LEADER 03966nam 22006615 450 001 9910254576303321 005 20200701062114.0 010 $a3-319-63417-8 024 7 $a10.1007/978-3-319-63417-3 035 $a(CKB)4340000000061879 035 $a(DE-He213)978-3-319-63417-3 035 $a(MiAaPQ)EBC4922104 035 $a(PPN)203669746 035 $a(EXLCZ)994340000000061879 100 $a20170721d2017 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aManifestations of Dark Matter and Variations of the Fundamental Constants in Atoms and Astrophysical Phenomena /$fby Yevgeny V. Stadnik 205 $a1st ed. 2017. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2017. 215 $a1 online resource (XXI, 88 p. 22 illus., 18 illus. in color.) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 311 $a3-319-63416-X 320 $aIncludes bibliographical references. 327 $aIntroduction -- New Methods of Axion Dark Matter Detection -- New Methods of Scalar Dark Matter Detection -- New Spectroscopy Methods to Search for Anomalous Fifth-Forces -- Concluding Remarks. 330 $aThis thesis explores the possibility of searching for new effects of dark matter that are linear in g, an approach that offers enormous advantages over conventional schemes, since the interaction constant g is very small, g<<1. Further, the thesis employs an investigation of linear effects to derive new limits on certain interactions of dark matter with ordinary matter that improve on previous limits by up to 15 orders of magnitude. The first-ever limits on several other interactions are also derived. Astrophysical observations indicate that there is five times more dark matter?an ?invisible? form of matter, the identity and properties of which still remain shrouded in mystery?in the Universe than the ordinary ?visible? matter that makes up stars, planets, dust and interstellar gases. Conventional schemes for the direct detection of dark matter involve processes (such as collisions with, absorption by or inter-conversion with ordinary matter) that are either quartic (g4) or quadratic (g2) in an underlying interaction constant g. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aGravitation 606 $aAstronomy 606 $aAstrophysics 606 $aAtoms 606 $aPhysics 606 $aParticles (Nuclear physics) 606 $aQuantum field theory 606 $aClassical and Quantum Gravitation, Relativity Theory$3https://scigraph.springernature.com/ontologies/product-market-codes/P19070 606 $aAstronomy, Astrophysics and Cosmology$3https://scigraph.springernature.com/ontologies/product-market-codes/P22006 606 $aAtomic, Molecular, Optical and Plasma Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P24009 606 $aElementary Particles, Quantum Field Theory$3https://scigraph.springernature.com/ontologies/product-market-codes/P23029 615 0$aGravitation. 615 0$aAstronomy. 615 0$aAstrophysics. 615 0$aAtoms. 615 0$aPhysics. 615 0$aParticles (Nuclear physics) 615 0$aQuantum field theory. 615 14$aClassical and Quantum Gravitation, Relativity Theory. 615 24$aAstronomy, Astrophysics and Cosmology. 615 24$aAtomic, Molecular, Optical and Plasma Physics. 615 24$aElementary Particles, Quantum Field Theory. 676 $a530.1 700 $aStadnik$b Yevgeny V$4aut$4http://id.loc.gov/vocabulary/relators/aut$0823081 906 $aBOOK 912 $a9910254576303321 996 $aManifestations of Dark Matter and Variations of the Fundamental Constants in Atoms and Astrophysical Phenomena$91831948 997 $aUNINA