Discriminating hadronic and quark stars through gravitational waves of fluid pulsation modes [PDF]
, 2013 We investigate non-radial oscillations of hadronic, hybrid and pure self-bound strange quark stars with maximum masses above the mass of the recently observed massive pulsars PSR J1614-2230 and PSR J0348-0432 with $M \approx 2 M_{\odot}$.
Flores, C. V., Lugones, G.
core +1 more source
Radial stability of anisotropic strange quark stars [PDF]
, 2016 The influence of the anisotropy in the equilibrium and stability of strange stars is investigated through the numerical solution of the hydrostatic equilibrium equation and the radial oscillation equation, both modified from their original version to ...
J. Arbañil, J. Arbañil, M. Malheiro
semanticscholar +1 more source
Heavy hadrons spectra on lattice using NRQCD
EPJ Web of Conferences, 2018 Comparison of radial excitation energies to masses show that the velocity of b quark is very non-relativistic in bottomonium states. In a mixed system like charmed B meson, the b quark has less velocity than it has in bottomonium states and in strange B ...
Mohanta Protick, Basak Subhasish
doaj +1 more source
Electric transitions of the charmed-strange mesons in a relativistic quark model
European Physical Journal C: Particles and Fields, 2020 In the present work, we adopt a relativistic constituent quark model to depict the charmed strange meson spectroscopy, in which $$D_{s0}(2317)$$ Ds0(2317) and $$D_{s1}(2460)$$ Ds1(2460) are considered as the $$1^3P_0$$ 13P0 and $$1P_1^\prime $$ 1P1 ...
Shao-Feng Chen +3 more
doaj +1 more source
Effects of density-dependent quark mass on phase diagram of three-flavor quark matter
, 2005 Considering the density dependence of quark mass, we investigate the phase transition between the (unpaired) strange quark matter and the color-flavor-locked matter, which are supposed to be two candidates for the ground state of strongly interacting ...
Li Xue-Qian, M. Alford, Zhang Xiao-Bing
core +1 more source
Light Quark Masses with Dynamical Wilson Fermions [PDF]
, 1997 We determine the masses of the light and the strange quarks in the $\bar{MS}$-scheme using our high-statistics lattice simulation of QCD with dynamical Wilson fermions. For the light quark mass we find $m^{light}_{\bar{MS}}(2 GeV) = 2.7(2) MeV$, which is
A Spitz +23 more
core +3 more sources
Massive charged-current coefficient functions in deep-inelastic scattering at NNLO and impact on strange-quark distributions [PDF]
, 2017 A bstractWe present details on calculation of next-to-next-to-leading order QCD corrections to massive charged-current coefficient functions in deep-inelastic scattering.
Jun Gao
semanticscholar +1 more source
Searching for Strange Quark Matter Objects in Exoplanets [PDF]
, 2017 The true ground state of hadronic matter may be strange quark matter (SQM). Consequently, observed pulsars may actually be strange quark stars, but not neutron stars.
Y. F. Huang, Y. B. Yu
semanticscholar +1 more source
Is distinct location evidence of distinct objects? Multilocation and the problem of parsimony
Analytic Philosophy, Volume 66, Issue 3, Page 394-401, September 2025.Abstract For an object to be multilocated is for it to wholly occupy disjoint spatial regions simultaneously. If multilocation is possible, it is possible that a multilocated particle is wholly located at 1080 distinct locations, such that it constitutes a particle‐for‐particle duplicate of the actual universe.
David Harmon
wiley +1 more source
Properties of strange quark stars with isovector interactions
Physics Letters B, 2020 We study the properties of strange quark stars by employing a 3-flavor Nambu-Jona-Lasinio model with both scalar-isovector and vector-isovector interactions.
He Liu, Jun Xu, Che Ming Ko
doaj +1 more source