Send the link below via email or IMCopy
Present to your audienceStart 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
Physics 200 Black Holes & Dark Matter
Transcript of Physics 200 Black Holes & Dark Matter
1. Flat universe
2. inconstancies in density from hills and valley A form of the cosmological constant, filling empty space evenly An energy force controlled by the time and space, density dependent on time and space Expansion of supernovas at an even rate. The Universe is flat, according to the cosmic microwave background anisotropies. In order to maintain flatness, a density must be even Large scale structures show a lack of critical mass, and voids without dark energy Nature of dark matter
- very sparse and reacts only to gravity
-negative pressure, helps expansion of the universe Why is it Important?
1. 73% of the Universe
2. Controls movement of the universe
3.helps explain the cyclic model of the universe Abell 2218 Galaxies? Notice the bendy bits... distorts space and time The presence of mass actually ? ? ? (Weakly Interacting Massive Particles) "cold" dark matter supersymmetric the dark matter enigma Not originally proposed to solve Slightly electromagnetically reactive? dark matter Bad news as a candidate parallel universes Could the extra "mass" be interacting with ours? Early "clumping" of dark matter the universe as it is today may have been crucial in the forming of Star Clusters Galaxies Clusters Filaments Planetary systems Black Holes Stellar Systems YOUCH! 23% 73% Where are Black Holes?
Where do they come from?
How do we see them?
What are the different types?
History What Are Black Holes? History Dark Matter