IMAGE CAPTIONS
upper left corner:
if there's more than one universe, maybe they come in different sizes and flavors, like bubbles! (Our universe is the light green bubble, enlarged at lower right.)
lower right corner:
the texture of our universe is lumpy, as the WMAP observation shows

Anthony Aguirre

PERSONAL:

My new, biggest, most fun project, called Zander.

(billions of more pictures available by request.)

Anthony Aguirre, PhD
Assistant Professor of Physics

Department of Physics
University of California, Santa Cruz
1156 High Street
Santa Cruz, CA 95060

831.459.2449
aguirre@scipp.ucsc.edu

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FQXi
Ask me about an exciting new venture in philanthropically funded research into foundational questions in physics and cosmology!

One theory of the early universe, called "inflation," posits that the universe underwent an enormously rapid growth phase very early in its history. This theory explains some otherwise-puzzling features of the Big Bang, and makes specific predictions about the texture of the observed universe, recently confirmed in a spectacular fashion by the WMAP results (right). But inflationary theory has a downside: once it starts, it cannot end everywhere;