PaperPanorama

Nuclear Theory·nucl-th

Thursday·July 4, 2024

6 papers3 primary·3 cross-listed

  1. 01

    Nuclear shell model study of neutrinoless double beta decay under Left-Right symmetric model

    Dong-Liang Fang🇨🇳 · B. Alex Brown🇺🇸 · Fedor Šimkovic🇸🇰

    We use the large scale nuclear shell model to calculate the nuclear matrix elements for the neutrino mediated neutrinoless double beta decay within the Left-Right symmetric model for four nuclei: Ge, Se, Te and Xe. We perform a systematic analysis on the general magnitude of different terms for related mechanisms. For the mechanism, we find that the weak magnetism term dominates the decay rate while the -wave effect is suppressed. While for the mechanism, the and the terms are with equal importance. For the latter term, important contributions from weak-magnetism MM part are observed. Finally, we give the constraints on the new physics parameters , and from current experiments.

    nucl-thhep-phPRC(2024)·4 citations
  2. 02

    Two-cluster approach to the properties of one- and two-neutron-halo nuclei

    H. M. Maridi · Jagjit Singh · N. R. Walet · D. K. Sharp

    In this work, we present a new approximate method for obtaining simple wave functions for the ground state of exotic nuclei with a neutron halo. We model the system as a two-cluster structure, treating the core and halo as inert objects. The relative wave function is expressed as a combination of simple harmonic oscillator states, with the oscillator parameter determined from the separation energy. Since these wave functions lack the expected exponential decay, we introduce a simple multiplicative renormalization factor based on the nuclear root mean square radius. This approach, combining oscillator wave functions and the renormalization factor, is then applied to calculate dipole strength distributions and Coulomb dissociation cross section for several - and -halo nuclei. The results show excellent agreement with the available experimental data.

    nucl-thPRC(2025)·3 citations
  3. 03

    Assessing the joint effect of temperature and magnetic field on the neutron star equation of state

    Luigi Scurto · Valéria Carvalho · Helena Pais · Constança Providência

    In this work, we study the effect of strong magnetic fields on the equation of state (EoS) of warm, homogeneous, Neutron Star (NS) matter in beta equilibrium. NS matter is described within a relativistic mean field (RMF) approximation, including both models with non-linear meson terms or with density dependent nucleon-meson couplings. We first study the effect of magnetic fields and finite temperature on the EoS separately, finding that the effect of the latter to be significantly stronger than the one of the former. We then study the combined effect of magnetic fields and temperature on the internal composition. We show how both factors cause an increase in the proton fraction at low density and that, as long as the temperatures considered are not higher than 10 MeV, the effect of the magnetic field on the proton fraction is not small enough to be neglected.

    nucl-thPRC(2024)·9 citations
  4. 04

    Dissipative tidal effects to next-to-leading order and constraints on the dissipative tidal deformability using gravitational wave data

    Abhishek Hegade K. R.🇺🇸 · Justin L. Ripley🇺🇸 · Nicolás Yunes🇺🇸

    Dissipative tidal interactions can be used to probe the out-of-equilibrium physics of neutron stars using gravitational wave observations. In this paper, we present the first post-Newtonian (PN) corrections to the orbital dynamics of a binary system containing objects whose tidal interactions have a dissipative contribution. We derive the 1PN-accurate equations of motion in the center-of-mass frame and a generalized energy-balance law that is valid for dissipative tidal interactions. We show how mass and energy loss due to the absorption of orbital energy change the orbital dynamics and derive the next-to-leading order correction to the gravitational wave phase of a binary system in a quasi-circular orbit containing initially non-spinning components. We then use this waveform model to constrain, for the first time, the individual dissipative tidal deformabilities of each of the binary components that generated the GW170817 event using real data. We find that the GW170817 data requires and at 90\% confidence, where are the individual tidal deformabilities of the primary and secondary binary components that produced the GW170817 event.

    gr-qcnucl-thPRD(2024)·24 citations
  5. 05

    Properties of the QCD Matter -- An Experimental Review of Selected Results from RHIC BES Program

    Jinhui Chen · Xin Dong · Xionghong He · Huanzhong Huang · Feng Liu · Xiaofeng Luo · Yu-Gang Ma · Lijuan Ruan · Ming Shao · Shusu Shi · Xu Sun · Aihong Tang and 16 other authors

    In the paper, we discuss the development of the multi-gap resistive plate chamber Time-of-Flight (TOF) technology and the production of the STAR TOF detector in China at the beginning of the 21st century. Then we review recent experimental results from the first beam energy scan program (BES-I) at the Relativistic Heavy Ion Collider (RHIC). Topics cover measurements of collectivity, chirality, criticality, global polarization, strangeness, heavy-flavor, di-lepton and light nuclei productions.

    nucl-exhep-exnucl-thNucl.Sci.Tech.(2024)·203 citations
  6. 06

    Droplets of Bosons at a Narrow Resonance

    Ke Wang · Thimo Preis · Dam Thanh Son

    We consider bosons interacting through a narrow -wave resonance. Such a resonance is characterized by an infinite scattering length and a large and negative effective range . We argue that any number of bosons can form a self-bound cluster with the binding energy per particle increasing as for , where is the background scattering length (between atoms and molecules). In the opposite limit , bosons form droplets with binding energy per particle saturating to a constant value independent of the particle number. The stability of clusters and droplets when the interaction is detuned from the resonance is also studied.

    cond-mat.quant-gasnucl-thPRA(2025)·2 citations

Affiliations

first authorsco-authorsvia INSPIRE