Description - The Evolution of Matter by Igor Tolstikhin
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.
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(247mm x 174mm x 29mm)
Cambridge University Press
Publisher: Cambridge University Press
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Author Biography - Igor Tolstikhin
Igor Tolstikhin was awarded a Ph.D. in geochemistry from the St Petersburg Mining Institute in 1966 and a D.Sc. from the Vernadsky Institute, Moscow, in 1975. He is currently a Senior Research Scientist at the Russian Academy of Sciences where his research has encompassed noble gases, radiogenic isotope geochemistry, isotope hydrology, and geochemical modelling. His more recent contributions include a chemical Earth model with wholly convective mantle. Jan Kramers was awarded a Ph.D. from the University of Berne in Switzerland in 1973 and went on to work in South Africa, the UK and Zimbabwe, before returning to the University of Berne, where he is currently Professor of Geochemistry in the Institute of Geological Sciences. Professor Kramer's research interests include mantle geochemistry (kimberlites, diamonds), the origin of Archaean continental crust, global radiogenic isotope systematics, early evolution of the Earth's atmosphere, and, more recently, palaeoclimate research using the speleotherm archive.