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Neutron Stars, Black Holes, and Gravitational Waves (Paperback)
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Neutron Stars, Black Holes, and Gravitational Waves (Paperback)
Series: IOP Concise Physics
Expected to ship within 10 - 15 working days
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Albert Einstein's General Theory of Relativity, published in 1915,
made a remarkable prediction: gravitational radiation. Just like
light (electromagnetic radiation), gravity could travel through
space as a wave and affect any objects it encounters by alternately
compressing and expanding them. However, there was a problem. The
force of gravity is around a trillion, trillion, trillion times
weaker than electromagnetism so the calculated compressions and
expansions were incredibly small, even for gravity waves resulting
from a catastrophic astrophysical event such as a supernova
explosion in our own galaxy. Discouraged by this result, physicists
and astronomers didn't even try to detect these tiny, tiny effects
for over 50 years. Then, in the late 1960s and early 1970s, two
events occurred which started the hunt for gravity waves in
earnest. The first was a report of direct detection of gravity
waves thousands of times stronger than even the most optimistic
calculation. Though ultimately proved wrong, this result started
scientists thinking about what instrumentation might be necessary
to detect these waves. The second was an actual, though indirect,
detection of gravitational radiation due to the effects it had on
the period of rotation of two 'neutron stars' orbiting each other.
In this case, the observations were in exact accord with
predictions from Einstein's theory, which confirmed that a direct
search might ultimately be successful. Nevertheless, it took
another 40 years of development of successively more sensitive
detectors before the first real direct effects were observed in
2015, 100 years after gravitational waves were first predicted.
This is the story of that hunt, and the insight it is producing
into an array of topics in modern science, from the creation of the
chemical elements to insights into the properties of gravity
itself.
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