KEK Theory Workshop is an annual workshop on string theory and quantum field theory. Since KEK Theory Workshop 2014, it has been held as an international workshop. Speakers are invited from abroad as well as from Japan, and all talks are given in English.
This year we aim to provide a valuable opportunity to have extensive discussions on new developments in tensor networks, quantum information and quantum computing from the viewpoint of particle physics, quantum gravity and condensed matter physics applications. The invited speakers are selected from various research fields, and we have asked them to give a pedagogical exposition of the big picture in their own research field with the right amount of technical details, which are useful in building up a comprehensive understanding of the notions and their mutual relationship.
The workshop will be ON-SITE at KEK Tsukuba Campus on December 11 (Wed.) -- 13 (Fri.), 2024, without on-line attendance. Please visit K03 Building.
Invited Speakers
Short Talks
We will arrange short talk sessions on more diverse topics, for which participants can apply. If there are too many applicants, we will have to make some selection.
Scam Email Warning
Please be aware of potential scams claiming to make housing reservations on your behalf. We were made aware of some participants receiving such messages from "Conferences@reservationsmanagement.org" or similar addresses. Please ignore such emails and do not reply, do not click shared links, and do not provide your credit card information.
Organizers
Yuta Hamada, Kohta Hatakeyama, Machiko Hatsuda,
Satoshi Iso, Gregory Joseph Loges, Kohtaroh Miura,
Shun'ya Mizoguchi, Jun Nishimura, Hiroki Ohata, Katsuta Sakai
Secretary
Yuko Ohno (Ms.) yukoohno[at]post.kek.jp
(Please replace [at] with @.)
Tensor network is a powerful numerical tool to compute the wave function of quantum many-body systems and to directly evaluate the path integrals in quantum field theory. In this talk, I mainly explain the latter case in detail. After introducing the basics of the tensor network. I give an overview of its recent progress especially in elementary particle physics. As specific examples, I explain how to compute the entanglement entropy, spectroscopy using tensor network, and recent developments of the tensor network coarse-graining algorithms. Finally I mention future perspective towards lattice QCD.
Monte Carlo simulations of quantum time-evolution based on the real-
time path integral have been thought to be extremely difficult since it involves a
phase factor exp(iS) in the integrand, which causes a severe sign
problem. We apply the Lefschetz thimble method with various new
techniques to such systems. In this talk, I would like to discuss a new
understanding of quantum tunneling and quantum decoherence that arises
as complex saddle point configurations. I would also like to discuss how
one can apply this method to investigate the beginning of the universe
based on quantum gravity.
Catering from 百香亭 (Chinese Restaurent)
A central challenge in large-scale quantum information processing is
managing noise in quantum systems. Quantum error correction (QEC)
addresses this by encoding quantum states into quantum error
correction codes (QECCs) before noise occurs and decoding them
afterward. Recently, QEC has attracted significant attention in
theoretical physics due to its potential connections to quantum chaos
and quantum gravity. As interest in QEC becomes broader, the decoding
problem --how to decode a general QECC-- is increasingly important. A
few were known so far, but we recently proposed two approaches: one
extends decoders for the standard class of QECCs based on stabilizers
[1], and the other generalizes the Yoshida-Kitaev decoder [2],
originally used to explore the black hole information paradox. In this
talk, we present an overview of these approaches.
1) "Decoding general error correcting codes and the role of
complementarity", YN, T. Matsuura, and M. Koashi, arXiv:2210.06661 (2022).
2) "Explicit decoders using fixed-point amplitude amplification based
on QSVT", T. Utsumi, and YN, arXiv:2405.06051 (2024).
The generalized uncertainty relation is expected to be an essential element in a theory of quantum gravity. We examine its effect on the Hawking radiation of a Schwarzschild black hole formed from collapse by incorporating a minimal uncertainty length scale into the radial coordinate of the background. This is implemented in both the ingoing Vaidya coordinates and a family of freely falling coordinates. We find that, regardless of the choice of the coordinate system, Hawking radiation is turned off at around the scrambling time. Interestingly, this phenomenon occurs while the Hawking temperature remains largely unmodified.
We reexamined the connection between the Hawking radiation of a Schwarzschild black hole formed from collapse and ultraviolet(UV) physics with the local Lorentz symmetry violation or the existence of a minimal length. Significant modifications are reported after the scrambling time in both cases, which reflects the UV sensitivity of Hawking radiation. Depending on the physics at the singularity, Hawking radiation with the modified dispersion relation may be largely suppressed with a striking tunneling phenomenon behind. The Hawking wavepacket may exceed the size of the black hole under the generalized uncertainty principle that it longer employs the near horizon Unruh vacuum with a diminishing Hawking radiation amplitude. While a turned-off effect is shared in these two implementations, the Hawking temperature remains the same or only perturbatively corrected.