'Cold dark matter' presentation slideshows

Gamma ray astroparticle physics with GLAST

Gamma ray astroparticle physics with GLAST. a rotating black hole in an accretion disk. Binary system formed by a black hole and a companion star. A model of Gamma Ray Burst. PULSARS. Multiwavelength light curves of the seven pulsars detected by GRO.

1.01k views • 87 slides

DARK MATTER IN THE MILKY WAY

DARK MATTER IN THE MILKY WAY. ALEXEY GLADYSHEV (JINR, DUBNA & ITEP, MOSCOW) SMALL TRIANGLE MEETING 2005. Outlook. Introduction. Evidence for Dark Matter. Types of Dark Matter. Direct searches for the Dark Matter. EGRET data: an excess of the diffuse gamma ray flux

1.13k views • 87 slides

Dan Hooper Particle Astrophysics Center Fermi National Laboratory dhooper@fnal.gov

Hot on the Trail of Particle Dark Matter. Dan Hooper Particle Astrophysics Center Fermi National Laboratory dhooper@fnal.gov. University of Kansas April 17, 2006. What do we know about dark matter?. What do we know about dark matter?. Ask An Astrophysicist:. ? A Great Deal!.

876 views • 73 slides

Cosmic Acceleration Then and Now

Cosmic Acceleration Then and Now. Josh Frieman Fermilab and the University of Chicago Progress on Old and New Themes in Cosmology Avignon, April 18, 2014. Last Supper (in earlier version of program). Cosmologists discuss BICEP2 results at PONT banquet. April, c. 33 AD.

769 views • 60 slides

25(+) Years of Research in Nuclear and Particle Physics

25(+) Years of Research in Nuclear and Particle Physics. Prof. Donald Koetke Valparaiso University. 5 February 2010. Outline. Nuclear Physics vs. Particle Physics Experiment Goals Experimental Methods A Timeline The Local Players The Future. Nuclear Physics.

801 views • 57 slides

CMB: Sound Waves in the Early Universe

Before recombination: Universe is ionized. Photons provide enormous pressure and restoring force. Photon-baryon perturbations oscillate as acoustic waves. After recombination: Universe is neutral. Photons can travel freely past the baryons.

836 views • 57 slides

863 views • 55 slides

Axions

855 views • 55 slides

Axions

665 views • 54 slides

3rd International Summer School on Astroparticle Physics "NIJMEGEN09"

3rd International Summer School on Astroparticle Physics "NIJMEGEN09". Hadron Collider Results Impact on Particle Astrophysics David Toback Texas A&M University. Some Context Before We Begin. Experimental Particle Physicist by Training CDF (Tevatron) and CMS (LHC) experiments

444 views • 44 slides

Bernard60: Conference Summary

501 views • 37 slides

New Museum of Contemporary Art, NYC designed by SANAA: Kazuyo Sejima & Ryue Nishizawa

Post-Minimalist Architectural Sculpture Sculptural Architecture http://www.nytimes.com/packages/khtml/2007/03/27/arts/artsspecial/20070328_BIRTH_AUDIOSS.html?adxnnl=1&adxnnlx=1175178451-CKgno4UBJdFF1+NuoR9TeA. New Museum of Contemporary Art, NYC designed by SANAA: Kazuyo Sejima & Ryue Nishizawa.

630 views • 33 slides

Quasars and Low Surface Brightness Galaxies as Probes of Dark Matter

Quasars and Low Surface Brightness Galaxies as Probes of Dark Matter. Erik Zackrisson. Outline. Dark matter Dark matter halos Baryonic and non-baryonic dark matter Cold dark matter Quasars Gravitational lensing Redshift Low Surface Brightness Galaxies Rotation curves Summary of Results.

507 views • 29 slides

Quasars and Low Surface Brightness Galaxies as Probes of Dark Matter

Quasars and Low Surface Brightness Galaxies as Probes of Dark Matter. Erik Zackrisson. Outline. Dark matter Dark matter halos Baryonic and non-baryonic dark matter Cold dark matter Quasars Gravitational lensing Redshift Low Surface Brightness Galaxies Rotation curves Summary of Results.

484 views • 29 slides

Cosmological Structure Formation A Short Course

Cosmological Structure Formation A Short Course. I. Why Dark Matter, and why Cold? Chris Power. Zwicky (1933) measured the radial velocities for eight galaxies in the Coma cluster and found an unexpectedly large velocity dispersion of ~1000 km/s.

462 views • 25 slides

Dynamical Dark Energy and Its Coupling to Matter

Dynamical Dark Energy and Its Coupling to Matter . Kin-Wang Ng ( ??? ) ASIoP ( ???????? ) & ASIAA ( ???????? ), Taipei NTHU Oct 4, 2007. Thanks to D.-S. Lee( ??? ), W-L. Lee( ??? ) , S. Lee( ??? ) , G.-C. Liu ( ??? ) for collaboration . The Hot Big Bang Model. What is CDM?

328 views • 24 slides

Primordial perturbations and precision cosmology from the Cosmic Microwave Background

Primordial perturbations and precision cosmology from the Cosmic Microwave Background. Antony Lewis CITA, University of Toronto. http://cosmologist.info. Evolution of the universe. Opaque. Transparent. Hu & White, Sci. Am., 290 44 (2004).

396 views • 18 slides

Cosmological Structure Formation A Short Course

322 views • 18 slides

How Was The Universe Created ?

How Was The Universe Created ?. A look into the theory on how we and our Universe were created. By : Michael. The Dawn Of Time. But We Have A little bit, more to cover.

195 views • 11 slides