prepublication copy - The Department of Astronomy & Astrophysics ...
prepublication copy - The Department of Astronomy & Astrophysics ...
prepublication copy - The Department of Astronomy & Astrophysics ...
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
FIGURE 2‐2 <strong>The</strong> source 3C 75, shown here in x‐rays (blue) and radio waves (pink), is a rare example where<br />
two galaxies have been caught in the act <strong>of</strong> merging. Not only do their stars merge, but their central black<br />
holes ‐ each producing a pair <strong>of</strong> jets containing gas moving outward with speed close to that <strong>of</strong> light ‐ will<br />
do likewise in perhaps a few hundred million years. Many similar mergers involving smaller black holes in<br />
the nuclei <strong>of</strong> younger galaxies are thought to have taken place. When black holes coalesce, they create<br />
intense bursts <strong>of</strong> gravitational radiation. (Credit: X‐ray: NASA/CXC/AIfA/D.Hudson & T.Reiprich et al.;<br />
Radio: NRAO/VLA/NRL.)<br />
galaxies form and evolve will be possible. We are on the verge <strong>of</strong> a new era <strong>of</strong> discovery in gravitational<br />
wave astronomy.<br />
In addition, gravitational waves could be created by exotic processes occurring in the young<br />
universe and would have been propagating freely to us ever since. Several speculative sources such as<br />
cosmic strings and abrupt changes in the form that the contents <strong>of</strong> the universe assumed—“phase<br />
changes,” like the change from water to ice—have been suggested but the truth is that we do not quite<br />
know what to expect. A possible way to see if there are any measurable signals with wavelengths <strong>of</strong><br />
roughly light years employs very precise radio measurements <strong>of</strong> naturally occurring cosmic “clocks”<br />
called pulsars. 2 Spread across the sky, the separations between these cosmic clocks will change as a long<br />
wavelength gravitational wave passes by, potentially measurably changing the arrival times <strong>of</strong> their radio<br />
pulses.<br />
Opening the Time Domain: Making Cosmic Movies<br />
By eye, the universe appears static apart from the twinkling <strong>of</strong> starlight caused by Earth’s<br />
atmosphere. In fact, it is a place where dramatic things happen on timescales we can observe—from a<br />
tiny fraction <strong>of</strong> a second to days to centuries. Stars in all stages <strong>of</strong> life rotate, pulsate, and undergo<br />
activity cycles while many flare, accrete, lose mass, and erupt, and some die in violent explosions. Binary<br />
neutron stars and black holes merge, emitting, in addition to bursts <strong>of</strong> radiation, gravity waves.<br />
Supermassive black holes in the centers <strong>of</strong> galaxies swallow mass episodically and erupt in energetic<br />
outbursts. Some objects travel rapidly enough for us to measure their motion across the sky.<br />
2 <strong>The</strong> 1993 Nobel Prize in Physics was awarded to two American astronomers for their work on binary pulsars.<br />
PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION<br />
2-6