Assessment of the progress in indentifying dark matter was the objective of the first "International Workshop on the Identification of Dark Matter", in particular to consider what techniques, both observational and experimental, are being used, how successful they are and what new techniques will improve the prospects of identifying the likely candidates. The meeting included reviews on major particle astrophysics topics in dark matter but was largely devoted to short contributed talks on new work in the field. This book offers the proceedings of the meeting.
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This review is from: The Identification of Dark Matter (Hardcover)
IDM98. I was a participant of the conference with the topic " The attenuated red giant stars as baryonic dark matter". The specific theme was 'Hubble Space Telescope of Mira cocoon stars as evidence of baryonic dark matter': The dark matter should be composed of the same type of matter as the common stars to be consistent with the established Universal laws and its was declareted in universal form at the IDM96. In scientific term, I think that this is the mostest and important conception to understand the genesis of the life in the Universe.
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Inside This Book
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Key Phrases - Statistically Improbable Phrases (SIPs):
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log frequency, cosmic decoherence, monoenergetic quarks, hydrocarbon shielding, standard halo model, magnet rotation frequency, dual phase detector, caustic ring radii, low background techniques, muon track length, wimp mass, nuclear recoil rate, electron recoil events, primary scintillation light, quasar light curves, nuclear recoil events, other existing uncertainties, sapphire bolometer, caustic rings, liquid xenon target, ring caustic, neutralino density, local dark matter density, dark matter paradigm, microlensing candidates Key Phrases - Capitalized Phrases (CAPs): (learn more)
Monte Carlo, Milky Way, Gran Sasso, World Scientific, Astroparticle Physics, Department of Physics, Physics Letters, Weakly Interacting Massive Particles, University of Sheffield, Germany E-mail, Standard Model, High Energy Phys, University of Zaragoza, Physics Department, Canfranc Underground Laboratory, Castle Ringberg, Stockholm University, Nuclear Physics, International Workshop, North Yorkshire, Nuovo Cim, University of Tokyo, Big Bang, Local Group, Imperial College London New!
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log frequency, cosmic decoherence, monoenergetic quarks, hydrocarbon shielding, standard halo model, magnet rotation frequency, dual phase detector, caustic ring radii, low background techniques, muon track length, wimp mass, nuclear recoil rate, electron recoil events, primary scintillation light, quasar light curves, nuclear recoil events, other existing uncertainties, sapphire bolometer, caustic rings, liquid xenon target, ring caustic, neutralino density, local dark matter density, dark matter paradigm, microlensing candidates Key Phrases - Capitalized Phrases (CAPs): (learn more)
Monte Carlo, Milky Way, Gran Sasso, World Scientific, Astroparticle Physics, Department of Physics, Physics Letters, Weakly Interacting Massive Particles, University of Sheffield, Germany E-mail, Standard Model, High Energy Phys, University of Zaragoza, Physics Department, Canfranc Underground Laboratory, Castle Ringberg, Stockholm University, Nuclear Physics, International Workshop, North Yorkshire, Nuovo Cim, University of Tokyo, Big Bang, Local Group, Imperial College London New!
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Citations (learn more)
24
books
cite this book:
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- Sources and Detection of Dark Matter and Dark Energy in the Universe: Fourth International Symposium Held at Marina del Rey, CA, USA February 23-25, 2000 by David B. Cline on 5 pages
- Cryogenic Particle Detection by Christian Enss on page 355, and page 356
- Technique and Application of Xenon Detectors: Proceedings of the International Workshop, University of Tokyo, Japan, 3-4 December, 2001 by Y. Suzuki on page 92, and page 176
- Stellar Collapse (Astrophysics and Space Science Library) by Chris L. Fryer on page 131
- Origins of Existence: How Life Emerged in the Universe by Fred Adams in Back Matter
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