Roger Blandford: New Horizons in Physics Education

Roger Blandford, KIPAC, Stanford University

New Horizons in Physics Education

Modern astrophysics is very well-suited to motivate, substantiate, and illustrate the concepts and applications that need to be conveyed when teaching physics. Astrophysics exploits the power of the image and taps into a common fascination with exploration and discovery that unites student and teacher, scientist and lay person. It can draw young people into careers in technology, science, medicine, and education, and it is a powerful way to help those who choose other careers to develop critical thinking skills and trust in rational argument. Astrophysics offers physics students a sure path to confident familiarity with principles and techniques of great generality. Besides, it is a lot of fun!

In this talk, I shall draw on recent astrophysical developments for examples that illustrate each of these attributes. I shall conclude by asking some questions concerning the skills that today’s students will need when they enter the workforce.

Duncan Brown (public): The New Astronomy of LIGO

Duncan Brown, Syracuse University

The New Astronomy of LIGO

Gravitational waves are among the most remarkable predictions of Einstein’s theory of general relativity. These waves—ripples in the curvature of spacetime—carry information about the changing gravitational fields of distant objects. Almost a century after Einstein first predicted the existence of gravitational waves, scientists are on the brink of directly detecting them for the first time. Gravitational waves will be a radically new tool for exploring fundamental physics and astronomy. They will probe the physics driving the most violent astrophysical events in the universe in ways inaccessible to electromagnetic observations. When the gravitational-wave window on the universe opens, the potential for discovery will be immense.

Construction of the U.S. Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) is well underway. Within the next five years, observers at Advanced LIGO expect to make the first detections of gravitational waves. Gravitational waves produced by the collision of black holes, asymmetric core collapse supernovae, rapidly spinning neutron stars, and even by the Big Bang itself are targets for detection in the years to come. I will give an overview of the new field of gravitational-wave astronomy: how the waves are generated, our efforts to detect them and what we hope to achieve when we can observe the universe in this new way.