The Evolution of Matter
From the Big Bang to the Present Day

This volume follows the chemical history of matter from the Big Bang to the present.

Igor Tolstikhin (Author), Jan Kramers (Author)

9780521866477, Cambridge University Press

Hardback, published 12 June 2008

532 pages
25.3 x 18 x 2.9 cm, 1.19 kg

'Overall, The Evolution of Matter is a good, deep and readable combination of the textbook and monograph, which brought under one cover a link between cosmo- and geochemistry; solar system formation and evolution; Earth's core, crust and mantle. It also combines a description of sophisticated geodynamic models with considerable cosmo-geochemical reference information.' Pure and Applied Geophysics

The Evolution of Matter explains how all matter in the Universe developed following the Big Bang and through subsequent stellar processes. It describes the evolution of interstellar matter and its differentiation during the accretion of the planets and the history of the Earth. Unlike many books on geochemistry, this volume follows the chemical history of matter from the very beginning to the present, demonstrating connections in space and time. It provides also solid links from cosmochemistry to the geochemistry of Earth. The book presents comprehensive descriptions of the various isotope systematics and fractionation processes occurring naturally in the Universe, using simple equations and helpful tables of data. With a glossary of terms and over 900 references, this volume is a valuable reference for researchers and advanced students studying the chemical evolution of the Earth, the Solar System and the wider Universe.

Introduction
Part I. The Elements: 1. Isotopes – weights and abundances
2. Introduction to the universe – the baryonic matter
3. Element and isotope abundances – reference collection
4. Cosmological nucleosynthesis – production of H and He
5. Stellar nucleosynthesis – lower mass stars and s-process
6. Stellar nucleosynthesis – r- and associated processes
7. Timing of stellar nucleosynthesis
8. Chemical evolution of the galaxy
Part II. Early Solar System – Nebula Formation, Evolution and Lifetime: 9. Introduction to the solar nebula
10. The primary solar system objects and related processes
11. Chondritic meteorites
12. Highly processed meteorites
13. A summary of early solar system chronology
Part III. Accretion of the Earth: 14. Introduction to the planetary system, earth and moon
15. Introduction to planetary accretion
16. Earth accretion – the giant impact(s)
17. The post-accretion silicate earth – comparison with meteorites
18. Core segregation
19. Heavy 'crust' on the top of the core
20. The early atmo-hydrophere
21. Light from the moon…
Part IV. Global Evolution of the Earth: 22. First look on the Earth
23. The plate tectonic concept – some phenomenology
24. Oceanic ridge and island magmatism
25. Subduction and island arc magmatism
26. Composition of the continental crust – magmatic, metamorphic and sedimentary processes
27. Isotopic records of the evolution of the earth's accessible reservoirs
28. Geochemical earth model
References
Glossary
Abbreviations
List of meteorites, rocks and minerals
Index.

Subject Areas: Materials science [TGM], Geochemistry [RBGK], Chemistry [PN]