PPT-Dark Matter

Author : trish-goza | Published Date : 2016-03-30

Axion Dark Matter Georg G Raffelt MaxPlanck Institut f ür Physik München Physics Colloquium University of Sydney 3 March 2014 Axions as Cold Dark Matter of

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Dark Matter: Transcript


Axion Dark Matter Georg G Raffelt MaxPlanck Institut f ür Physik München Physics Colloquium University of Sydney 3 March 2014 Axions as Cold Dark Matter of the Universe Dark . Not in compact objects (brown dwarfs, etc.). Baryons should also contribute to . nucleosynthesis. But we got it to work out assuming it’s . not. baryons. Most likely: it will be some sort of undiscovered particle: . Susan Cartwright. University of Sheffield. Neutrinos and the Universe. Discovering neutrinos. Detecting neutrinos. Neutrinos and the Sun. Neutrinos and Supernovae. Neutrinos and Dark Matter. Neutrinos and the Universe. Fabio Bossi . INFN-LNF. Talking about «dark light» may seem an oximore. We naturally connect the idea of darkness with that of absence of light. . In our macroscopic everyday’s world this is in fact correct, not only from the point of view of our instinctive perception but also from that of a rigorous physical description of reality. . 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.. D.S. . Hajdukovic. GBAR Collaboration Meeting. 18. th. April 2012. Our best physics . The Standard Model of Particles and Fields. +. . General Relativity . is . considered. as insufficient to explain the observed phenomena in Astrophysics and Cosmology.. Ron-Chou Hsieh. CYCU. Outline. It seems to have something there!. What are they?. Link with physics beyond the SM.. DM searches.. Constructing a DM model. Summary. It seems to have something there!. Galactic rotation curves:. Paul McMillan. Surveys For All, 1st February 2016 . Why do we care?. On the biggest scales, the ΛCDM model works. Why do we care?. On the scale of individual galaxies, agreement is less obvious.. Things are more complicated, we have to consider the baryons. 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. National Science Foundation • Division of Astronomical Sciences . Prepared by the . Association of Universities for Research in Astronomy . SCIENCE. . PEOPLE TECHNOLOGY. Scientists Discover Galaxy that is 99.99 Percent Dark Matter. Prof. David Toback. Texas A&M . University. Mitchell Institute for . Fundamental Physics and Astronomy. March 2018. Gents of Texas A&M. Prologue. 2. We live in a . time of remarkable scientific . Gravity . and Light. Black Holes. What is Dark Matter?. Recap. Midterm . Friday . 11/. 1: summary review sheet posted. Canvas homework : . due Wednesday. Lab this week. Using . gravity to measure . masses. Cao Hoang Nam. Phenikaa. . University. Based on . arXiv. : 2007.xxx. ICISE - . Quy. Nhon, July 2020. Plan of the talk. GR+SM . and . m. otivations for beyond. Flipped . U(1) extended Standard Model and Majorana dark matter. LAPTh. IRN . Terascale. meeting . May 21. st. , 2019. Annecy. w. / . G. Bélanger. , . T. M. a. , . Y. Soreq. work. in . progress. 2. Dark Matter. c. ompelling. o. bservational. . evidence. . through . Niayesh Afshordi. Western University. Friday, April 13, 2012. “Friday . the 13th. . is a date considered to be bad luck in. . Western. . superstition. .” . -Wikipedia. . Outline. Introduction: Cold Dark Matter (CDM) .

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