January 17, 2021

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Dark Matter

Dark Matter
Author : Blake Crouch
Publisher : Ballantine Books
Release Date : 2017
Category : Fiction
Total pages :359
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"Extra Libris: Essays, Reader's Guides, and More"--Page [345].

Dark Matter

Dark Matter
Author : Debasish Majumdar
Publisher : CRC Press
Release Date : 2014-08-27
Category : Science
Total pages :269
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Dark Matter: An Introduction tackles the rather recent but fast-growing subject of astroparticle physics, encompassing three main areas of fundamental physics: cosmology, particle physics, and astrophysics. Accordingly, the book discusses symmetries, conservation laws, relativity, and cosmological parameters and measurements, as well as the astrophysical behaviors of galaxies and galaxy clusters that indicate the presence of dark matter and the possible nature of dark matter distribution. This succinct yet comprehensive volume: Addresses all aspects essential to the study of dark matter Explores particle candidates for cold dark matter beyond the theory of the standard model, providing examples of basic extensions and introducing theories such as supersymmetry and extra dimensions Explains—in simple text and mathematical formulations—calculation of the freeze-out temperature of a dark matter species and its relic density Provides theoretical background for dark matter scattering off a target, event rate calculation, and dark matter annihilation essential to study direct and indirect detection of dark matter Complete with a detailed review of the latest dark matter experiments and techniques, Dark Matter: An Introduction is an ideal text for beginning researchers in the field as well as for general readers with an inquisitive mind, as the important topic of astroparticle physics is treated both pedagogically and with deeper insight.

Dark Matter

Dark Matter
Author : J. Val Blain
Publisher : Nova Publishers
Release Date : 2006
Category : Science
Total pages :151
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It is generally believed that most of the matter in the universe is dark, i.e. cannot be detected from the light which it emits (or fails to emit). Its presence is inferred indirectly from the motions of astronomical objects, specifically stellar, galactic, and galaxy cluster/supercluster observations. It is also required in order to enable gravity to amplify the small fluctuations in the cosmic microwave background enough to form the large-scale structures that we see in the universe today. For each of the stellar, galactic, and galaxy cluster/supercluster observations the basic principle is that if we measure velocities in some region, then there has to be enough mass there for gravity to stop all the objects flying apart. Dark matter has important consequences for the evolution of the universe and the structure within it. According to general relativity, the universe must conform to one of three possible types: open, flat, or closed. The total amount of mass and energy in the universe determines which of the three possibilities applies to the universe. In the case of an open universe, the total mass and energy density (denoted by the Greek letter Ù) is less than unity. If the universe is closed, Ù is greater than unity. For the case where Ù is exactly equal to one the universe is "flat". This new book details leading-edge research from around the globe.

Baryonic Dark Matter

Baryonic Dark Matter
Author : D. Lynden-Bell,Gerry Gilmore
Publisher : Springer Science & Business Media
Release Date : 1990-03-31
Category : Science
Total pages :298
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The visible universe is a small perturbation on the material universe. Zwicky and Sinclair Smith in the 1930s gave evidence of invisible mass in the Coma and Virgo Clusters of Galaxies. Better optical data has only served to confound their critics and the X-ray data confirms that the gravitational potentials are many times larger than those predicted on the basis of the observed stars. Dynamical analyses of individual galaxies have found that significant extra mass is needed to explain their rotational velocities. On much larger scales, tens of megaparsecs, there is suggestive evidence that there is even more mass per unit luminosity. What is this non-luminous stuff of which the universe is made'? How much of it is there? Need there be only one kind of stuff? There are three basic possi bili ties:- all of it is ordinary (baryonic) matter, all of it is some other kind of (non-baryonic) matter, or some of it is baryonic and some is non-baryonic.

Trends in Dark Matter Research

Trends in Dark Matter Research
Author : J. Val Blain
Publisher : Nova Publishers
Release Date : 2005
Category : Science
Total pages :227
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It is generally believed that most of the matter in the universe is dark, i.e. cannot be detected from the light which it emits (or fails to emit). Its presence is inferred indirectly from the motions of astronomical objects, specifically stellar, galactic, and galaxy cluster/supercluster observations. It is also required in order to enable gravity to amplify the small fluctuations in the cosmic microwave background enough to form the large-scale structures that we see in the universe today. For each of the stellar, galactic, and galaxy cluster/supercluster observations the basic principle is that if we measure velocities in some region, then there has to be enough mass there for gravity to stop all the objects flying apart. Dark matter has important consequences for the evolution of the universe and the structure within it. According to general relativity, the universe must conform to one of three possible types: open, flat, or closed. The total amount of mass and energy in the universe determines which of the three possibilities applies to the universe. In the case of an open universe, the total mass and energy density (denoted by the Greek letter Ù) is less than unity. If the universe is closed, Ù is greater than unity. For the case where Ù is exactly equal to one the universe is "flat". This new book details leading-edge research from around the globe.

Dark Sky, Dark Matter

Dark Sky, Dark Matter
Author : J.M Overduin,P.S Wesson
Publisher : CRC Press
Release Date : 2002-09-01
Category : Science
Total pages :216
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Olbers' paradox states that given the Universe is unbounded, governed by the standard laws of physics, and populated by light sources, the night sky should be ablaze with light. Obviously this is not so. However, the paradox does not lie in nature but in our understanding of physics. A Universe with a finite age, such as follows from big-bang theor

Dark Matter in Astro- and Particle Physics

Dark Matter in Astro- and Particle Physics
Author : Hans Volker Klapdor-Kleingrothaus,R. D. Viollier
Publisher : Springer Science & Business Media
Release Date : 2002
Category : Science
Total pages :663
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The search for Dark Matter in the Universe has established itself as one of the most exciting and central fields of astrophysics, particle physics and cosmology. The lectures and talks in this book emphasize the experimental and theoretical status and future perspectives, stressing in particular the interplay between astro- and particle physics.

