A Particle Physicist View of Particle Astrophysics Bill Atwood SCIPP/UCSC 18-Sept-2008.

Slides:



Advertisements
Similar presentations
Observation of the Universe from the Moon – Elisabetta Cavazzuti – LNF May 7, 2007 ITALIAN VISION FOR MOON EXPLORATION OBSERVATION OF THE UNIVERSE FROM.
Advertisements

ICECUBE & Limits on neutrino emission from gamma-ray bursts IceCube collaboration Journal Club talk Alex Fry.
Implication of recent cosmic ray data Qiang Yuan Institute of High Energy Physics Collaborated with Xiaojun Bi, Hong Li, Jie Liu, Bing Zhang & Xinmin Zhang.
J. Hewett, HEP2010 Signatures of Supersymmetry Without Prejudice Berger, Conley, Cotta, Gainer, JLH, Le, Rizzo arXiv: , , in progress.
Committee on Science, Engineering and Public Policy Board on Physics and Astronomy Committee on Setting Priorities for NSF’s Large Research Facility Projects.
Astrophysical and Cosmological Impact of Extra Dimensions.
Workshop on the interconnection between particle physics and cosmology Gordy Kane Texas A&M May 2007.
High Energy  -rays Roger Blandford KIPAC Stanford.
Large Magellanic Cloud, 1987 (51.4 kparsec) SN 1987a after before 2006 Hubble.
07/12/061 Huge Black Holes: Measuring the Monster in the Middle Logan Hill and Sarah Silva Sonoma State University.
Gamma-Ray Astronomy Dana Boltuch Ph. D
07/12/061 Huge Black Holes: Measuring the Monster in the Middle Fill in your information here. Fill in your information here.
The Extreme Universe of Gamma-ray Astronomy Professor Lynn Cominsky Department of Physics and Astronomy Sonoma State University.
Simulating the Gamma Ray Sky Andrew McLeod SASS August 12, 2009.
TeV Particle Astrophysics 2009 Welcome & SLAC Connections David MacFarlane Associate Laboratory Director for PPA.
Concluding Comments For the Course Cosmology Fascinating Past Highly accomplished present (for example, the material covered in this course). Really exciting.
Physics with ATLAS and CMS Are there new symmetries or extra-dimensions? What is dark matter? Where does mass come from? The two big multi-purpose experiments.
Survey of the Universe Greg Snow U Nebraska Lincoln CROP.
The latest experimental evidence suggests that the universe is made up of just 4% ordinary matter, 23% cold dark matter and 73% dark energy. These values.
Primordial BHs. 2 Main reviews and articles astro-ph/ Primordial Black Holes - Recent Developments astro-ph/ Gamma Rays from Primordial.
Eduardo do Couto e Silva - ATC/LM Colloquium, June How many neutralinos are there? Expansion of universe Depletion of neutralinos Creation of neutralinos.
Program 1.The standard cosmological model 2.The observed universe 3.Inflation. Neutrinos in cosmology.
J. Nielsen1 The ATLAS experiment at the Large Hadron Collider Jason Nielsen UC Santa Cruz VERTEX 2004 July 28, 2010.
Gamma-ray Astrophysics Pulsar GRB AGN SNR Radio Galaxy The very high energy  -ray sky NEPPSR 25 Aug Guy Blaylock U. of Massachusetts Many thanks.
LHC ~E -2.7 ~E -3 ankle 1 part km -2 yr -1 knee 1 part m -2 yr -1 T. Gaisser 2005 Nature accelerates particles 10 7 times the energy of LHC! where?how?
International collaboration in high energy physics experiments  All large high energy physics experiments today are strongly international.  A necessary.
Quintessino model and neutralino annihilation to diffuse gamma rays X.J. Bi (IHEP)
SUSY Dark Matter Collider – direct – indirect search bridge. Sabine Kraml Laboratoire de Physique Subatomique et de Cosmologie Grenoble, France ● 43. Rencontres.
Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach.
Physics at the High Energy Frontier J. Hewett PANIC 2005.
Relating dark matter and radiative Seesaw neutrino mass scales without beyond SM gauge symmetry Xiao-Gang He 1. Introduction 2. Radiative seesaw and dark.
Physics Session Summary Nobuchika Okada Institute of Particle and Nuclear Studies, High Energy Accelerator Research Organization (KEK) TILC09, Tsukuba,
Tension Between A Fourth Generation And The LHC Higgs Searches Xiao-Gang He (SJTU&NTU) Xiao-Gang He and German Valencia, arXiv: Xiao-Gang He and.
CMB observations and results Dmitry Pogosyan University of Alberta Lake Louise, February, 2003 Lecture 1: What can Cosmic Microwave Background tell us.
Planning for Discoveries in Particle Physics Michael Witherell EPP2010 May 16, 2005.
Richard E. Hughes lastClass p.1 “The most incomprehensible thing about the universe is that it is comprehensible” - Albert Einstein.
The Energy in our Universe Dr. Darrel Smith Department of Physics.
P5 and the Particle Physics Roadmap A. Seiden UC Santa Cruz Chair of P5.
SLUO LHC Workshop: Closing RemarksPage 1 SLUO LHC Workshop: Closing Remarks David MacFarlane Associate Laboratory Directory for PPA.
Dark Matter Particle Physics View Dmitri Kazakov JINR/ITEP Outline DM candidates Direct DM Search Indirect DM Search Possible Manifestations DM Profile.
DARK MATTER CANDIDATES Cody Carr, Minh Nguyen December 9 th, 2014.
Cosmic Rays GNEP Teacher Workshop Steve Shropshire, July 2007.
1 Additional observable evidences of possible new physics Lecture from the course “Introduction to Cosmoparticle Physics”
Dan Hooper Theoretical Astrophysics Group Fermi National Laboratory Theoretical Particle-Astrophysics At Fermilab Annual DOE Review May.
260404Astroparticle Physics1 Astroparticle Physics Key Issues Jan Kuijpers Dep. of Astrophysics/ HEFIN University of Nijmegen.
DARK MATTER & GALACTIC ROTATION 2012 ASTRO SUMMER SCHOOL.
Collider searchIndirect Detection Direct Detection.
WILGA k61/10 Search for cosmic rays from gamma ray bursts Marcin Molak Faculty of Physics Warsaw University of Technology.
Particle Physics: Status and Perspectives Part 9: Energy Frontier and Open Questions Manfred Jeitler SS 2015.
High Energy Accelerators Dennis Silverman Physics and Astronomy U. C. Irvine.
Low scale gravity black holes at LHC Enikő Regős ( CERN )
Dark Matter Mathematics Janet Moore NASA Educator Ambassador Janet Moore NASA Educator Ambassador.
Extreme Astrophysics the the > 10 GeV photon energy < cm wavelength > 10 8 TeV particles exist > 10 8 TeV particles exist they should.
KCL Group of Theoretical Particle Physics & Cosmology (TPPC) Prof. John Ellis (head) (JE) Dr. Bobby Acharya (BA) Dr. Jean Alexandre (JA) Dr. Malcolm Fairbairn.
Fermi Gamma-ray Space Telescope Searches for Dark Matter Signals Workshop for Science Writers Introduction S. Ritz UCSC Physics Dept. and SCIPP On behalf.
Lisa Randall Harvard  It has gravitational interactions—of matter!  Gravitational lensing  Rotation curves in galaxies  Detailed.
07/12/061 Modeling a Black Hole Fill in your information here. Fill in your information here.
High Energy Observational Astrophysics. 1 Processes that emit X-rays and Gamma rays.
CPM 2012, Fermilab D. MacFarlane & N. Holtkamp The Snowmass process and SLAC plans for HEP.
Stanford Linear Accelerator
AstroParticle Physics European Consortium
Unveiling Fundamental Physics from the Cosmic First Light
Roger Blandford KIPAC Stanford
Comparison of GAMMA-400 and Fermi-LAT telescopes
Primordial BHs.
Stanford Linear Accelerator
Introduction to universal extra dimensions (UEDs)
Stanford Linear Accelerator
Primordial BHs.
TeV Physics and ILC 何红建 清华大学.
Presentation transcript:

