I-Love-Q universal relations remain valid within about 1% for neutron stars whose equation of state includes a coupled dark energy fluid in Lambda-CDM and quintessence-like models.
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I-Love-Q relations for Neutron Stars with Dark Energy
I-Love-Q universal relations remain valid within about 1% for neutron stars whose equation of state includes a coupled dark energy fluid in Lambda-CDM and quintessence-like models.