Hiroshi Suzuki, Kyushu University
Gradient flow exact renormalization group
Online (Zoom) https://kds.kek.jp/event/38153/
The so-called gradient flow, a gauge covariant diffusion of the gauge field, bears a close resemblance to the coarse graining involved in the Wilsonian renormalization group (RG). In scalar field theory, a precise connection between the gradient flow and the Wilsonian RG flow can be made. By imitating the structure of this connection, we propose a Wilsonian RG equation that preserves manifest gauge invariance in vector-like gauge theory. I also mention some ongoing studies on the basis of this formulation.
Kei Yamamoto, Hiroshima University
EFT approach in U(2) and U(3) flavor symmetries
Online (Zoom), indico page, slides (kek.jp only) The measurements of quark flavor-violating observables show a success of the Standard Model (SM). If we insist that new physics (NP) has to emerge in the TeV region, we need to conclude that NP possesses a highly non-generic flavor structure (flavor problem). One of the reasonable solutions to the flavor problem is to introduce flavor symmetry hypothesis. U(3) flavor symmetry is the maximal flavor symmetry allowed by the SM gauge group, and it is known as the Minimal Flavor Violation hypothesis. U(2) is the corresponding subgroup acting only on the first two (light) generations, and shows a good agreement with Yukawa and CKM hierarchical structures. Interestingly, it is shown that U(2) has a good compatibility with the recent B-anomalies. On the other hand, LHC results so far show that there is a mass gap between the SM spectrum and NP. It has motivated the systematic Effective Field Theory (EFT) approach. In this talk, after a brief review of U(3) and U(2) flavor symmetry, I will show how these flavor symmetries act on the SMEFT, providing an organizing principle to classify the large number of dimension-six operators involving fermion fields. The phenomenological study focusing on B-anomalies will be also discussed.
The measurements of quark flavor-violating observables show a success of the Standard Model (SM). If we insist that new physics (NP) has to emerge in the TeV region, we need to conclude that NP possesses a highly non-generic flavor structure (flavor problem). One of the reasonable solutions to the flavor problem is to introduce flavor symmetry hypothesis. U(3) flavor symmetry is the maximal flavor symmetry allowed by the SM gauge group, and it is known as the Minimal Flavor Violation hypothesis. U(2) is the corresponding subgroup acting only on the first two (light) generations, and shows a good agreement with Yukawa and CKM hierarchical structures. Interestingly, it is shown that U(2) has a good compatibility with the recent B-anomalies. On the other hand, LHC results so far show that there is a mass gap between the SM spectrum and NP. It has motivated the systematic Effective Field Theory (EFT) approach. In this talk, after a brief review of U(3) and U(2) flavor symmetry, I will show how these flavor symmetries act on the SMEFT, providing an organizing principle to classify the large number of dimension-six operators involving fermion fields. The phenomenological study focusing on B-anomalies will be also discussed.
References
JHEP 08 (2020) 166, e-Print: 2005.05366 [hep-ph]
Phys.Lett.B 800 (2020) 135080, e-Print: 1909.02519 [hep-ph]
Kinya Oda, Tokyo Woman's Christian University
New effect in wave-packet scatterings of quantum fields: Saddle points, Lefschetz thimbles, and Stokes phenomenon
Online (Zoom), indico page, slides (kek.jp only)
We find a new contribution in wave-packet scatterings, which has been overlooked in the standard formulation of S-matrix. As a concrete example, we consider a two-to-two scattering of light scalars ϕ by another intermediate heavy scalar Φ, in the Gaussian wave-packet formalism: ϕϕ→Φ→ϕϕ. This contribution can be interpreted as an “in-time- boundary effect” of Φ for the corresponding Φ→ϕϕ decay, proposed by Ishikawa et al., with a newly found modification that would cure the previously observed ultraviolet divergence. We show that such an effect can be understood as a Stokes phenomenon in an integral over complex energy plane: The number of relevant saddle points and Lefschetz thimbles (steepest descent paths) discretely changes depending on the configurations of initial and final states in the scattering.
Xin-Li Sheng, Central China Normal Univ.
[QCD theory Seminar] From Kadanoff-Baym to Boltzmann equations for massive spin-1/2 fermions
Online (Zoom)
The quark-gluon plasma (QGP) generated in high-energy heavy-ion collisions is the most vortical system human ever made. The orbital angular momentum of the system will be converted into spin polarization of quarks during the evolution of the QGP. In this work, we use a matrix-valued distribution function for massive spin-1/2 fermions. The diagonal part of this distribution is the particle number density and the remaining parts are spin polarization density in the rest frame. From the Kadanoff-Baym equation, we derive Boltzmann equations for the matrix-valued distribution function, where nonlocal collision terms appear at next-to-leading order in space-time gradient. The nonlocal terms contribute as sources for the spin polarization part of the matrix-valued distribution function. The Boltzmann equations we obtained pave the way for numerically simulating spin-transport processes involving spin-vorticity coupling.
Ryohei Kobayashi, ISSP, The University of Tokyo
Interacting fermionic topological phases with time reversal symmetry
Online (Zoom) https://kds.kek.jp/event/37875/
In this talk, we discuss a recipe to produce a lattice construction of fermionic topological phases of matter on unoriented spacetime, which plays a crucial role to study topological phases or anomalies based on the time reversal symmetry. As an application, we construct a gapped boundary for a large class of fermionic SPT phases protected by finite onsite symmetry, based on our path integral description in the presence of boundaries. We will also formulate a local path integral for the (1+1)d topological superconductor in class BDI classified by Z8, and discuss its application to the problem of finding non-local order parameter for the Z8 classification if time permits.
