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History and Structure of the Universe


Nikhil Padmanabhan– Dark Matter and Dark Energy
Dr. Padmanabhan discussed Dark Matter and Dark Energy, explaining that regular matter only comprises about 4% of the universe. The rest is composed of dark matter and dark energy.  He also presented supporting scientific evidence. Lecture summary.

 

Video clip: Gravity and universe expansion
Video clip: Universe structure
Video clip: Sloan Digital Sky Survey

PPT Video
PDF of Powerpoint Presentation

 

 

Hubble Constant and the Age of the Universe

Sean Fotrell

Sean Fottrell explained how the age of the universe is determined by using a supernova’s redshift to calculate the Hubble Constant, and how this has changed over time.

 

Teacher Resources:

Accelerating Universe activity
This lesson examines the acceleration of the expansion rate of the universe as evidence of Dark Energy.

 

Connecting Cosmic Rays to Particle Physics - Stu Loken

 

 

A proton from outer space (yellow) hits the upper atmosphere, and produces a shower of other particles (green). Some of these particles (mostly pions) decay into muons (red). Only a small fraction of the muons reaches the earth's surface, because most decay in flight. Therefore, at higher altitudes there are more muons, because fewer have decayed. At sea level, one muon goes through an area the size of your fingernail about every minute!

 

 

Powerpoint Presentation pdf

 

Discovery Station


Earth's Gravity - Rollie Otto - Vernier / LoggerPro
Dr. Otto used the Vernier program to teach students how to graph objects and find the acceleration caused by gravity.  The students made short videos of themselves throwing a variety of balls.  The videos were then imported into Vernier where the data was graphically analyzed to determine the value of g on earth.

 

Relativity and Time Dilation

Glen Melnik

 

 

Glen Melnik illustrated Einstein’s theory of Special Relativity using a theoretical scenario of a person in a room traveling at relativistic speed. There is a clock in the room consisting of a photon beam bouncing between the ceiling and the floor. The photon beam must travel a larger distance when set in motion than when at rest - making the clock "tick" slower. Glen used simple trigonometry and algebra to show the students a derivation of the Lorentz Transformations from the assumptions of Special Relativity.

 

 

Day one: Cosmology for the 21st Century

Day two: History and Structure of the Universe

Day four: Standard Model of Particles and Interactions

Day five: Beyond the Standard Model of Particles and Interactions

Day six: Cosmologists for the 21st Century

 

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