Loading presentation...
Prezi is an interactive zooming presentation

Present Remotely

Send the link below via email or IM

Copy

Present to your audience

Start remote presentation

  • Invited audience members will follow you as you navigate and present
  • People invited to a presentation do not need a Prezi account
  • This link expires 10 minutes after you close the presentation
  • A maximum of 30 users can follow your presentation
  • Learn more about this feature in our knowledge base article

Do you really want to delete this prezi?

Neither you, nor the coeditors you shared it with will be able to recover it again.

DeleteCancel

Make your likes visible on Facebook?

Connect your Facebook account to Prezi and let your likes appear on your timeline.
You can change this under Settings & Account at any time.

No, thanks

Dark Matter and Energy

No description
by

Michael Chen

on 11 June 2013

Comments (0)

Please log in to add your comment.

Report abuse

Transcript of Dark Matter and Energy

Michael Chen What's the Matter with Dark Matter? Crazy Clusters Cosmic Microwave Background Gravitational Lensing What is Dark Matter? What's Next? Funky Galaxies Black Holes
MACHOS
Modified Newtonian Dynamics The Big Mystery What is the Universe made of? Dark Matter Dark Energy "Normal" Matter ? % ? % ? % Galactic Rotation Curves B: Observed behavior A: Expected Behavior Coma Cluster Fritz Zwicky 1933 400 TIMES! Andromeda Inner arms Outer arms http://www.nytimes.com/2011/04/14/science/space/14dark.html?_r=0
http://iopscience.iop.org/1367-2630/11/10/105002/pdf/1367-2630_11_10_105002.pdf
http://www.physics.purdue.edu/darkmatters/blog/
http://www.roe.ac.uk/~heymans/website_images/Gravitational-lensing-galaxyApril12_2010-1024x768.jpg
http://astro.berkeley.edu/~mwhite/darkmatter/dm.html
http://www.universetoday.com/61587/dark-matter/
http://hitoshi.berkeley.edu/public_html/susy/susy.html
http://www.pbs.org/wgbh/nova/physics/dark-matter.html
http://scienceblogs.com/startswithabang/files/2008/02/010cmb.jpg
http://xenon.astro.columbia.edu/
http://www.youtube.com/watch?feature=player_embedded&v=-kEYRm4NWEYhttp://www.youtube.com/watch?v=wco8kAQT5SIhttp://www.nytimes.com/2011/04/14/science/space/14dark.html?_r=0
http://www.youtube.com/watch?v=JZIUbZw3i78http://www.youtube.com/watch?v=JZIUbZw3i78 v^2=GM/r A flat curve suggests that mass must increase linearly with radius 2.725 degrees K WIMP Weakly Interacting Massive Particle Non-Baryonic, Cold Dark Matter The Hunt for WIMPS WIMP DETECTION CDMS AMS XENON Alpha Magnetic Spectrometer Where: ISS Liquid Noble Detector Sources Where: Gran Sasso, Italy Cryogenic Dark Matter Search Where: Soudan Mine, Minnesota Understand Dark Energy
Full transcript