Jan Pawlowski, Heidelberg University
Emergent Hadrons and Diquarks
online (Zoom) indico page, slides (kek.jp only)
We discuss the emergence of a low-energy effective theory with quarks, mesons, diquarks and baryons at vanishing and finite baryon density from first principle QCD. The present work also includes an overview on diquarks at vanishing and finite density, and elucidates the physics of transitional changes from baryonic matter to quark matter including diquarks. This set-up is discussed within the functional renormalisation group approach with dynamical hadronisation. In this framework it is detailed how mesons, diquarks, and baryons emerge dynamically from the renormalisation flow of the QCD effective action. Moreover, the fundamental degrees of freedom of QCD, quarks and gluons, decouple from the dynamics of QCD below the respective mass gaps. The resulting global picture unifies the different low energy effective theories used for low and high densities within QCD, and allows for a determination of the respective low energy constants directly from QCD.
Hidetoshi Taya, RIKEN
[QCD Theory Seminar] How time-dependent electric fields affect the Schwinger mechanism?
Online (Zoom) The Schwinger mechanism, the vacuum pair production in the presence of strong electric fields, is one of the most remarkable predictions of strong-field QED. For a constant electric field, it was established by Schwinger in 1951 that the vacuum pair production is driven by quantum tunneling and the resulting production number is non-perturbatively suppressed. The constant electric field configuration is, however, too idealistic. Strong electric fields that may be realized in actual physical situations (e.g., intense lasers and heavy-ion
The Schwinger mechanism, the vacuum pair production in the presence of strong electric fields, is one of the most remarkable predictions of strong-field QED. For a constant electric field, it was established by Schwinger in 1951 that the vacuum pair production is driven by quantum tunneling and the resulting production number is non-perturbatively suppressed. The constant electric field configuration is, however, too idealistic. Strong electric fields that may be realized in actual physical situations (e.g., intense lasers and heavy-ion
collisions) must be time- (as well as space-) dependent. Thus, we need to go beyond Schwinger’s constant-field result.
In this talk, I discuss how time-dependence affects the vacuum pair production based on my works. In particular, I plan to discuss (1) the interplay between non-perturbative and perturbative pair production mechanisms and show that the widely-used Keldysh parameter is not the only parameter that controls the interplay [1, 2]; (2) dynamically assisted Schwinger mechanism and Franz-Keldysh effect in strong-field QED based on the perturbation theory in the Furry picture [3]; and (3) spin and chirality production by time-depending electric fields [4, 5, 6].
Refs:
[1] HT, H. Fujii, K. Itakura, PRD 90, 014039 (2014) [2] HT, T. Fujimori, T. Misumi, M. Nitta, N. Sakai, JHEP 03, 082 (2021) [3] HT, PRD 99, 056006 (2019) [4] X.-G. Huang, M. Matsuo, HT, PTEP 2019, 113B02 (2019) [5] X.-G. Huang, HT, PRD 100, 016013 (2019) [6] HT, PRR 2, 023257 (2020)
Sunao Sugiyama, IPMU, University of Tokyo
Exploring Dark Matter Candidates with Microlensing
Online (Zoom), indico page, slides (kek.jp only)
I will talk about constraints on dark matter (DM) candidates, especially primordial black hole (PBH), with optical microlensing search. Microlensing is a gravitational lensing phenomenon, caused purely by the gravitational effect, and is a powerful tool for studying the nature of dark matter. MACHO, Kepler, OGLE and Subaru HSC, have explored dark matter candidates until now. My project is to utilize current/future dataset of HSC to test various dark matter candidates, and to develop more sophisticated analysis method to study the nature of dark matter further. PBH is a viable candidate of dark matter, and has received attention these days, because it could also explain the counterparts of LIGO GW binary BH systems and the seed of super massive black holes that exist at nuclei of every galaxy. I will talk about a new PBH model proposed by us to account for these events as well as DM at the same time, and forecast of constraint on this model with HSC.
Nodoka Yamanaka, Kennesaw State University
[EX] Electric dipole moment and CP violation in many-body systems
Online (Zoom) The electric dipole moment (EDM) is an attractive experimental probe of CP violation beyond the standard model, and it may be measured in many systems such as the muon, neutron, atoms, and molecules.
The electric dipole moment (EDM) is an attractive experimental probe of CP violation beyond the standard model, and it may be measured in many systems such as the muon, neutron, atoms, and molecules.
An important physics to be understood is the many-body effect relating the elementary level (TeV scale) CP violation and the final EDM of the composite system to be measured.
In this talk, I review the current understanding of the many-body physics relevant in the context of the EDMs, focussing on the enhancement and suppression of the CP violation, and see the prospects for the discovery of new physics beyond the standard model.
Lee Roberts, Boston University
[EX] Exploring Terra Incognita with the World’s Largest Penning Trap
Online (Zoom) The Standard Model provides a very precise prediction of the muon’s magnetic anomaly aμ = (gμ – 2)/2, the deviation from 2 of the gyromagnetic ratio gμ. In his seminal 1926 paper, P.A.M. Dirac predicted that for electrons ge = 2, but experiments then revealed that ge was slightly larger than 2. The reason was to be found in Quantum Mechanics, and the first radiative correction to ge , calculated by Julian Schwinger, explained a deviation of order 0.1 %. Today, the Standard Model predicts the value of aμ to a precision of ± 0.36 parts per million (ppm). Dedicated experiments have measured aμ to ± 0.35 ppm precision. Therefore, precision measurements of the anomaly provide a stringent test of the Standard Model’s completeness, since Nature knows about all forces that could contribute to the muon’s magnetism, including those from New Physics that has not yet been discovered.
