Hadron Ion Tea (HIT) Seminar Series
[formerly the Heavy Ion Tea Seminars]
Nuclear Science Division
Lawrence Berkeley National Laboratory
[formerly the Heavy Ion Tea Seminars]
Nuclear Science Division
Lawrence Berkeley National Laboratory
Organizers: Yuxun Guo, Yuuka Kanakubo, Felipe Ortega, Mateusz Ploskon, Bigeng Wang and Zhenyu Ye (Contact us at hit-organizers@lbl.gov)
Previous seminars can be viewed on our HIT Youtube Channel
Welcome to our Hadron-Ion Tea Seminar Series in 2026! All talks are available on zoom, some are in-person as well - we hope you join us!
Mar. 10, 2026 (In person)
Prof. Keh-Fei Liu
Location: Swiatecki Lounge B70 annex - 228
Time: 4:00pm Pacific Time
ZOOM for those who are unable to come in-person: LINK
Host: Yuuka Kanakubo
Title: Pressure-Energy Equations of State of Hadrons, Superconductor
Vortices, and the Cosmos
Abstract: The pressure–energy relations in the nucleon are derived from the
gravitational form factors, which parameterize matrix elements of the
energy-momentum tensor (EMT), together with EMT conservation. The static
pressure distribution arising from the Lorentz trace part of the EMT, as
manifested in the spatial stress $\frac{1}{3} T^{ii}$, equals minus the
corresponding trace part of the energy density, which can be understood
in terms of the gluon and quark condensates. It can be shown that this
trace-anomaly- and sigma-term-induced pressure plays a fundamental role
in the confinement dynamics of QCD. In contrast, the dynamic pressure
distribution from the traceless part of the spatial stress tensor equals
$1/d$ of the corresponding traceless part of the energy density, where
$d$ is the spatial dimension. We point out that the same pressure–energy
relations also hold for vortices in type-II superconductors, where the
static pressure–energy relation originates from the Cooper-pair
condensate. Furthermore, identical equations of motion appear in the
$\Lambda{\rm CDM}$ model of cosmology, where the static pressure–energy
relation arises from the cosmological constant.
Mar. 17, 2026 (In person)
Dr. Julian Kahlbow
Location: Room 328, Birge Hall, UC Berkeley Campus MAP
Time: 4:00pm Pacific Time
ZOOM for those who are unable to come in-person: LINK
Host: Shujie Li
Title: Probing nuclear correlations with high-energy hadronic reactions
Abstract: The atomic nucleus is a complex many-body system fundamentally rooted in QCD, yet effectively described by protons and neutrons at adequate scale. We use high-energy reactions to probe nucleon correlations at long and short range. However, extracting ground-state information is inherently challenged by initial- and final-state interactions. In this talk, I will discuss leveraging single-nucleon knockout reactions in inverse and hard kinematics to study single-particle behavior and short-range nucleon-nucleon correlations (SRCs). I will present results from JINR and GSI-FAIR using (p,2p) reactions with a 12C beam at a few GeV/nucleon. The results indicate a scale-dependent interpretation of nuclear structure. Additionally, I will report the first SRC measurements using a radioactive 16C beam. These results will enable future SRC studies across the nuclear chart.
[postponed]
Prof. Jen-Chieh Peng (University of Illinois at Urbana-Champaign)
Location: Swiatecki Lounge B70 annex - 228
Time: 4:00pm Pacific Time
ZOOM for those who are unable to come in-person: LINK
Host: Keh-Fei Liu
Title: Evolution of Helicity Property of Relic Neutrinos and Implications
on Their Detection
Abstract: Neutrinos in the early Universe decoupled essentially in helicity eigenstates.
As they propagate through the Universe, their helicities could be modified via
two effects. First, neutrinos with a finite magnetic moment would rotate their
spins with respect to their momenta as they encounter cosmic magnetic fields,
modifying their helicities. Second, the bending of neutrino's spin by a
gravitational field lags the bending of its momentum, again modifying its helicity.
We study both effects and investigate the implications of the
helicity modification on the detection of relic neutrinos using the Inverse
Tritium Beta Decay (ITBD) reaction. We find that the ITBD rate depends
sensitively on the neutrino mass hierarchy and on the Dirac or Majorana nature
of the neutrinos. This talk is based on several papers in collaboration with
Gordon Baym.