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Nuclear Matter and Heavy Ion Collisions (1989)

Nuclear Matter and Heavy Ion Collisions

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"Nuclear Matter and Heavy Ion Collisions" by Madeleine Soyeur is a astronomy book and space science reference focused on Cosmology. Best for students, researchers, and serious astronomy enthusiasts.

The Winter School "Nuclear Matter and Heavy Ion Collisions", a NATO Research Workshop held at Les Houches in February 89, has been devoted to recent developments in nuclear matter theory and to the study of central heavy ion collisions in which quasi macroscopic nuclear systems can be formed at various temperatures and densities. At in cident energies below 100 Me V per nucleon, the kinematic conditions are favourable for producing transient hot nuclei with temperatures of the order of a few MeV. At higher ener gies (100 MeV

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Best For: Researchers and students in nuclear physics and cosmology
Focus: Recent developments in nuclear matter theory and central heavy ion collisions
Covers: Theory of nuclear matter and experimental conditions in heavy ion collisions below 100 MeV per nucleon
Why It Matters: Provides insights into the formation of transient hot nuclear systems at varying temperatures and densities relevant to advanced nuclear physics studies

"Nuclear Matter and Heavy Ion Collisions" by Madeleine Soyeur is a astronomy book and space science reference focused on Cosmology. Best for students, researchers, and serious astronomy enthusiasts.

Topic: Cosmology

Author: Madeleine Soyeur

Who this is for:

  • Astronomy students
  • Researchers and advanced hobbyists
  • Readers exploring space science topics

Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.

The Winter School "Nuclear Matter and Heavy Ion Collisions", a NATO Research Workshop held at Les Houches in February 89, has been devoted to recent developments in nuclear matter theory and to the study of central heavy ion collisions in which quasi macroscopic nuclear systems can be formed at various temperatures and densities. At in cident energies below 100 Me V per nucleon, the kinematic conditions are favourable for producing transient hot nuclei with temperatures of the order of a few MeV. At higher ener gies (100 MeV

AuthorMadeleine Soyeur
PublisherSpringer
Published2012-03-07
ISBN-139781468457179
BindingPaperback
Pages511
LanguageEnglish
SubjectsScience
TopicCosmology
SeriesNATO Science Series B:

Format: Paperback

Length: 511 pages

Language: English

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