The equation of state of hot dense matter, including the occurrence of phase transitions, is of growing important in physics with the increase in laboratory experiments under high static and dynamic pressure; and in astrophysics as the observations, for example helioseismological measurements of the solar plasma to a new degree of precision, have f
Read More
The equation of state of hot dense matter, including the occurrence of phase transitions, is of growing important in physics with the increase in laboratory experiments under high static and dynamic pressure; and in astrophysics as the observations, for example helioseismological measurements of the solar plasma to a new degree of precision, have f
Read Less
Add this copy of Equation-of-State and Physe-Transition Issues in Models to cart. $213.83, new condition, Sold by Media Smart rated 4.0 out of 5 stars, ships from Hawthorne, CA, UNITED STATES, published 2004 by American Institute of Physics.
