セミナー

Akira Ohnishi, YITP Kyoto University

[EX] (Part II) Femtoscopic approach to hadron-hadron interactions

Online (Zoom), indico page, slides (kek.jp only)
Hadron-hadron interactions are the basic inputs to discuss hadronic molecules and hadronic nuclei. Flavored hadron interactions, however, are generally difficult to access in standard scattering experiments. Recent research activities on hadron-hadron correlation functions open the ways to systematically access flavored hadron interactions such as Ω, Ξ, − and even (¯. Since the correlation function is given as the average of the wave function squared with the normalized source function weight (Koonin-Pratt formula), it contains the information of the hadron-hadron interaction. Thus, provided that the source function is known, one can examine the hadron-hadron interaction. In this seminar, after a short introduction, I first explain how we can calculate the correlation function in simple two cases; (1) quantum statistics operates but there is no pairwise interaction (Hanbury-Brown–Twiss effects), and (2) non-identical particle pairs with a short-range interaction in an analytic model (Lednicky-Lyuboshits model). Next I explain some other effects such as the Coulomb potential and coupled-channel effects. In the third part, I show some of the recent correlation function data reported by the RHIC-STAR and LHC-ALICE collaborations. These data give constraints on the low-energy scattering parameters, and seem to suggest the existence of bound states in some of the hadron-hadron pairs. In the last part, I will give an outlook.

Takumi Doi, RIKEN

[EX] (Part I) Hadron-hadron interactions from Lattice QCD

Online (Zoom), indico page, slides (kek.jp only)
In this talk, I review the first-principles calculations of hadron-hadron interactions from lattice QCD. I introduce a theoretical framework, HAL QCD method, where it is shown that the notion of potential can be rigorously introduced/calculated as a representation of the S-matrix of QCD. Recent numerical results are presented, in particular, for hyperon forces obtained near the physical point. The physical implications for exotic dibaryons, hyper-nuclei, equation of state of high dense matter and the structure of neutron stars are also discussed and future prospects will be given.

Milad Delfan Azari, Waseda University

Physics of fast collective neutrino oscillations in core-collapse supernovae

Online (Zoom), indico page, slides (kek.jp only)
Neutrinos are highly populated inside the core of massive stars. They play an important role in the explosion mechanism of core-collapse supernovae. It is known that, almost all of the energy in the gravitational collapse is emitted in the form of neutrinos. They may change their identity through so-called fast flavor conversion induced by mutual forward scatterings. If this fast flavor conversion happens, it may have an impact on the dynamics of supernova explosions, since it may occur near the neutrino sphere. In this presentation, the latest results of our understanding of the neutrino fast flavor conversions in core-collapse supernovae will be reported.

Graham White, Kavli IPMU

Learning about cosmology using astrometry

Online (Zoom), indico page, slides (kek.jp only)
Gaia is observing the position and path of an enormous number of stars. Future experiments promise to do so for even more stars at high precision. If the light from such a star is traveling to us through a stochastic gravitational wave background, the apparent position of the star will be displaced by an amount essentially independent of the distance but dependent on the strength of the gravitational wave. Correlations in such shifts from many stars can be used to detect or constrain a gravitational wave background. The frequency range probed partially fills the gap between pulsar timing arrays and LISA. We explore the potential cosmological consequences of this by looking at phase transitions, topological defects and pbhs.

Zebin Qiu, University of Tokyo

[QCD theory Seminar] Magnetic effects in dense nuclear matter through Skyrme model

Online (Zoom)
Skyrme model is among the simplest extensions of chiral effective theory including anomaly. We investigate how an external magnetic field deforms the classical Skyrmion soliton structure while maintaining the topological winding. We further identify quantized Skyrmions as neutrons and protons, revealing a mass split between them induced by the magnetic field. More intriguing aspects arise when we annex multiple Skyrmions to form a crystal and realize the ¥pi^0 domain wall as a special class of solution. We establish the thermodynamics and phase diagram of different classes of Skyrme crystals, beneath which is the topological transmutation between ¥pi_3(S^3) and ¥pi_1(S^1).

