Simulation (STOLAS), to investigate the physics of the primordial black hole as a candidate for dark matter. I'm also interested in the theoretical framework of dynamical dark energy, and its observational signatures.
I'm from Saitama, Japan. I completed B.Sc. in Physics in 2012 and M.Sc. in Physics in 2014, and received Ph.D. in Physics from the University of Tokyo in March 2017.
Yuichiro Tada
4335, Bldg.4, Rikkyo University
3-34-1 Nishi-Ikebukuro, Toshima-ku
Tokyo 171-8501, Japan
+81 (0)3-3985-4637
yuichiro.tada@rikkyo.ac.jp
Stochastic formalism can view inflation as a set of "random walks". We have developed a computer simulator of inflation, STOLAS, based on this stochastic formalism. It is the first simulation which can calculate the curvature perturbation in a non-perturbative way. It would be helpful to investigate the physics of, e.g., the primordial black hole as a candidate for dark matter. Also, it could be connected to the existing simulations of halos/galaxies, enabling us to simulate the whole history of the universe! Inflation, Random walk, Lattice simulation
Primordial black holes (PBHs) are hypothetical black holes formed in the very early universe. They are a candidate of dark matter as well as a source of merger gravitational waves detected by LIGO/Virgo/KAGRA observatories. I have so far working on their formation scenarios, gravitational wave signatures, precise calculation of their abundance, etc., which are summarised in the anthology textbook.
Dark Matter, Gravitational Wave, Inflation
Recent detailed observations of the large-scale structure of galaxies suggested that "dark energy", the source of the accelerated expansion of the universe today, might be time-evolving. We have quickly reported its interpretation as a dynamical scalar field known as "quintessence". We have also investigated what happens if the quintessence field resonantly enhances its fluctuations.
Dark energy, Quintessence, Resonance
(Possible) large primordial density perturbations can induce gravitational waves via their accoustic oscillation, known as "scalar-induced gravitational waves (SIGWs)". Not only can they be a smoking gun of PBHs, but also they can record the thermal history of the universe, such as a plasma crossover represented by QCD.
Gravitational wave, Primordial black hole, Thermal history
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Photography
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Branding, Illustration
Ph.D. in Physics
•
23rd March 2017
Department of Physics, Adviser:
Dr. Masahiro Kawasaki & Dr. Hitoshi Murayama
M.Sc. in Physics
•
24th March 2014
Department of Physics, Adviser:
Dr. Masahiro Kawasaki & Dr. Hitoshi Murayama
B.Sc. in Physics
•
23rd March 2012
Department of Phyiscs
Graduate • March 2008
Assistant Professor
•
April 2025–Present
Department of Physics
Designated Assistant Professor
•
April 2021–March 2025
Institute for Advanced Research & Department of Physics, C-lab.
Associate Researcher
•
April 2022–March 2023
Institute of Particle and Nuclear Studies
Lecturer (part-time)
•
April 2019–March 2021
Classical mechanics 1, 2
JSPS Fellow (PD)
•
April 2018–March 2021
C-lab., Department of Physics
PD researcher
•
April 2017–March 2018
Dr. Sébastien Renaux-Petel's Group
JSPS Fellow (DC2)
•
April 2015–March 2017
Kavli IPMU & ICRR
ALPS Fellow
•
October 2012–March 2017
Kavli IPMU & ICRR
Department of Physics, The University of Tokyo,
Bunkyo-ku, Tokyo 113-0033, Japan
Kavli Institute for the Physics and
Mathematics of the Universe (WPI), UTIAS,
The University of Tokyo, 5-1-5 Kashiwanoha,
Kashiwa, Chiba 277-8583, Japan
Institute for Cosmic Ray Research,
The University of Tokyo, 5-1-5 Kashiwanoha,
Kashiwa, Chiba 277-8582, Japan
| Referees | |
|---|---|
| Dr. Masahiro Kawasaki | Supervisor |
| Dr. Hitoshi Murayama | Supervisor |
| Dr. Koichi Hamaguchi | Chief Examiner |
| Dr. Aya Bamba | Examiner |
| Dr. Masahiro Ibe | Examiner |
| Dr. Shinji Miyoki | Examiner |
| Dr. Jun’ichi Yokoyama | Examiner |
Department of Physics, The University of Tokyo,
Bunkyo-ku, Tokyo 113-0033, Japan
