This book concerns the discovery of S. Chandrasekar, that white dwarfs have a maximum mass (1.4 times the mass of the Sun) and how this was work was received by his fellow scientist, in particular by Sir Arthur Eddington. The conclusions drawn from Chandra's work was that more massive stars would continue to collapse until nothing is left (i.e. black holes would form; however, black holes were not yet discovered). It is in particular this aspect which Eddington and other scientist did not believe. Chandra's life in Cambridge and struggle(s) (such as his fights against racism) is well described. In the second part of the book, the author explains some aspects of the physics involved. Read this book and you will learn a lot about Chandra's life (which is fascinating) and the consequences of his work. The book is not meant to be about details of stellar evolution, white dwarfs, neutron stars and black holes. Readers who want to learn the physics in detail need to look elsewhere. However, the book describes very nicely an important chapter in the history of astrophysics. It will be of interest to everyone who has interest in astronomy/astrophysics.
|