Results 11 to 20 of about 1,482,374 (348)
On quintessence star model and strange star [PDF]
European Physical Journal C: Particles and Fields, 2020 The astronomical observations on the accelerated expansion of the universe generate the possibility that the internal matter of the stars is not only formed by ordinary matter but also by matter with negative pressure.
Gabino Estevez-Delgado +1 more
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The extended, relativistic hyperon star model [PDF]
Physical Review C, 2002 In this paper an equation of state of neutron star matter which includes strange baryons in the framework of Zimanyi and Moszkowski (ZM) model has been obtained.
.P.-G. Reinhard +31 more
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Converting neutron stars into strange stars: Instanton model [PDF]
International Journal of Modern Physics D, 2014 We calculate the quasiclassical probability to emerge the quantum fluctuation which gives rise to the quark-matter drop with interface propagating as the self-similar spherical detonation wave (DN) in the ambient nuclear matter. For this purpose, we make use of instanton method which is known in the quantum field theory.
Gurovich, Victor Ts., Fel, Leonid G.
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Symposium - International Astronomical Union, 1981 The current state of neutron star structure calculations is reviewed. Uncertainties in the equation of state for matter at and above nuclear density remain. The role of the delta resonance, pion condensates, and quark matter is reviewed. Despite uncertainties, we find that recent models yield stable neutron star masses which are consistent with ...
V. Canuto, Richard L. Bowers
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RJA-Star Algorithm for UAV Path Planning Based on Improved R5DOS Model
Applied Sciences, 2023 To improve the obstacle avoidance ability of agricultural unmanned aerial vehicles (UAV) in farmland settings, a three-dimensional space path planning model based on the R5DOS model is proposed in this paper. The direction layer of the R5DOS intersection
Jian Li +5 more
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A progeroid syndrome caused by a deep intronic variant in TAPT1 is revealed by RNA/SI‐NET sequencing
EMBO Molecular Medicine, 2023 Exome sequencing has introduced a paradigm shift for the identification of germline variations responsible for Mendelian diseases. However, non‐coding regions, which make up 98% of the genome, cannot be captured.
Nasrinsadat Nabavizadeh +20 more
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Symposium - International Astronomical Union, 1974 The properties of fully relativistic rotating hadron star models are discussed using models based on recently developed equations of state. All of these stable neutron star models are bound with binding energies as high as ∼ 25%. During hadron star formation, much of this energy will be released.
Jeffrey M. Cohen, Gerhard Börner
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Modern Physics Letters A, 1995 The star-matrix models are difficult to solve due to the multiple powers of the Vandermonde determinants in the partition function. We apply to these models a modified Q-matrix aprpoach and we get results consistent with those obtained by other methods.
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Monolithic or hierarchical star formation? A new statistical analysis [PDF]
, 1998 We consider an analytic model of cosmic star formation which incorporates supernova feedback, gas accretion and enriched outflows, reproducing the history of cosmic star formation, metallicity, supernovae type II rates and the fraction of baryons ...
Kampakoglou, Marios +2 more
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Early-forming Massive Stars Suppress Star Formation and Hierarchical Cluster Assembly
The Astrophysical Journal, 2023 Feedback from massive stars plays an important role in the formation of star clusters. Whether a very massive star is born early or late in the cluster formation timeline has profound implications for the star cluster formation and assembly processes. We
Sean C. Lewis +10 more
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