Continuum Lambda spectra for a 6LiLambda hypernucleus in the 6Li(K-, pi-) reactionWe theoretically investigate Lambda production via a (K-, pi-) reaction on a 6Li target, using the distorted-wave impulse approximation (DWIA) with a Fermi-averaged K-n --> pi-Lambda amplitude. We…Toru Harada, Yoshiharu Hirabayashi·May 11, 2025SaveLearn
Half-vortex states in the rotating outer core of neutron starsWe probe the superfluid-superconductor dynamics of the rotating outer core of neutron stars through half-vortex states. By means of a generalized hydrodynamic model, where proton and neutron fluids…J. A. Gil Granados, A. Muñoz Mateo, X. Viñas·May 10, 2025SaveLearn
Temperature-dependent nuclear partition functions and abundances in stellar interiorWe calculate temperature-dependent nuclear partition functions (TDNPFs) and nuclear abundances for 728 nuclei assuming nuclear statistical equilibrium (NSE). The theories of stellar evolution…Jameel-Un Nabi, Abdel Nasser Tawfik, Nada Ezzelarab et al.·May 10, 2025SaveLearn
Unique first-forbidden β-decay transitions in odd-odd and even-even heavy nucleiThe allowed Gamow-Teller (GT) transitions are the most common weak nuclear processes of spin-isospin (στ) type. These transitions play a key role in numerous processes in the domain of…Jameel-Un Nabi, Necla Cakmak, Muhammad Majid et al.·May 10, 2025SaveLearn
Phenomenology of baryon dynamics with directed flow in relativistic heavy-ion collisionsThis thesis aims to elucidate the role of initial baryon stopping and its diffusion in heavy-ion collisions (HIC) using hydrodynamic model. In this regard, we have studied the observable-directed…Tribhuban Parida·May 10, 2025SaveLearn
Synthesis of the superheavy elements beyond Og: extrapolating from 48Ca to 54CrTheoretical predictions on the optimal reaction energies are essential for producing superheavy elements (SHEs) beyond Og. Due to the limitation of the targets, synthesizing elements 119 and 120 will…Yueping Fang, Long Zhu·May 9, 2025SaveLearn
Order, Collectivity, Structured Yrast Lines, and Correlated Energies in Random Bosonic SystemsSignatures of order and collectivity appear in a broad range of one and two level boson systems. Toy systems of N particles on a single j=3,\,4… 7 level, and on 2 levels (j1,\,j2) with…Declan Mulhall·May 8, 2025SaveLearn
Comparison of integral equations used to study Tcc+ for a stable D*We perform a detailed comparison between three formalisms used in recent studies of DD* scattering, which aim to understand the properties of the doubly-charmed tetraquark, Tcc+(3875). These…Sebastian M. Dawid, Fernando Romero-López, Stephen R. Sharpe·May 8, 2025SaveLearn
Manifest Gauge Invariance for Structure Dependent Radiative Corrections to Processes Involving Atoms and NucleiRadiative corrections to reactions involving atoms or nuclei can become sensitive to the structure of the bound state. Generically, one encounters correlation functions of multiple currents which…Ryan Plestid, Mark B. Wise·May 8, 2025SaveLearn
Insights into Neutron Star Matter: EoS Models and ObservationsThe equation of state (EoS) for neutron stars is a crucial topic in astrophysics, nuclear physics, and quantum chromodynamics (QCD), influencing their structure, stability, and observable properties.…Zuhua Ji, Jiarui Chen, Yan Chen·May 8, 2025SaveLearn
The candidates of 2α condensate around the 16O nucleus studied by the real-time evolution methodBackground: Searching for alpha condensation around a core nucleus, a new class of nuclear clustering, is an interesting topic. Previous theoretical studies predicted 16O + 2α condensed…Y. M. Htet, T. Oishi, M. Kimura et al.·May 8, 2025SaveLearn
Point-proton density distributions of stable nucleiPoint-proton density distributions are deduced for 130 stable nuclei from 7Li to 232Th from nuclear charge densities determined in elastic electron scattering. There are…Tianyu Wu, Baohua Sun, Huihui Xie et al.·May 8, 2025SaveLearn
Heisenberg Uncertainty Inequality and Breaking of Isospin Symmetry in Atomic NucleiThe Heisenberg uncertainty inequality is used to derive a rigorous lower bound to the amount of isospin impurities in N=Z atomic nuclei, caused by the violation of isospin symmetry. The bound is…Sandro Stringari·May 7, 2025SaveLearn
