Direct detection experiments - PowerPoint PPT Presentation
Lecture 11 : Galaxies
Lecture 11 : Galaxies. Robert Fisher. Items. Nathan Hearn guest lecture on dark matter on April 20th. Lunch in the loop (on me) with Nathan following the lecture at Frontera Fresco for anyone who wants to join us.
By salene
Dark matter and hidden U(1) X
Dark matter and hidden U(1) X. (Work in progress, In collaboration with E.J. Chun & S. Scopel ) Park, Jong-Chul (KIAS) August 10, 2010 Konkuk University. Outline. Motivation Hidden U(1) X model and dark matter Constraints from EW precision Relic density and direct detection
By gella
Issues in hidden sector dark matter
Issues in hidden sector dark matter . Seungwon Baek (KIAS) Summer Institute 2013 Jirisan National Park, Aug . 17-23, 2013 based on JHEP1202; JHEP1211; JHEP1305 in collaboration with Pyungwon Ko , Wan-Il Park, Eibun Senaha. Outline.
By noel
Dark Matter Searches with the ATLAS detector Mono-ANYTHING ?
Dark Matter Searches with the ATLAS detector Mono-ANYTHING ?. ENIGMASS – 11.10.2012 Marie-Hélène Genest – LPSC ; Helenka Przysiezniak – LAPP. While astrophysical observations provide convincing proof for the existence of a non-baryonic dark component to the Universe
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Radio Detection Experiments
. A tale of two spectra
Exoplanets : direct detection
Exoplanets : direct detection. ASTR 1420 Lecture 17 Sections 11.2. Imaging planet is hard!. Direct imaging is very hard, because … tremendous brightness contrast ratio between stars and planets ( e.g.) Sun outshines Earth about 10 billion times
DEBUNKING NEUTRINO DETECTION EXPERIMENTS
DEBUNKING NEUTRINO DETECTION EXPERIMENTS. THE GHOSTLY NEUTRINOS. Hate them or love them, neutrinos do exist. Vector Particle Physics (VPP) automatically gives the correct structures and characteristics for the neutrinos.
Direct Detection of Dark Matter
Direct Detection of Dark Matter. Ankur Deep Bordoloi , Cristian Gaidau. Outline. Cold Dark Matter (WIMP hypothesis) Why? What? Direct detection techniques What to detect Detector types Cryogenic Dark Matter Detection Experimental method Results. Indirect means:.
Tensions in DM Direct Detection
2 nd Internationl Workshop on Particle Physics and Cosmology after Higgs and Plank. Qing Wang Tsinghua Univ. Beijing. Tensions in DM Direct Detection. Outline. √. Motivation & Status. Three old Exps : DAMA ； CRESST ； CoGeNT. Reconciliation Methods. Our Latest Result.
Neutrino mass and DM direct detection
Erice2013 21 Sept., 2013. Neutrino mass and DM direct detection. Daijiro Suematsu (Kanazawa Univ.). Based on the collaboration with S.Kashiwase PRD86 (2012) 053001, EPJC73 (2013) 2484. Outline. Motivation and ｂ a sic idea M odel and its features
Dark Matter Direct Detection roadmap strategy
Dark Matter Direct Detection roadmap strategy. G. Chardin, J. Jochum, A. Rubbia, N.Smith For the WG5 working group. Dark Matter and Dark Energy. Outstanding question : What is the Universe made of ?. Ordinary (baryonic) matter only represents only ≈ 4% of the Universe energy content.
micrOMEGAs_2.2 : direct detection and new models
micrOMEGAs_2.2 : direct detection and new models. G. Bélanger LAPTH. G. B, F. Boudjema, A. Pukhov, A. Semenov, hep-ph/0112278, hep-ph/0405253, hep-ph/0607059, arXiv:08032360[hep-ph]. Plan. General presentation - automation micrOMEGAs_2.2: direct detection
Neutrino mass and DM direct detection
Erice2013 21 Sept., 2013. Neutrino mass and DM direct detection. Daijiro Suematsu (Kanazawa Univ.). Based on the collaboration with S.Kashiwase PRD86 (2012) 053001, EPJC73 (2013) 2484. Outline. Motivation and ｂ a sic idea M odel and its features