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Ch 15: Oscillations
Chapter 15, Problem 13

September 2015 saw the historic discovery of gravitational waves, almost exactly 100 years after Einstein predicted their existence as a consequence of his theory of general relativity. Gravitational waves are a literal stretching and compressing of the fabric of space. Even the most sensitive instruments—capable of sensing that the path of a 4-km-long laser beam has lengthened by one-thousandth the diameter of a proton—can detect waves created by only the most extreme cosmic events. The first detection was due to the collision of two black holes more than 750 million light years from earth. Although a full description of gravitational waves requires knowledge of Einstein's general relativity, a surprising amount can be understood with the physics you've already learned. (d) Two black holes collide and merge when their Schwarzchild radii overlap; that is, they merge when their separation, which we've defined as 2r, equals 2RSch . Find an expression for ΔE=Ef−Ei , where Ei ≈ 0 because initially the black holes are far apart and Ef is their total energy at the instant they merge. This is the energy radiated away as gravitational waves. Your answer will be a fraction of Mc², and you probably recognize that this is related to Einstein's famous E=mc² . The quantity Mc² is the amount of energy that would be released if an entire star of mass M were suddenly converted entirely to energy.

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Identify the given variables and constants: The mass of the merged black holes is denoted as M, and c represents the speed of light. The initial energy Ei is approximately 0 because the black holes are initially far apart.
Understand that the final energy Ef at the instant of merging can be expressed in terms of the mass-energy equivalence from Einstein's equation, E=mc². Here, M is the total mass of the system and c is the speed of light.
Recognize that the energy difference ΔE = Ef - Ei represents the energy radiated away as gravitational waves. Since Ei ≈ 0, ΔE ≈ Ef.
Express ΔE as a fraction of Mc² to find the proportion of the total mass-energy that is converted into gravitational waves during the merging of the black holes.
Conclude that the expression for ΔE will be some fraction of Mc², indicating how much energy is emitted as gravitational waves relative to the total mass-energy of the system.

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Key Concepts

Here are the essential concepts you must grasp in order to answer the question correctly.

Gravitational Waves

Gravitational waves are ripples in spacetime caused by the acceleration of massive objects, such as colliding black holes. Predicted by Einstein's general relativity, these waves carry energy away from their source, allowing us to detect cosmic events that are otherwise invisible. Their detection requires highly sensitive instruments, as the distortions they create in spacetime are incredibly small, often on the order of a fraction of the diameter of a proton.
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Schwarzschild Radius

The Schwarzschild radius is a measure of the size of the event horizon of a black hole, representing the radius at which the escape velocity equals the speed of light. When two black holes approach each other and their Schwarzschild radii overlap, they can merge into a single black hole. This concept is crucial for understanding the conditions under which gravitational waves are generated during such cosmic events.
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Energy-Mass Equivalence (E=mc²)

Einstein's equation E=mc² expresses the principle of energy-mass equivalence, stating that mass can be converted into energy and vice versa. In the context of merging black holes, the energy radiated as gravitational waves can be expressed as a fraction of Mc², where M is the mass of the system. This relationship highlights how significant amounts of energy can be released during extreme astrophysical events, such as black hole mergers.
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