Constraints on bosonic dark matter from ultralow-field nuclear magnetic resonance [PDF]
CASPEr-ZULF offers a new way to search for ultralight dark matter using ultralow-field nuclear magnetic resonance. The nature of dark matter, the invisible substance making up over 80% of the matter in the universe, is one of the most fundamental ...
Antoine Garcon +11 more
semanticscholar +1 more source
Tensile strength prediction of orthogonal CFRP under high intensity CW laser irradiation
Considering the two most important factors, delamination and tensile strength temperature dependence, a tensile strength prediction model for orthogonal carbon fiber reinforced polymer (CFRP) under continuous wave (CW) laser irradiation is proposed.
Jiawei Wang +6 more
doaj +1 more source
Search for Axionlike Dark Matter with a Liquid-State Nuclear Spin Comagnetometer. [PDF]
We report the results of a search for axionlike dark matter using nuclear magnetic resonance (NMR) techniques. This search is part of the multifaceted Cosmic Axion Spin Precession Experiment program.
Teng Wu +11 more
semanticscholar +1 more source
Measurement of the 52Fe mass via the precise proton-decay energy of 53Com
The proton decay of 53Com(3174.1 keV; 19/2−) was investigated via the fragmentation of a 58Ni primary beam. The proton-decay energy was determined with an improved precision to be 1558(8) keV.
Shen Yangping +34 more
doaj +1 more source
In this paper, a method to obtain the CuInGaSe2 (CIGS) absorber layer with an appropriate selenium content is put forward, in which a Se-rich target is used to deposit a CIGS thin-film and this film is annealed in a Se-free inert atmosphere.
Qiang Ma +6 more
doaj +1 more source
Warming nuclear pasta with dark matter: kinetic and annihilation heating of neutron star crusts [PDF]
Neutron stars serve as excellent next-generation thermal detectors of dark matter, heated by the scattering and annihilation of dark matter accelerated to relativistic speeds in their deep gravitational wells.
Javier F. Acevedo +3 more
semanticscholar +1 more source
Hyperonic Interactions in Neutron Stars
The matter of neutron stars is characterised by the density of the order of typical nuclear densities; hence, it can be described with methods of nuclear physics.
Semyon Mikheev +3 more
doaj +1 more source
Constraining the nuclear matter equation of state around twice saturation density [PDF]
Using FOPI data on elliptic flow in Au + Au collisions between 0.4 and 1.5 A GeV we extract constraints for the equation of state (EOS) of compressed symmetric nuclear matter using the transport code IQMD by introducing an observable describing the ...
Y. Leifels +4 more
semanticscholar +1 more source
Combined Constraints on the Equation of State of Dense Neutron-rich Matter from Terrestrial Nuclear Experiments and Observations of Neutron Stars [PDF]
Within the parameter space of the equation of state (EOS) of dense neutron-rich matter limited by existing constraints mainly from terrestrial nuclear experiments, we investigate how the neutron star maximum mass Mmax > 2.01 ± 0.04 M⊙, radius 10.62 km ...
Nai-Bo Zhang, Bao-An Li, Jun Xu
semanticscholar +1 more source
Soliton matter as a model of dense nuclear matter [PDF]
We employ the hybrid soliton model of the nucleon consisting of a topological meson field and deeply bound quarks to investigate the behavior of the quarks in soliton matter as a function of density. To organize the calculation, we place the solitons on a spatial lattice.
Glendenning, N.K., Banerjee, B.
openaire +3 more sources