A Particle Physicist View of Particle Astrophysics Bill Atwood SCIPP/UCSC 18-Sept-2008

All good stories start with “….in the beginning…”  GLAST (now FERMI) began in 1992 one year after EGRET began revealing an extraordinary Gamma Ray Sky  HEP detector development for SSC in full swing  A re-do of EGRET with modern HEP detectors, saturating the launch capabilities of a Delta II rocket resulted in the GLAST design  Rapid simulation capability added credibility to design concept Marriage between High Energy Astro and HEP communities  Each brings a unique perspective and expertise.  And… each brings their own culture and “way of doing business” High Energy Astrophysics + HEP Particle Astrophysics Glast was amoung the first in the new interdisciplinary field….

HEP - Particle Astro Community Comparison HEPCollecting Particle decay modes (Br. Ratios) Particles & their parameters Cross-sectionsExploring Neutrino generations Parity Violation Searches – Higgs, SUSY, Extra Dimensions, etc. Particle-AstroCollecting Pulsars AGN Other exoticsExploring CMB Hubble expansion Dark Matter Lorentz Invariance Primordial relics Laboratories for GR Collecting in the two groups is quite disjoint Explorers are on similar quests My personal preference is Exploring

Furthermore the Keplerian velocities depend only the ratio r s /r So the inner edge of accretion disks have v ~ ~ parsecs Accretion Disk r s Black Hole Diameter = 2r s ~ 4 AU A Sketch of a Massive Black Hole……not-to-scale An example distinguishing Gathering/Exploring from Astrophysics A Laboratory for Exploring Extreme Environments

A Question for All: The Dark Matter Mystery Only visible effect due to Gravitational Interactions FERMI-LAT FERMI-LAT  Self Interactions could produce measurable effects in Gamma Ray and Cosmic Ray Spectra.  It is doubtful that it will positively identify the precise nature of the particles LHC: ATLAS / CMS  May find particle DM candidate(s).  If so, this will sharpen the search in FERMI A Plausible Scenario  LHC finds new particles  FERMI tells what their role is in the Universe at large For Explorers – this coming year is remarkable & exciting!!! IF… IF… Dark Matter has a particle component…