Perturbation theory for a systematic account of the bound-state motionWe derive a perturbation theory (PT) for the Lorentz boost operator in the space of two-nucleon wave functions. The latter is expressed in terms of the nucleon-nucleon (NN) potentials, developed so…Alexander N. Kvinikhidze, Hagop Sazdjian, Boris Blankleider·May 6, 2025SaveLearn
Shear viscosity and electrical conductivity of rotating quark matter in Nambu--Jona-Lasinio ModelThe Lagrangian for strongly interacting and rotating quark matter is modified with the inclusion of the spinorial connections, which in turn affect the thermodynamic equation of state and transport…Ashutosh Dwibedi, Dushmanta Sahu, Jayanta Dey et al.·May 6, 2025SaveLearn
Parameterizations of Electron Scattering Form Factors for Elastic Scattering and Electro-Excitation of Nuclear States for 27Al and 40CaWe report on empirical parameterizations of longitudinal ( RL) and transverse ( RT) nuclear electromagnetic form factors for elastic scattering and the excitations of nuclear states…Arie Bodek, M. E. Christy, Zihao Lin et al.·May 6, 2025SaveLearn
Nuclear structure and weak rates of heavy waiting point nuclei under rp-process conditionsThe structure and the weak interaction mediated rates of the heavy waiting point (WP) nuclei 80Zr, 84Mo, 88Ru, 92Pd and 96Cd along N = Z line were studied within the…Jameel-Un Nabi, Mahmut Boyukata·May 6, 2025SaveLearn
Gamow-Teller strength and lepton captures rates on 66-71Ni in stellar matterCharge-changing transitions play a significant role in stellar weak-decay processes. The fate of the massive stars is decided by these weak-decay rates including lepton (positron and electron)…Jameel-Un Nabi, Muhammad Majid·May 6, 2025SaveLearn
Allowed and unique first-forbidden stellar electron emission rates of neutron-rich copper isotopesThe allowed charge-changing transitions are the most common weak interaction processes of spin-isospin form that play a crucial role in several nuclear/astrophysical processes. The first-forbidden…Muhammad Majid, Jameel-Un Nabi, Gul Daraz·May 6, 2025SaveLearn
Thermal properties of zero sound in asymmetric nuclear matterThe zero-sound modes at finite temperature are investigated with the relativistic random phase approximation to signal the uncertainty of the equation of state (EOS) of asymmetric nuclear matter. It…Jing Ye, Wei-Zhou Jiang·May 6, 2025SaveLearn
Relativistic dissipative hydrodynamics for particles of arbitrary massEmploying a kinetic framework, we calculate all transport coefficients for relativistic dissipative (second-order) hydrodynamics for arbitrary particle masses in the 14-moment approximation. Taking…Semyon Potesnov, David Wagner·May 6, 2025SaveLearn
Dynamical coupled-channel models for hadron dynamicsDynamical coupled-channel (DCC) approaches parametrize the interactions and dynamics of two and more hadrons and their response to different electroweak probes. The inclusion of unitarity, three-body…Michael Döring, Johann Haidenbauer, Maxim Mai et al.·May 5, 2025SaveLearn
Transverse momentum fluctuations as a probe of thermalization and collective dynamics of QGPWe study fluctuations of mean transverse momentum per particle ([pT]) in ultrarelativistic heavy-ion collisions. We show that the steep fall in the variance of transverse momentum fluctuation in…Rupam Samanta, Tribhuban Parida·May 5, 2025SaveLearn
Constraining the neutron star equation of state by including the isoscalar-vector and isovector-vector coupling using the Bayesian analysisWe constrain the nuclear matter equation of state within the relativistic mean field model by including the isoscalar-vector and isovector-vector coupling term at a fundamental level using the…Deepak Kumar, Pradip Kumar Sahu·May 5, 2025SaveLearn
Probing potential via its v2 flow in hypernuclei-induced reactionThe hyperon potential, particularly its behavior at high densities, is crucial for resolving the ``hyperon puzzle'' in neutron stars and for advancing our understanding of the strong interactions…Gao-Chan Yong·May 5, 2025SaveLearn