Speaker
Prof.
Azwinndini Muronga
(University of Johannesburg)
Apply to be<br> considered for a student <br> award (Yes / No)?
No
Abstract content <br> (Max 300 words)
Neutron stars are powerful laboratories for constraining the equation of state of dense nuclear matter. Many aspects of neutron star structure depend on specific equation of state parameters.
Because many aspects of equation of state including
symmetry and thermal properties are uncertain and not well constrained by experiments, it is important to develop an equation of state with easily adjustable parameters.The purpose of this presentation is to discuss the development of the nuclear matter equation of state for dense nuclear matter.
Would you like to <br> submit a short paper <br> for the Conference <br> Proceedings (Yes / No)?
Yes
Primary author
Prof.
Azwinndini Muronga
(University of Johannesburg)
