FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2807769507> ?p ?o ?g. }

• W2807769507 endingPage "72" @default.
• W2807769507 startingPage "72" @default.
• W2807769507 abstract "High-density nuclear symmetry energy is of crucial importance in astrophysics. Information on such energy has been obtained from mass–radius determinations of neutron stars (NSs), and in the future NS mergers will increasingly contribute. In the laboratory, the symmetry energy can be studied in heavy-ion collisions (HICs) at different incident energies over a large range, from very low to several times higher saturation density. Transport theory is necessary to extract the symmetry energy from the typically non-equilibrated nuclear collisions. In this contribution, we first review the transport approaches, their differences, and recent studies of their reliability. We then discuss several prominent observables, which have been used to determine the symmetry energy at high density: collective flow, light cluster emission, and particle production. It is finally argued that the results of the symmetry energy from microscopic many-body calculations, nuclear structure, nuclear reactions, and astrophysics begin to converge but still need considerable improvements in terms of accuracy." @default.
• W2807769507 created "2018-06-21" @default.
• W2807769507 creator A5035936678 @default.
• W2807769507 date "2018-06-14" @default.
• W2807769507 modified "2023-09-26" @default.
• W2807769507 title "The High-Density Symmetry Energy in Heavy-Ion Collisions and Compact Stars" @default.
• W2807769507 cites W1967959012 @default.
• W2807769507 cites W1973689270 @default.
• W2807769507 cites W1974455323 @default.
• W2807769507 cites W1978618029 @default.
• W2807769507 cites W1984609518 @default.
• W2807769507 cites W1985752314 @default.
• W2807769507 cites W1991102973 @default.
• W2807769507 cites W1996268188 @default.
• W2807769507 cites W2001069305 @default.
• W2807769507 cites W2001632885 @default.
• W2807769507 cites W2012430171 @default.
• W2807769507 cites W2016975306 @default.
• W2807769507 cites W2018298698 @default.
• W2807769507 cites W2020692504 @default.
• W2807769507 cites W2023120691 @default.
• W2807769507 cites W2024112767 @default.
• W2807769507 cites W2024320182 @default.
• W2807769507 cites W2026166712 @default.
• W2807769507 cites W2032332167 @default.
• W2807769507 cites W2036225851 @default.
• W2807769507 cites W2042825346 @default.
• W2807769507 cites W2043039259 @default.
• W2807769507 cites W2047213274 @default.
• W2807769507 cites W2052784716 @default.
• W2807769507 cites W2055068132 @default.
• W2807769507 cites W2057551049 @default.
• W2807769507 cites W2061964942 @default.
• W2807769507 cites W2079136448 @default.
• W2807769507 cites W2084001590 @default.
• W2807769507 cites W2092350553 @default.
• W2807769507 cites W2106036896 @default.
• W2807769507 cites W2106558292 @default.
• W2807769507 cites W2108064387 @default.
• W2807769507 cites W2110764800 @default.
• W2807769507 cites W2115139593 @default.
• W2807769507 cites W2119734739 @default.
• W2807769507 cites W2125418715 @default.
• W2807769507 cites W2140559132 @default.
• W2807769507 cites W2146020709 @default.
• W2807769507 cites W2147917528 @default.
• W2807769507 cites W2151676963 @default.
• W2807769507 cites W2153430156 @default.
• W2807769507 cites W2157284909 @default.
• W2807769507 cites W2160339942 @default.
• W2807769507 cites W2201776064 @default.
• W2807769507 cites W2272518768 @default.
• W2807769507 cites W2332004489 @default.
• W2807769507 cites W2508860606 @default.
• W2807769507 cites W2516674350 @default.
• W2807769507 cites W2592231571 @default.
• W2807769507 cites W2766013620 @default.
• W2807769507 cites W2766627241 @default.
• W2807769507 cites W2767400734 @default.
• W2807769507 cites W2768265440 @default.
• W2807769507 cites W2768432612 @default.
• W2807769507 cites W2772938691 @default.
• W2807769507 cites W3100881821 @default.
• W2807769507 cites W3104773239 @default.
• W2807769507 cites W3104946210 @default.
• W2807769507 cites W3105880739 @default.
• W2807769507 doi "https://doi.org/10.3390/universe4060072" @default.
• W2807769507 hasPublicationYear "2018" @default.
• W2807769507 type Work @default.
• W2807769507 sameAs 2807769507 @default.
• W2807769507 citedByCount "5" @default.
• W2807769507 countsByYear W28077695072019 @default.
• W2807769507 countsByYear W28077695072020 @default.
• W2807769507 countsByYear W28077695072021 @default.
• W2807769507 crossrefType "journal-article" @default.
• W2807769507 hasAuthorship W2807769507A5035936678 @default.
• W2807769507 hasBestOaLocation W28077695071 @default.
• W2807769507 hasConcept C121332964 @default.
• W2807769507 hasConcept C150846664 @default.
• W2807769507 hasConcept C159985019 @default.
• W2807769507 hasConcept C165410206 @default.
• W2807769507 hasConcept C172695262 @default.
• W2807769507 hasConcept C185544564 @default.
• W2807769507 hasConcept C192562407 @default.
• W2807769507 hasConcept C192887742 @default.
• W2807769507 hasConcept C204323151 @default.
• W2807769507 hasConcept C206191943 @default.
• W2807769507 hasConcept C20892832 @default.
• W2807769507 hasConcept C2524010 @default.
• W2807769507 hasConcept C2779886137 @default.
• W2807769507 hasConcept C32848918 @default.
• W2807769507 hasConcept C33923547 @default.
• W2807769507 hasConcept C44870925 @default.
• W2807769507 hasConcept C54116275 @default.
• W2807769507 hasConcept C62520636 @default.
• W2807769507 hasConceptScore W2807769507C121332964 @default.
• W2807769507 hasConceptScore W2807769507C150846664 @default.
• W2807769507 hasConceptScore W2807769507C159985019 @default.

• next