Dark Matter

Dark Matter
Author : Sheree R. Thomas
Publisher : Aspect
Release Date : 2004-01-02
Category : Fiction
Total pages :416
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Dark Matter is the first and only series to bring together the works of black SF and fantasy writers. The first volume was featured in the "New York Times," which named it a Notable Book of the Year.

Dark Matter in Astro- and Particle Physics

Dark Matter in Astro- and Particle Physics
Author : Germany) Dark 200 (2000 Heidelberg,Hans Volker Klapdor-Kleingrothaus
Publisher : Springer Science & Business Media
Release Date : 2001
Category : Science
Total pages :740
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Dark matter in the Universe has become one of the most exciting and central fields of astrophysics, particle physics and cosmology. The lectures and talks in this book emphasize the experimental and theoretical status and perspectives of the ongoing search for dark matter, and the future potential of the field into the next millennium, stressing in particular the interplay between astro- and particle physics.

The Dark Matter Problem

The Dark Matter Problem
Author : Robert H. Sanders
Publisher : Cambridge University Press
Release Date : 2010-04-22
Category : Science
Total pages :129
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Most astronomers and physicists now believe that the matter content of the Universe is dominated by dark matter: hypothetical particles which interact with normal matter primarily through the force of gravity. Though invisible to current direct detection methods, dark matter can explain a variety of astronomical observations. This book describes how this theory has developed over the past 75 years, and why it is now a central feature of extragalactic astronomy and cosmology. Current attempts to directly detect dark matter locally are discussed, together with the implications for particle physics. The author comments on the sociology of these developments, demonstrating how and why scientists work and interact. Modified Newtonian Dynamics (MOND), the leading alternative to this theory, is also presented. This fascinating overview will interest cosmologists, astronomers and particle physicists. Mathematics is kept to a minimum, so the book can be understood by non-specialists.

The Identification of Dark Matter

The Identification of Dark Matter
Author : Neil J. C. Spooner,Vitaly Kudryavtsev
Publisher : World Scientific
Release Date : 2001
Category : Science
Total pages :637
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The objective of the workshop series ?The Identification of Dark Matter? is to assess critically the status of work attempting to identify what constitutes dark matter; in particular, to consider what techniques are currently being used, how successful they are, and what new techniques are likely to improve the prospects for identifying dark matter candidates in the future. This proceedings volume includes reviews on major particle astrophysics topics in the field of dark matter, as well as short contributed papers.

Progress in Dark Matter Research

Progress in Dark Matter Research
Author : J. Val Blain
Publisher : Nova Publishers
Release Date : 2005
Category : Science
Total pages :255
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It is generally believed that most of the matter in the universe is dark, i.e. cannot be detected from the light which it emits (or fails to emit). Its presence is inferred indirectly from the motions of astronomical objects, specifically stellar, galactic, and galaxy cluster/supercluster observations. It is also required in order to enable gravity to amplify the small fluctuations in the cosmic microwave background enough to form the large-scale structures that we see in the universe today. For each of the stellar, galactic, and galaxy cluster/supercluster observations the basic principle is that if we measure velocities in some region, then there has to be enough mass there for gravity to stop all the objects flying apart. Dark matter has important consequences for the evolution of the Universe and the structure within it. According to general relativity, the Universe must conform to one of three possible types: open, flat, or closed. The total amount of mass and energy in the universe determines which of the three possibilities applies to the Universe. In the case of an open Universe, the total mass and energy density (denoted by the Greek letter Omega) is less than unity. If the Universe is closed, Omega is greater than unity. For the case where Omega is exactly equal to one the Universe is "flat". This book details leading-edge research from around the globe.

Sources and Detection of Dark Matter and Dark Energy in the Universe

Sources and Detection of Dark Matter and Dark Energy in the Universe
Author : David B. Cline
Publisher : Springer Science & Business Media
Release Date : 2013-03-09
Category : Science
Total pages :544
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Dark matter research is one of the most fascinating and active fields among current high-profile scientific endeavours. It holds the key to all major breakthroughs to come in the fields of cosmology and astroparticle physics. The present volume is particularly concerned with the sources and the detection of dark matter and dark energy in the universe and will prove to be an invaluable research tool for all scientists who work in this field.

Dark Matter

Dark Matter
Author : Jean Audouze,J. Thanh Van Tran
Publisher : Atlantica Séguier Frontières
Release Date : 1988
Category : Cosmology
Total pages :498
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Our Universe Via Drexler Dark Matter

Our Universe Via Drexler Dark Matter
Author : Jerome Drexler
Publisher : Universal-Publishers
Release Date : 2009
Category : Science
Total pages :283
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This book is different from all other modern cosmology books in several ways. It introduces a cosmologic universe, which is orderly, logical, and systematic. It teaches and explains by illustrating how a variety of cosmic mysteries have been solved. It raises the status of dark matter in the universe by illuminating its roles as the principal source of energy, the principal source of matter in the form of hydrogen and helium, and the principal source of cosmic relationships with the principal cosmic phenomena of the universe. This book simplifies the universe as Nicolaus Copernicus' book simplified the solar system in 1543. With more and more cosmic mysteries being discovered and the slow progress in solving them, cosmologists and astrophysicists must re-train themselves to understand and to utilize the postmodern unified astrophysical cosmology model and to maximize the knowledge derived from the astronomical data. These are the three principal objectives of this book.