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Constraining hypernuclear density functional with Λ-hypernuclei and compact stars

  • We present a simultaneous calculation of heavy single-Λ hypernuclei and compact stars containing hypernuclear core within a relativistic density functional theory based on a Lagrangian which includes the hyperon octet and lightest isoscalar-isovector mesons which couple to baryons with density-dependent couplings. The corresponding density functional allows for SU(6) symmetry breaking and mixing in the isoscalar sector, whereby the departures in the σ–Λ and σ–Σ couplings away from their values implied by the SU(3) symmetric model are used to adjust the theory to the laboratory and astronomical data. We fix σ–Λ coupling using the data on the single-Λ hypernuclei and derive an upper bound on the σ–Σ from the requirement that the lower bound on the maximum mass of a compact star is 2M⊙.

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Metadaten
Author:Ellardus Nicolaas Eric van DalenGND, Giuseppe ColucciORCiDGND, Armen SedrakianORCiDGND
URN:urn:nbn:de:hebis:30:3-770186
DOI:https://doi.org/10.1016/j.physletb.2014.06.002
ISSN:0370-2693
Parent Title (English):Physics Letters B
Publisher:Elsevier
Place of publication:Amsterdam
Document Type:Article
Language:English
Date of Publication (online):2014/06/05
Date of first Publication:2014/06/05
Publishing Institution:Universitätsbibliothek Johann Christian Senckenberg
Release Date:2023/10/06
Tag:Equations of state: nuclear matter; Hypernuclei; Neutron stars
Volume:734
Page Number:5
First Page:383
Last Page:387
HeBIS-PPN:513579354
Institutes:Physik
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Sammlungen:Universitätspublikationen
Licence (German):License LogoCreative Commons - Namensnennung 3.0