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Manifestations of Dark Matter and Variations of the Fundamental Constants in Atoms and Astrophysical Phenomena
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(Buch) |
Dieser Artikel gilt, aufgrund seiner Grösse, beim Versand als 3 Artikel!
| Lieferstatus: |
 Auf Bestellung (Lieferzeit unbekannt) |
| Veröffentlichung: |
August 2018
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| Genre: |
Naturwissensch., Medizin, Technik |
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astronomy /
Astronomy, Astrophysics and Cosmology /
Astronomy, Cosmology and Space Sciences /
Astrophysics /
Atomic & molecular physics /
Atomic, Molecular, Optical and Plasma Physics /
Atoms /
B /
Classical and Quantum Gravitation, Relativity Theory /
Classical and Quantum Gravity /
Elementary particles (Physics) /
Elementary Particles, Quantum Field Theory /
Gravitation /
Physics /
Physics and Astronomy /
Quantum field theory /
Quantum physics (quantum mechanics & quantum field theory) /
Relativity physics /
Theoretical & mathematical astronomy |
| ISBN: |
9783319875507 |
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EAN-Code:
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9783319875507 |
| Verlag: |
Springer Nature EN |
| Einband: |
Kartoniert |
| Sprache: |
English
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| Serie: |
Springer Theses |
| Dimensionen: |
H 235 mm / B 155 mm / D |
| Gewicht: |
186 gr |
| Seiten: |
88 |
| Illustration: |
XXI, 88 p. 22 illus., 18 illus. in color., schwarz-weiss Illustrationen, farbige Illustrationen |
| Zus. Info: |
Previously published in hardcover |
| Bewertung: |
Titel bewerten / Meinung schreiben
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| Inhalt: |
| This thesis explores the possibility of searching for new effects of dark matter that are linear in g, an approach that offers enormous advantages over conventional schemes, since the interaction constant g is very small, g<<1. Further, the thesis employs an investigation of linear effects to derive new limits on certain interactions of dark matter with ordinary matter that improve on previous limits by up to 15 orders of magnitude. The first-ever limits on several other interactions are also derived. Astrophysical observations indicate that there is five times more dark matter-an 'invisible' form of matter, the identity and properties of which still remain shrouded in mystery-in the Universe than the ordinary 'visible' matter that makes up stars, planets, dust and interstellar gases. Conventional schemes for the direct detection of dark matter involve processes (such as collisions with, absorption by or inter-conversion with ordinary matter) that are either quartic (g4) or quadratic (g2) in an underlying interaction constant g. |
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