PDF-(BOOK)-Introduction To Particle Dark Matter, An (Advanced Textbooks in Physics)

What is the dark matter that fills the Universe and binds together galaxies How was it produced What are its interactions and particle propertiesThe paradigm of dark matter is one of the key developments at the interface of cosmology and elementary particle physics It is also one of the foundations of the standard cosmological model This book presents the state of the art in building and testing particle models for dark matter Each chapter gives an analysis of questions research directions and methods within the field More than 200 problems are included to challenge and stimulate the readers knowledge and provide guidance in the practical implementation of the numerous tools of the trade presented Appendices summarize the basics of cosmology and particle physics needed for any quantitative understanding of particle models for dark matterThis interdisciplinary textbook is essential reading for anyone interested in the microscopic nature of dark matter as it manifests itself in particle physics experiments cosmological observations and highenergy astrophysical phenomena from graduate students and advanced undergraduates to cosmologists and astrophysicists interested in particle models for dark matter and particle physicists interested in earlyuniverse cosmology and highenergy astrophysics. ASPERA. 1. Roger Blandford. KIPAC. Stanford. One Hundred Years . of Cosmic Ray Physics . 21 xi 2011. ASPERA. 2. Roger Blandford. KIPAC. Stanford. …mi . ritrovai. per . una. . selva. . oscura. … . This . powerpoint. will show you the basics of dark matter and dark energy . Their place in the universe . By Jordan . Ilori. . DARK MATTER. Dark matter is a type of matter hypothesized in astronomy and cosmology to account for a large part of the mass that appears to be missing from the universe. Dark matter cannot be seen directly with telescopes; evidently it neither emits nor absorbs light or other electromagnetic radiation at any significant level. Instead, the existence and properties of dark matter are inferred from its gravitational effects on visible matter, radiation, and the large-scale structure of the universe. According to the Planck mission team, and based on the standard model of cosmology, the total mass–energy of the known universe contains 4.9% ordinary matter, 26.8% dark matter and 68.3% dark energy. Thus, dark matter is estimated to constitute 84.5% of the total matter in the universe and 26.8% of the total content of the universe.. Axion Dark Matter. Georg G. . Raffelt. , Max-Planck-. Institut. f. ür Physik, . München. Physics Colloquium, University of Sydney, 3 March 2014. Axions. as Cold Dark Matter of the Universe. Dark . Spring 2011. (Chapter 1: getting started). . the elementary particles. the forces. the model . how can we understand it?. Elementary particle: . an entity not able to be further decomposed. . with a unique set of properties. Wrap Up. The Volume of the Red Ball. An engineer, mathematician, and physicist are each asked to determine the volume of a red metal ball.. The mathematician measures the diameter, divides it by two to obtain the radius, and then performs a double . Isabel . Baransky. About Me. Sophomore at Columbia University's Engineering School (SEAS). Majoring in Applied Physics. Minoring. in Music. Volunteer at multiple teaching organizations. Peace by P.E.A.C.E. Introduction to Cosmology. Adel . A. wad. Centre for Theoretical Physics. British University. Content. Observed Universe. General Relativity and Cosmology. Cosmological Eras. Dark matter. Dark energy. Cody . Carr. , Minh Nguyen. December 9. th. , 2014.. Agenda. Motivations (Cosmic & Atomic scales). Dark Matter categories. The Dark Matter Zoo. Neutrinos. Neutralinos. Kaluza. -Klein particles. Summary. antimatter. ?. Susan Cartwright. The Standard Model of particle . physics contains 12 fundamental . particles. 9 of these have electric charge. It turns out that each of these particles has a corresponding antiparticle. Susan Cartwright. University of Sheffield. 1. Dark Matter. Astrophysical Evidence. Candidates. Detection. 2. The Astrophysical Evidence. Rotation curves of spiral galaxies. flat at large radii: if mass traced light we would expect them to be . Dr. Simona . Murgia. (UC, Irvine). Dr. Will Dawson (Lawrence Livermore National Laboratory). Carolyn Slivinski (STScI). Facilitator: Dr. Emma Marcucci (STScI). Science Briefing. October . 5. , 2017. . Dan Hooper . – . Fermilab. Saturday Morning Physics. What is Physics?. Physics is hard to define. Here are some definitions that I found in online dictionaries:. “. T. he . science that deals with matter, energy, motion, and force.. and LHC. :. la . grande. . sfida. . della. . Nuova. . Fisica. Antonio Masiero. Univ. di Padova e INFN. Univ. di Napoli, . Dipt. . Di . Fisica. , 15 . giugno. 2012. FCNC, CP ≠, (g-2), (. ). Cosmic Opportunities. . –. 45. th. SLAC Summer Institute. Jonathan . Feng. , UC Irvine. 16 August 2017. INTRODUCTION. We’ve learned a lot about the Universe. Dark . Matter: 23% . ± 4. %. Dark .