Kazuya Yonekura, Tohoku University

Atiyah-Patodi-Singer index theorem from axial anomaly

Online (Zoom) https://kds.kek.jp/event/38462/
I will talk about a simple physical derivation of the so-called Atiyah-Patodi-Singer (APS) index theorem. The derivation is just a minor modification of Fujikawa’s argument for the axial U(1) anomaly once we we understand a physical interpretation of the APS boundary condition. It is based on my recent work with Shun K. Kobayashi https://arxiv.org/abs/2103.10654

Juan Carlos Vasquez, University of Massachusetts

Resurgence of the QCD Adler function

Online (Zoom) https://kds.kek.jp/event/38304/
We study the QCD Adler function in the energy region ≈ 0.7 − 2.5 GeV, in which the non perturbative effects become dominant. Our analysis is a renormalon-based evaluation using transseries within the resurgence of the Renormalization-Group-Equation and does not require the Operator-Product-Expansion.

Christophe Royon, University of Kansas

[EX and IPNS joint seminar] Measuring intact protons at the LHC: From the odderon discovery to the search for axion-like particles

Online (Zoom)
In the first part of the talk, we will describe the odderon discovery by the TOTEM and D0 experiments. The analysis compares the p pbar elastic cross section as measured by the D0 Collaboration at a center-of-mass energy of 1.96 TeV to that in pp collisions as measured by the TOTEM Collaboration at 2.76, 7, 8, and 13 TeV. The two data sets disagree at the 3.4 sigma level and thus provide evidence for the t-channel exchange of a colorless, C-odd gluonic compound, also known as the odderon. We combine these results with a TOTEM analysis of the same C-odd exchange based on the total cross section and the ratio of the real to imaginary parts of the forward elastic strong interaction scattering amplitude in pp scattering, leading to a combined significance larger than 5 sigma. In a second part of the talk, we will describe the perspective on the search for quartic anomalous couplings and axion-like particles using tagged protons in the final state, leading to sensitivities to beyond standard model physics that improve by 2 to 3 orders of magnitude on the coupling. We will finish by decribing briefly the ultra fast silicon detectors for timing measurements as well as for medical and cosmic ray physics applications.

Michal P. Heller, Max Planck Institute and NCBJ

[QCD theory Seminar] New results on convergence of hydrodynamic gradient expansion

Online (Zoom)
Relativistic hydrodynamics, viewed as an effective field theory, is formulated in a derivative expansion. Studies of applicability of relativistic hydrodynamics in nuclear collisions at RHIC and LHC prompted 1302.0697 to explore convergence properties of this expansion. This and subsequent works showed that the Bjorken flow gives rise to a gradient expansion with a vanishing radius of convergence in all but a single studied quark-gluon plasma model. In my talk I will overview the current status of this field, as well as outline new developments on this topic that, for the first time, allow to make definite statements about the
convergence of hydrodynamic gradient expansion. New results follow from 2007.05524 and an ongoing work.

Tokiro Numasawa, University of Tokyo

Four coupled SYK models and Nearly AdS2 gravities: Phase Transitions in Traversable wormholes and in Bra-ket wormholes

Online (Zoom) https://kds.kek.jp/event/38340/
Wormholes are interesting and important objects in gravity.
In particular, recently controllable examples of traversable wormholes are constructed.
To understand these wormholes better, we study the two traversable wormhole configurations through the study of four coupled SYK models and nearly AdS2 gravities.
In the SYK model side, we construct a model that couples two copies of two coupled SYK models.
In the nearly AdS2 gravity side, we entangle matter fields in two copies of traversable wormholes.
In both cases, the systems show first order phase transitions at zero temperature by changing couplings, which is understood as the exchange of traversable wormhole configurations.
In nearly AdS2 gravity cases, through the double wick rotation, traversable wormholes are interpreted as bra-ket wormholes, which gives a connection between bra and ket vectors.
In Lorentzian signature, these bra-ket wormholes lead to two closed universes that are entangled with each other as well as matter fields in the flat space without dynamical gravity.
We study the effect of projection or entangling operation for matters on flat spaces and they cause phase transitions in bra-ket wormholes, which leads to the pair annihilation of closed universes.
Using these bra-ket wormholes, we discuss the way to embed states in 2d holographic CFTs into Hilbert space of many 2d free fields.

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