'Degenerate gas' presentation slideshows

Chapter two The physics of stellar interiors

Chapter two The physics of stellar interiors. 1. The pressures: --- equation of state of an ideal gas --- equation of state of a degenerate gas. 2. What is Opacity and its approximate form?. 3. Nuclear reactions in stars?. -- binding energy. -- Hydrogen and helium burning.

547 views • 34 slides

The structure and evolution of stars

The structure and evolution of stars. Lecture 12:White dwarfs, neutron stars and black holes. Learning Outcomes. The student will learn How to derive the equation of state of a degenerate gas How polytropic models can be applied to degenerate stars - white dwarfs

286 views • 27 slides

Stellar Evolution II

209 views • 19 slides