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Wolfgang Kapferer - The Mystery of Dark Matter In Search of the Invisible

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Wolfgang Kapferer The Mystery of Dark Matter In Search of the Invisible
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Book cover of The Mystery of Dark Matter Astronomers Universe Series - photo 1
Book cover of The Mystery of Dark Matter
Astronomers' Universe
Series Editor
Martin Beech
Campion College, The University of Regina, Regina, SK, Canada

The Astronomers Universe series attracts scientifically curious readers with a passion for astronomy and its related fields. In this series, you will venture beyond the basics to gain a deeper understanding of the cosmosall from the comfort of your chair.

Our books cover any and all topics related to the scientific study of the Universe and our place in it, exploring discoveries and theories in areas ranging from cosmology and astrophysics to planetary science and astrobiology.

This series bridges the gap between very basic popular science books and higher-level textbooks, providing rigorous, yet digestible forays for the intrepid lay reader. It goes beyond a beginners level, introducing you to more complex concepts that will expand your knowledge of the cosmos. The books are written in a didactic and descriptive style, including basic mathematics where necessary.

More information about this series at http://www.springer.com/series/6960

Wolfgang Kapferer
The Mystery of Dark Matter
In Search of the Invisible
1st ed. 2021
Logo of the publisher Wolfgang Kapferer Telfs Austria ISSN 1614-659X - photo 2
Logo of the publisher
Wolfgang Kapferer
Telfs, Austria
ISSN 1614-659X e-ISSN 2197-6651
Astronomers' Universe
ISBN 978-3-662-62201-8 e-ISBN 978-3-662-62202-5
https://doi.org/10.1007/978-3-662-62202-5
The translation was done with the help of artificial intelligence (machine translation by the service DeepL.com). A subsequent human revision was done primarily in terms of content.
Springer-Verlag GmbH Germany, part of Springer Nature 2021
This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed.
The use of general descriptive names, registered names, trademarks, service marks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use.
The publisher, the authors and the editors are safe to assume that the advice and information in this book are believed to be true and accurate at the date of publication. Neither the publisher nor the authors or the editors give a warranty, expressed or implied, with respect to the material contained herein or for any errors or omissions that may have been made. The publisher remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.

Binding illustration: Wolfgang Kapferer

Responsible Editor: Lisa Edelhaeuser

This Springer imprint is published by the registered company Springer-Verlag GmbH, DE part of Springer Nature.

The registered company address is: Heidelberger Platz 3, 14197 Berlin, Germany

Foreword

Today, the concept of dark matter has undergone an exciting two and a half centuries of history. From initially postulated dark stars to understand the strange movements of some luminaries on the firmament, to hypothetical planets in the outer reaches of our solar system, time and again it was possible to wrest matter from its darkness and, with advancing observation techniques, to discover its true nature.

At the beginning of the twentieth century however, a large gap regarding the masses of large-scale structures in the universe derived by various methods was discovered. The larger the structures, the greater the difference between masses derived from direct observations and masses derived from the dynamics of these objects. The successful conceptdark matterwas and is an approach to resolve this contradiction. It calls for an all-encompassing, purely gravitationally interacting substance in the universe, which is otherwiseat least until nowcompletely invisible. This concept of hidden matter that only reveals itself to us indirectly was and is very successful. A well known example of this is the theory of the formation and development of large-scale structures in the cosmos.

To the layman however, this concept often seems erratic and arbitrary. The aim of this book is, on the one hand, to show the great historical successes of the concept of dark matter in astronomy. The most important key observations in this field of research and their interpretations will be presented. These numerous observations have led to a world view in which our universe is mainly dominated by a form of matter as yet unknown to us. On the other hand, the potential candidates for dark matter are also presented, and the reader is familiarized with the great experiments in this highly topical field of research, the search for them and the most promising results to date.

The search for the nature of dark matter resembles a quest of the grail, transported into the modern age of the natural sciences. The book cover is dedicated to this parable. It shows the artistic visualization of a simulated galaxy rotation curve, which resembles a chalice when it is mirrored and rotated accordingly. In the course of the book, you will learn that galaxy rotation curves are among the central key observations for the phenomenon of dark matter and how laborious the search for a satisfactory answer to the question of the nature of this matter is. I hope you find this search as exciting as I do.

Wolfgang Kapferer
Telfs
June 2017
Contents
Springer-Verlag GmbH Germany, part of Springer Nature 2021
W. Kapferer The Mystery of Dark Matter Astronomers' Universe https://doi.org/10.1007/978-3-662-62202-5_1
1. Introduction
Wolfgang Kapferer
(1)
Telfs, Austria
Wolfgang Kapferer
Email:
If you search for answers to the question What is dark matter? in the information source of our time, the Internet, you will be well served quantitatively. The simple question What is dark matter? entered into a common Internet search engine will bombard you with about 20million hits in a flash. I admit not to have read all pages found, but after a short review of the list of results, one must assume that dark matter is most probably something
  • invisible,

  • mysterious,

  • dominant,

  • to be believed in,

These are all attributes that are difficult to combine with the methods of natural science. It quickly becomes clear that almost all large structures in the universe, such as galaxies, groups of galaxies and clusters of galaxies, predominantly consist of dark matter. And one learns in several treatises that no dark matter has yet been found directly on Earth or by space probes within our solar system. One reads that it must be a form of matter that hardly resembles the matter we are familiar with. It is so weakly interacting that it permeates every material in our world, almost without any sign of interaction with the elements we know. The adverb

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