Kavli Institute for the Physics and
Mathematics of the Universe (WPI), UTIAS,
The University of Tokyo, 5-1-5 Kashiwanoha,
Kashiwa, Chiba 277-8583, Japan
| Referees | |
|---|---|
| Dr. Masahiro Kawasaki | Supervisor |
| Dr. Hitoshi Murayama | Supervisor |
| Dr. Jun’ichi Yokoyama | Examiner |
Editor: Manuel Arca Sedda, Elisa Bortolas, Mario Spera
ISBN: 978-0-323-95636-9
Prof. Kari Enqvist's group, University of Helsinki
•
1st October–22nd December 2014
ALPS course work
Classical and Quantum Gravity (CQG)
European Physical Journal C (EPJC)
Journal of Cosmology and Astroparticle Physics (JCAP)
Monthly Notices of the Royal Astronomical Society (MNRAS)
Modern Physics Letters A (MPLA)
Physical Review D (PRD)
Physical Review Letters (PRL)
Progress of Theoretical and Experimental Physics (PTEP)
Universe
Physics meets Mathematics
(PI)
International Research Network Extragalactic astrophysics and Cosmology (NECO)
理論天文学宇宙物理学懇談会 • 2015年6月4日–現在
日本物理学会 •
2013年6月1日–現在
Dynamics of primordial black hole formation II
•
7–10th October 2024
"Physics meets Mathematics" まとめ合宿
•
10–12th February 2024
JGRG 32
•
27th November–1st December 2023
自然科学カフェ
— 星が先かブラックホールが先か —
原始ブラックホール研究の最前線
多田祐一郎
2025年2月15日 @ 日比谷図書文化館 4階 スタジオプラス
— 星が先かブラックホールが先か —
原始ブラックホール研究の最前線
多田祐一郎
2024年11月14日 @ 豊田西高校
招待講演
名大発アカデミックフラッシュ 第2報
宇宙の「インフレ」と「金融工学」
多田祐一郎
2021年9月3日 @ オンライン, 招待
名古屋大学・名古屋市科学館 公開オンラインセミナー
星が先かブラックホールが先か?原始ブラックホール研究の最前線
多田祐一郎
2021年8月22日 @ オンライン, 招待
C++ workshop
@ Nagoya U.
Julia seminar
•
Introductory Seminar on Basic Physics
@ Rikkyo U.
確率形式によるインフレーション宇宙のゆらぎの非摂動的理解 • 2024年11月
Inflationary stochastic anomalies
L. Pinol, S. Renaux-Petel and Y. Tada
Class. Quant. Grav. 36, no. 7, 07LT01 (2019)
[arXiv:
1806.10126
[gr-qc]].
Conformal inflation in the metric-affine geometry
Y. Mikura, Y. Tada and S. Yokoyama
EPL 132, no.3, 39001 (2020)
[arXiv:
2008.00628
[hep-th]].
Online JGRG Workshop 2020
•
27th November 2020
Manifestly covariant theory of stochastic inflation (poster) ▼
The stochastic approach to inflation can non-perturbatively treat the superhorizon fluctuations
as the classical random noise to go beyond the standard perturbative QFT approach.
I first review how this approach enables us to calculate the observable curvature perturbations
in a non-perturbative way
and how it can be implemented in a numerical program. I then describe the covariance of the
stochastic theory
and the discretization scheme of the stochastic noise, which are important both theoretically
and practically.
Mathematically the stochastic noise can be discretized in an arbitrary manner, but we reveal the
physically motivated discretization,
which ensures the covariance of the stochastic theory on the inflatons' target manifold.
L. Pinol, S. Renaux-Petel, and Y. Tada
FAPESP-JSPS Workshop on dark energy, dark matter, and galaxies
•
February 2019
Aspects of primordial black hole as dark matter (oral)
K. Inomata, M. Kawasaki, A. Kusenko, K. Mukaida, Y. Tada,
T. T. Yanagida, and S. Yokoyama
ICRR Master and Doctor Thesis Workshop • 24th February 2017
天文・天体物理若手夏の学校 • 2015年7月30日
天文・天体物理若手夏の学校 • 2013年8月1日
JSPS Grant-in-Aid for Scientific Research (C)
•
1st April 2024–31st March 2027
No. 24K07047, Principal Investigator, ¥4,550,000.
2023 Collaborative Research Grants for YLC
•
1st July 2023–31st March 2024
Principal Investigator, ¥1,000,000.
JSPS Grant-in-Aid for Early-Career Scientists
•
1st April 2021–31st March 2024
No. 21K13918, Principal Investigator, ¥4,680,000.
JSPS Grant-in-Aid for Early-Career Scientists
•
1st April 2019–31st March 2022
No. 19K14707, Principal Investigator, ¥1,560,000.
Grant-in-Aid for JSPS Fellows
•
25th April 2018–31st March 2021
No. 18J01992, JSPS Fellow (PD), ¥3,640,000.
Grant-in-Aid for JSPS Fellows
•
24th April 2015–31st March 2017
No. 15J10829, JSPS Fellow (DC2), ¥1,900,000.
Yuichiro Tada
4335, Bldg.4, Rikkyo University
3-34-1 Nishi-Ikebukuro, Toshima-ku
Tokyo 171-8501, Japan
+81 (0)80-9566-9181
yuichiro.t.tada@gmail.com
yuichiro.tada@rikkyo.ac.jp
tada.yuichiro.y8@f.mail.nagoya-u.ac.jp
tada.yuichiro@e.mbox.nagoya-u.ac.jp
tada_at_iap.fr
yuichiro.tada_at_ipmu.jp