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The Search for Ultralight Bosonic Dark Matter

Derek F. Jackson Kimball - Personal Name; Viceconti - Personal Name; Karl van Bibber - Personal Name;

To set the stage for our study of ultralight bosonic dark matter (UBDM),
we review the evidence for the existence of dark matter: galactic and stellar
dynamics, gravitational lensing studies, measurements of the cosmic microwave
background radiation (CMB), surveys of the large-scale structure of the universe,
and the observed abundance of light elements. This diverse array of observational
evidence informs what we know about dark matter: its universal abundance, its
spatial and velocity distribution, and that its explanation involves physics beyond the
Standard Model. But what we know about dark matter is far outweighed by what we
do not know. We examine UBDM in the context of several of the most prominent
alternative hypotheses for the nature of dark matter: weakly interacting massive
particles (WIMPs), sterile neutrinos, massive astrophysical compact halo objects
(MACHOs), and primordial black holes (PBHs). Finally we examine some of the
key general characteristics of UBDM, including its wavelike nature, coherence
properties, and couplings to Standard Model particles and fields.


Availability
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220123032
Available
Detail Information
Series Title
-
Call Number
-
Publisher
: Springer Cham., 2023
Collation
XX, 363
Language
English
ISBN/ISSN
9783030958527
Classification
-
Content Type
-
Media Type
computer
Carrier Type
online resource
Edition
-
Subject(s)

The Search
Ultralight Bosonic Dark Matter
Specific Detail Info
-
Statement of Responsibility
Viceconti Derek F. Jackson Kimball, Karl van Bibber
Other Information
Cataloger
angga
Source
-
Validator
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Digital Object Identifier (DOI)
https://link.springer.com/book/10.1007/978-3-030-95852-7
Journal Volume
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Journal Issue
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Subtitle
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Parallel Title
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