'Dark matter' diaporamas de présentation

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

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

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?

Strangelets: Who is Looking (and how?). Evan Finch Yale University March 29, 2006. Strangelets (Small Lumps of Strange Quark Matter). Roughly equal numbers of u,d,s quarks in a single ‘bag’ of cold hadronic matter.

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

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 .

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

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

European Roadmap on Astroparticle Physics ApPEC. C oordination C ooperation C ompetition C onvergence. Integrated L arge I nfrastructures for A stroparticle S cience. ILIAS. ~1200 scientists, budget ~10 M€. Networking Activities (N2) Deep Underground science laboratories

1. Hubble’s Law. Dr. Bill Pezzaglia, Santa Clara University. 2. A1. Static Cosmology. Newton proposed that the universe must be infinite to be balanced; a finite universe would collapse due to gravity. 1920 Eddington shows that Newton’s infinite universe is unstable and would collapse.

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).

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.

Stephan’s Quintet. Phys 1830: Lecture 14. J. English. Next Classes: Image-making. Previous Classes: Newtonian Gravity tides Interacting Galaxies This Class: Interacting Galaxies continued Constant acceleration Orbits and mass Dark Matter Einstein’s Gravity Gravitational lensing.

DIRECT DARK MATTER DETECTION AT THE CANFRANC UNDERGROUND LABORATORY FPA2011-23749. JOSÉ ANGEL VILLAR RIVACOBA Universidad de Z aragoza. Plan of the talk. The Research Group Members and Scientific Activities Previous Projects on Dark Matter. The Search for Dark Matter

Strangelets: Who is Looking (and how?). Evan Finch Yale University March 29, 2006. Strangelets (Small Lumps of Strange Quark Matter). Roughly equal numbers of u,d,s quarks in a single ‘bag’ of cold hadronic matter.

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

Spiral Galaxies. Elliptical Galaxies. Irregular Galaxies. Classification of Galaxies. Properties of Galaxies. Other galaxy types : Peculiar, Interacting, Ring, Starburst, Dwarf, Luminous Infrared, Active Nuclei, Damped Lyman-alpha. Stephan’s Quintet – Colliding galaxies.

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.

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

Cosmic scaffolding and the growth of structure. Cosmic scaffolding and the growth of structure. Richard Massey (CalTech ) with Jason Rhodes (JPL), David Bacon (Edinburgh), Joel Berg é (Saclay), Richard Ellis (CalTech), Alexis Finoguenov (Garching), Catherine Heymans (UBC),