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FIGURE 5‐2 Simulated image <strong>of</strong> gravitational radiation from two merging black holes using NASA's<br />

Columbia supercomputer. A movie <strong>of</strong> this simulation can be found at<br />

http://www.nasa.gov/centers/goddard/mpg/146898main_viz_shiftingall_21.320x240.mpg<br />

(Credit: Chris Henze, NASA.)<br />

<strong>The</strong>oretical Challenges for the Next Decade<br />

A healthy theory program advances science on a broad front, and supports a range <strong>of</strong> targeted<br />

activities as well as the exploration <strong>of</strong> radical new ideas that inspire missions for the distant future. For<br />

this decade, the Science Frontier Panels (SFPs) and Chapter 2 <strong>of</strong> this report have identified questions on<br />

the forefront <strong>of</strong> astrophysics, several <strong>of</strong> which present specific and significant theoretical challenges.<br />

<strong>The</strong> Cosmology and Fundamental Physics panel raises the questions: What is the nature <strong>of</strong> dark<br />

energy and why is the universe accelerating What is the nature <strong>of</strong> inflation and what can we learn from<br />

the early universe about the fundamental laws <strong>of</strong> physics New observations are central to providing the<br />

necessary constraints to address these questions, but theories are ultimately being put to the test.<br />

One <strong>of</strong> the upcoming challenges associated with the Stars and Stellar Evolution Panel is the threedimensional<br />

simulation <strong>of</strong> the magnetic field observed in the solar corona using the Solar Dynamics<br />

Observer and other solar observatories. <strong>The</strong> quality <strong>of</strong> the data that is now being garnered presents a<br />

strong challenge to simulators. Success in explaining the behavior <strong>of</strong> the solar magnetic field will pay<br />

large dividends as astrophysicists attempt to understand how fields behave in other environments.<br />

Meanwhile the Galactic Neighborhood panel’s prime research topics involved study <strong>of</strong> the<br />

circumgalactic and interstellar media seen as complex ecosystems. <strong>The</strong>se are both topics where<br />

sophisticated simulations go hand in hand with the observational program. A third question concerns the<br />

fossil record <strong>of</strong> star formation as a means <strong>of</strong> understanding the first stars and the subsequent assembly <strong>of</strong><br />

galaxies like our own. Here the theories <strong>of</strong> stellar evolution and stellar dynamics are crucial. <strong>The</strong> fourth<br />

research area, the use <strong>of</strong> the galaxy to study dark matter (Figure 5-3), has already attracted the attention <strong>of</strong><br />

a large community <strong>of</strong> theoretical physicists.<br />

PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION<br />

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