17.–21. Sept. 2025
Erice
Europe/Berlin Zeitzone

Role of Hadron Structure in EoS of Dense Matter and Consequences for Neutron Stars

Nicht eingeplant
40m
Lecture Hall San Domenico

Lecture Hall San Domenico

Talk Lectures

Sprecher

ANTHONY THOMAS (University of Adelaide)

Beschreibung

The nature of nuclear matter at the huge densities associated with neutron stars is not known. One certainly expects very large scalar and vector fields which may be expected to affect the structure of hadrons in such a medium. We explore ideas about the possible effects and thier consequences.

Autor

ANTHONY THOMAS (University of Adelaide)

Präsentationsmaterialien

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