Neutron stars with dark energy. (22nd January 2015)

• Record Type: Journal Article
• Authors: Hess, P O; Rodríguez, I; Greiner, W; Boller, T
• Is Part Of: Journal of physics. Number 578(2015)
• Page Start: 012008
• Publication Date: 2015-01-22
• Subjects: Physics -- Congresses; 530.5
• DOI: 10.1088/1742-6596/578/1/012008
• Languages: English
• ISSNs: 1742-6588

Abstract

Abstract: After a short review on the possible experimental observations to verify pseudocomplex General Relativity, neutron stars as a particular object of interest are investigated. Dark energy is added to the structure of a neutron star, while for the nuclear part the chiral SU(3) model is used. For the coupling of matter to dark energy a special assumption is made. The consequences are discussed. We show that neutron stars of up to six solar masses are obtained, which already behave similar to a black hole.