This course explores the field of cosmology, focusing on the cosmic background radiation to understand the birth and evolution of the universe. The learning outcomes include gaining insights into the early expansion of space, the geometric shape of the universe, and the formation of galaxies. Participants will also delve into questions about the cosmos, such as the timing of the first stars and events post-Big Bang. The course teaches skills in analyzing cosmic background radiation data and understanding key concepts in cosmology. The teaching method involves presentations by leading scientists, including Nobel Laureate John Mather, and a moderator facilitating discussions. The intended audience includes individuals interested in astronomy, cosmology, and scientific discoveries about the universe.
Overview
Syllabus
Lawrence Krauss's Introduction
Robert Woodrow Wilson: Tuning in to the Big Bang
Participant introductions.
What lead you to the path of science?
Launching the COBE satellite.
Measuring temperatures 1/100,000 of three degrees.
When your wrong ... you move on.
The boomerang experiment from Antarctica.
How big is the universe?
How far back in time can we see?
Amber Miller and the EBEX project.
Polarization from gravity waves from the beginning of time.
What is the future of measuring the universe?
What is a microwave? Are we sure matter exists?
Taught by
World Science Festival
