422 papers
Nucl-Ex represents the dynamic frontier where scientists probe the fundamental building blocks of matter through high-energy experiments. By smashing particles together at incredible speeds or observing rare cosmic events, researchers uncover the forces that govern our universe and test the limits of our current understanding of physics.
At Gist.Science, we ensure these breakthroughs reach a broader audience by processing every new preprint in this field directly from arXiv. For each study, we provide both a clear, plain-language explanation of the core discoveries and a detailed technical summary for those seeking deeper insights. Below are the latest papers in nuclear experiment research, curated to help you stay informed on the latest developments from the lab.
This paper proposes a novel invariant-mass observable using the resonance to experimentally distinguish between nucleon coalescence and statistical thermal models for deuteron formation at the LHC, demonstrating that a specific resonance peak in the proxy mass spectrum emerges exclusively in the coalescence scenario.
This paper demonstrates through simulations and experiments at two research reactors that continuous-signal neutron noise analysis, utilizing pulse-shape deconvolution or detector pairs, effectively overcomes the dead-time and pile-up limitations of traditional pulse-counting to provide unbiased kinetic parameter estimation at high detection rates.
Using the - fast-timing technique with the VENTURE array at VECC, Kolkata, researchers measured the lifetimes of low-lying negative-parity states in Gd to determine that their transition strengths are strongly hindered, providing evidence for weak dipole strength in octupole bands.
This paper presents a direct measurement of the CuNi reaction cross section using the MUSIC detector at FRIB, which, combined with Bayesian model averaging, yields a revised astrophysical reaction rate that is systematically lower than previous evaluations and establishes the competing channel as the dominant uncertainty in the NiCu cycle.
This paper presents a high-precision, cost-effective laboratory technique using Associated Particle Imaging to measure neutron-induced gamma-ray production cross sections at 14 MeV, demonstrating its capability through proof-of-concept experiments on iron and carbon samples with uncertainties dominated by counting statistics that can be further reduced.
This paper presents a theoretical study using the TRENTo3D and CLVisc models with a novel initial longitudinal flow gradient to simultaneously describe STAR's global and azimuthal hyperon polarization measurements in isobaric Zr+Zr collisions, revealing that the azimuthal modulation is dominantly driven by shear effects while highlighting the challenges in achieving a unified description of all polarization observables.
This paper proposes that measuring the frequency of the asteroseismic crust-core interface mode in neutron stars, via resonant shattering flares or tidal resonances, can determine stellar radii to within 5–10% with minimal dependence on inner core physics, provided that low-density nucleonic matter is well-constrained.
This whitepaper proposes the Hyperon-Nucleon Spectrometer (H-NS) at the High-Intensity heavy-ion Accelerator Facility (HIAF) to systematically investigate the unresolved polarization puzzle through high-precision measurements of hyperon and proton spin observables across a wide range of collision energies and systems.
This study presents detailed projections demonstrating that the Electron-Ion Collider in China (EicC) can precisely measure pion and kaon structure functions via the Sullivan process with statistical uncertainties below 5% and 8%, respectively, thereby significantly advancing our understanding of meson parton distributions and bridging the gap between fixed-target and collider-era measurements.
A new direct measurement of the CuNi reaction using the MUSIC detector at FRIB reveals a systematically lower stellar rate than previously estimated, which significantly suppresses Ni-Cu cycle recycling in X-ray bursts while enhancing the efficiency of the p process in supernova nucleosynthesis.