Abstract
Why is ordinary matter (e.g., atoms, molecules, people, planets, stars) as stable as it is? Why is it the case, if an atom is thought to be a miniature solar system, that bringing very large numbers of atoms together (say 10 30) does not produce a violent explosion? Sometimes explosions do occur, as when stars collapse to form supernovae, but normally matter is well behaved. In short, what is the peculiar mechanics of the elementary particles (electrons and nuclei) that constitute ordinary matter so that the material world can have both rich variety and stability?
| Original language | English (US) |
|---|---|
| Title of host publication | The Stability of Matter |
| Subtitle of host publication | From Atoms to Stars: Fourth Edition |
| Publisher | Springer Berlin Heidelberg |
| Pages | 11-59 |
| Number of pages | 49 |
| ISBN (Print) | 3540420835, 9783540222125 |
| DOIs | |
| State | Published - Jan 1 2005 |
All Science Journal Classification (ASJC) codes
- Physics and Astronomy(all)