We also offer undergraduate minors in Astronomy and Astrophysics. Cosmology treats the big questions: What is the history of the universe, and what does its future look like? What is the mysterious dark matter that dominates its composition? How is the expansion of the universe accelerating with time, and why? How does structure form in the universe?
How can we use the observational evidence offered by astrophysics to address these questions? Cosmology within the School treats a range of these questions, from both theoretical and observational perspectives. Laboratory experiments in astronomy are usually impossible, and perhaps that's a good thing: Even if we could set up a supernova explosion in the lab, it would probably be a bad idea.
Therefore, astrophysicists turn instead to detailed computations, relying on the fact that the physical laws governing astronomical objects are the same ones that apply on Earth. Astrophysical processes are extremely nonlinear and computers are essential to understanding them.
Focusing telescopes in nuclear astrophysics|INIS
Stars are responsible for lighting up the universe and transforming the hydrogen and helium gas left by the big bang into the elements of the periodic table out of which the complex structures of planets and life are made. The evolution of stars is critical to understanding processes on scales from the evolution of galaxies over cosmic time to the formation and development of planets in individual solar systems. Star formation and stellar evolution are the story of the struggle between gravity and the energy produced by nuclear fusion in the interiors of stars.
Faculty at the School explore the problems of star formation and stellar evolution through a variety of observational and theoretical approaches. ASU researchers use the Hubble, Chandra, and Spitzer space telescopes to study star forming clouds and stellar populations in the Milky Way and other galaxies, the massive explosions that result when stars end their lives as supernovae, and the compact objects left at the end of a star's evolution.
Exploration systems engineers at the School are developing the next generation of ground and space-based multiwavelength instrumentation for studying star forming regions. State-of-the-art computer models are run on ASU's Saguaro parallel computing facility to model the clouds and disks that give birth to stars and planets and the lifecycles of stars, their dynamic interiors, and violent deaths.
About this book
Understanding the formation and evolution of galaxies is fundamental to understanding how the universe transformed from a bland mix of hydrogen and helium after the Big Bang to the beautiful diversity of objects we see today. Since many experts in different fields are needed to undertake this arduous task, it is crucial that the training of young researchers be focused both on providing them with a general physical background, and on specializing them in some specific field among those mentioned. This focus point aims to give the students and general readers an overview on the state of the art of modern research in stellar modelling and nucleosynthesis, in Gamma- and X-ray astronomy, in astro-particle physics, and in experimental low-energy nuclear astrophysics.
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