Описание: Dark matter research is one of the most fascinating and active fields among current high-profile scientific endeavours. The present volume is particularly concerned with the sources and the detection of dark matter and dark energy in the universe and will prove to be an invaluable research tool for all scientists who work in this field.
List of Talks from DM 2012.- List of Attendees at DM 2012.- Brief Overview.- Theoretical Precision: Cosmology and Dark Matter.- Radiative natural supersymmetry with mixed axion/higgsino cold dark matter.- Finite Temperature density profile in SFD.- An argument for axion dark matter.- Supersymmetric Dark Matter at XENON100 and the LHC: No-Scale F-SU(5) Stringy Correlations.- Approaches on self-gravitating Bose-Einstein condensates.- Search for Turbulent Gas through Interstellar Scintillation.- Search for Dark Matter - LHC, CMB, Fermi LAT- The missing energy events at the LHC and implications for dark matter search.- Where is SUSY?- Bounds on dark matter from CMB observations- Searches for Galactic Dark Matter Substructure with the Fermi LAT- Current Search Results and New Detectors- DAMA.- Xenon100 Detector.- Xenon 1 Ton.- Super CDMS.- Antideuterons.- Light WIMPs.- Directional Detection.- Cogent.- Low-mass WIMPs.
This thesis presents several significant new results that shed light on two major puzzles of modern cosmology: the nature of inflation, the very early phase of the universe that is thought to have given rise to the large-scale structures that we observe today; and that of the current accelerated expansion. In particular, it develops a clean method for characterizing linear cosmological perturbations for general theories where gravity is modified and/or affected by a new component, called dark energy, responsible for the accelerated expansion. It proposes a new extension to what were long thought to be the most general scalar field theories devoid of instabilities, and demonstrates the robustness of the relation between the energy scale of inflation and the predicted amplitude of gravitational waves. Finally, it consolidates a set of consistency relations between correlation functions of the cosmological density field and investigates the phenomenological consequences of their potential violation. Presented in a clear, succinct and rigorous style, each of these original results is both profound and important and will leave a deep mark on the field.
Автор: Humitaka Sato; Hideo Kodama Название: Dark Matter in the Universe ISBN: 3642860311 ISBN-13(EAN): 9783642860317 Издательство: Springer Рейтинг: Цена: 15672.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: "Dark matter" was first introduced by Zwicky in 1933 to resolve a discrepancy be- tween the dynamical and luminous masses of the Coma cluster. Though it is now certain that dark matter constitutes a dominant part of the matter in the universe, its distribution and accurate abundance are not known well.
Автор: J. Kormendy; G.R. Knapp Название: Dark Matter in the Universe ISBN: 9027723575 ISBN-13(EAN): 9789027723574 Издательство: Springer Рейтинг: Цена: 12157.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: Proceedings of the 117th Symposium of the International Astronomical Union, held in Princeton, New Jersey, June 24-28, 1985
Автор: Sabino Matarrese; Monica Colpi; Vittorio Gorini; U Название: Dark Matter and Dark Energy ISBN: 9400735294 ISBN-13(EAN): 9789400735293 Издательство: Springer Рейтинг: Цена: 14365.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: Dark Matter and Dark Energy offers a compact introduction to cosmological perturbation theory - a fundamental ingredient to understanding dark matter and energy in the universe. Current developments in research and theory are presented.
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