Mari

Margueron, Jean-Claude

doi:10.2307/j.ctvh1dt7w

Cited by 24 publications

(4 citation statements)

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“…Nearly all of the presented ranges encompass the 11.6 to 12.6 km interval that follows from the two laboratory experiments measuring the elliptic flows in 197 Au+ 197 Au and the neutron skin of 48 Ca. It holds also for the analysis of Tews et al [79] presented at this conference [80]. A tighter lower limit for the deformability Λ has been reported by Radice et al [81].…”

Section: Neutron Star Radiisupporting

confidence: 70%

High density with elliptic flows

Trautmann¹

2019

AIP Conference Proceedings

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The elliptic flow of emitted particles and fragments observed in heavy-ion reactions at high energy has become an important observable reflecting the pressure generated in the dense collision zone. More recently, the strength of the nuclear symmetry energy has been investigated by measuring the ratios or differences of the elliptic flows exhibited by neutrons and charged particles in 197 Au+ 197 Au collisions at 400 MeV/nucleon incident energy at the GSI laboratory. A moderately soft to linear dependence on density was deduced for a range of densities shown to reach beyond twice the saturation value in these experiments. The known sources of uncertainties and possible model dependencies were thoroughly studied with transport models of the UrQMD and Tübingen QMD type.A new source of information on the nuclear equation of state at high density has opened up with the observation of the first LIGO and Virgo GW170817 gravitational wave signal from a neutron star merger. The quantitative comparison of terrestrial and celestial results on the basis of measured or inferred neutron star radii or core pressures, including those obtained from X-ray observations, reveals a rather satisfactory agreement. Depending on the precision that can be achieved with future measurements and observations, it will thus become possible to assess the validity of the applied models and methods. The perspectives for improved experiments at FAIR using the NeuLAND and KRAB detection systems are outlined. *

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Section: Neutron Star Radiisupporting

confidence: 70%

High density with elliptic flows

Trautmann¹

2019

AIP Conference Proceedings

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“…The coefficients c sat,α and c sym,α are related to the empirical parameters, e.g. E sat ≈ −16 MeV, n sat ≈ 0.16 fm −3 and K sat ≈ 230 MeV in nuclear matter, considering the relativistic extension of the meta-model (for the kinetic term only) [33]. The present calculation is based on the nucleon Skyrme interaction SLy4, on which the meta-model is adjusted.…”

Section: Energy Density and Derivativesmentioning

confidence: 99%

Quarkyonic stars with isospin-flavor asymmetry

Margueron,

Hansen,

Proust

et al. 2021

Preprint

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“…If it was intended to be put in the water, its likely berth was in the port, yet undiscovered, on the straight, wide canal linking Mari with the Euphrates. 65 What features of the Minoan ship(s) docked in the harbor of Ugarit impressed Zimri-Lim so deeply that he desired his own version? Here, it may be instructive to look first at the elements that Egyptians thought most identified "Keftiu boats, " that is, ships with Aegean home ports, or vessels they associated primarily with Aegean mariners.…”

Section: A Minoan Boatmentioning

confidence: 99%

Mari and the Minoans

Foster¹

2018

Groniek

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Mari

Cited by 24 publications

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High density with elliptic flows

High density with elliptic flows

Quarkyonic stars with isospin-flavor asymmetry

Mari and the Minoans

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