'Dark matter' presentation slideshows

European Roadmap on Astroparticle Physics ApPEC

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General Relativity and Black Holes (Overview). 17 th ???????? 2562. ??????? ????????? ??????????????????????????????????. SHEAP2019, IF Naresuan University. Outline. General Relativity. Cosmology. Black Holes. Introduction.

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James L. Pinfold University of Alberta

AstroCollider Physics. ASTROPARTICLE PHYSICS AND THE LHC. James L. Pinfold University of Alberta. Menu. The LHC and its multi-purpose detectors, for high p t physics (and forward physics?) Forward physics at the LHC and Cosmic Ray physics The cosmic ray energy spectrum

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Direct Search for Dark Matter with XENON100

Direct Search for Dark Matter with XENON100. Oral Examination Ethan Brown June 16, 2009. Overview. Evidence for the existence of Dark Matter Galactic Rotation Curves Gravitational Lensing Matter Distribution Dark Matter Candidates Properties of Dark Matter The Neutralino

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Strangelets: Who is Looking (and how?)

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Strangelets: Who is Looking (and how?)

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Physics 306 (Basic Astronomy) Fall 2006 Instructor: Dr. Alexey Belyanin (979) 845-7785, Room ENPH 509 Email: belyanin@ta

Physics 306 (Basic Astronomy) Fall 2006 Instructor: Dr. Alexey Belyanin (979) 845-7785, Room ENPH 509 Email: belyanin@tamu.edu http://faculty.physics.tamu.edu/belyanin/phys306.html Office Hours -- 12:45-14:45 TTR, or by appointment

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Phys 1830: Lecture 14

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Welcome to RAL (STFC)

Welcome to RAL (STFC). Norman McCubbin Acting Director of Particle Physics. Particle Physics Department. ~100 people in Particle Physics Department (PPD), 72 have PhDs, plus engineering, instrumentation, accelerator, and computing in other parts of the laboratories.

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The Large Synoptic Survey Telescope Status Summary

The Large Synoptic Survey Telescope Status Summary. Steven M. Kahn SLAC/KIPAC. LSST Technical Concept. 8.4 Meter Primary Aperture 3.4 M Secondary 5.0 M Tertiary 3.5 degree Field Of View 3 Gigapixel Camera 4k x 4k CCD Baseline 65 cm Diameter 30 Second Cadence Highly Dynamic Structure

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Spiral Galaxies

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Cosmic scaffolding and the growth of structure

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DIRECT DARK MATTER DETECTION AT THE CANFRANC UNDERGROUND LABORATORY FPA2011-23749

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Office of High E nergy Physics Cosmic Frontier Subprogram - Research Support

Office of High E nergy Physics Cosmic Frontier Subprogram - Research Support. CMB-S4 collaboration and project meeting October 18 , 2019. Kathy Turner, Cosmic Frontier Program Manager + Drew Baden (IPA ), Karen Byrum ( Detailee ), Eric Linder (IPA).

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Cos mology Through the UniverseAdventure

Cos mology Through the UniverseAdventure.org. Laurie Kerrigan LBNL IISME mentor George Smoot . The Universeadventure.org website used in conjunction with the Physics in and Through Cosmology Workshop. History & Structure Evolution of the Universe

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The Last Epoch

The Last Epoch. Cosmic Structure Formation. Today we have a matter-dominated universe ruled by the force of gravity. Slight variations in density produces formation regions for stars and galaxies.

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Cosmology = Big Questions

Cosmology = Big Questions. What is the universe made of How does it evolve How do galaxies, stars and planets form How do they evolve What Laws of physics in extreme conditions What are the origins and properties of the energetic particles reaching the Earth

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SHAPES OF GALAXIES

SHAPES OF GALAXIES. ALL THE SHAPES, SIZES AND FACTS OF GALAXIES! BY HELSBY HIGH SCHOOL. INTRODUCTION - BETH. GALAXIES = STARS (MILLIONS AND BILLIONS) PLANETS DARK MATTER. DIFFERENT TYPES OF GALAXIES INCLUDING : SPIRAL ELLIPTICAL IRREGULAR LENTICULAR .

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Is the End in Sight for Ultrahigh Energy Cosmic Rays (UHECR)?

Is the End in Sight for Ultrahigh Energy Cosmic Rays (UHECR)?. S. Sakir: [ http://physicsweb.org/article/world/15/9/3 ] J. Bahcall + E. Waxman: [ hep-ph/0206217 v3 ]. Mark Pearce September 3 rd 2002. Cosmic Ray Energy Spectrum. Balloons and Satellites. Cosmic ray astronomy?

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