A DOM (Digital Optical Module) being lowered into the ice. Photo by Jim Haugen.
Why go to the bottom of the world to explore the universe? Because it is a nearly ideal place to study one of the most elusive particles known, the almost massless subatomic messenger called the neutrino. The IceCube Neutrino Observatory at the South Pole searches for neutrinos from the most powerful astrophysical sources: events like exploding stars and extreme environments around black holes and neutron stars. This requires a large detector, and IceCube is the largest detector by volume ever built, encompassing a cubic kilometer of instrumented ice. That much ice weighs more than all the people in the world!
The fully built Askaryan Radio Array (ARA) project will have an effective volume 100 times larger than IceCube. The tradeoff is that it will only be capable of observing radio waves from interactions with extremely high energy neutrinos, a million times more energetic than the neutrinos produced by cosmic rays in the atmosphere. IceCube studies those lower energy atmospheric neutrinos, 100,000 per year, to learn more about neutrino properties, including their ability to transform from one type to another.
The universe is a huge and mysterious place that is largely unexplored. New technologies and creative approaches allow us to see things that aren’t directly viewable. Neutrinos will reveal new information about the Universe that can’t be recorded with optical or even more exotic telescopes that measure other types of light, like radio waves, microwaves, x-rays, and gamma rays. Many different roles and talents are needed to develop new approaches—technicians to make and operate new machines, computer experts to store and retrieve data, and scientists to define goals, identify promising projects, and guide students. IceCube and ARA are discovery instruments that will lead to a greater understanding of the cosmos and will hopefully uncover new mysteries for scientists to solve.