MolaKule
Staff member
Gravity Waves: Evidence for Black Holes&Relativity.
A Semi-Technical Summary
by MolaKule
Back in 2006, theorists predicted the basic shape and timing of these waves based upon the inspiriling and merger of two black holes. [B.]
Gravity waves are a necessary result of the field equations of Einsteins General Theory of Relativity [A. Einstein, Reports of the Physical-Mathematical Session of the Prussion Academy, 1916, p. 689 and 1918, p. 154].
Similar to the Maxwell equations that predicted radio waves, due to accelerating charges (electrons) on an antenna, Einsteins field equations predicted that accelerating masses should make waves in the fabric of space moving at the speed of light. Very compact but massive objects, such as Neutron Stars, would be the most likely subjects for verification of Gravity Waves.
The signals detected by LIGO suggested that two large but compact masses (Black Holes), about 36 and 29 Solar Masses, had merged to about 62 Solar Masses. Now 36 + 29 = 65 Solar Masses.
65 Solar Masses - 62 Solar Masses = 3 Solar Masses. So how do we account for the missing 62 Solar Masses?
The difference of 3 Solar Masses was radiated as gravity-wave energy. The gravity wave was emited not as light in the EM spectrum, but as gravity-wave energy in the gravity- wave spectrum. Knowing the "brightness" of the gravity-wave, the LIGO team was able to determine the distance of the Black Holes merger with respect to earth.
So another of Albert Einstein's gravitational field equations has been verified using modern detection equipment such as LIGO.
References:
A. Abbot, B.P, et. al., Observation of gravitational waves from a binary black hole merger, Physical Review Letters, 116:061102, 2016.
B. Baker, J.G., et. al., Gravitational-wave extraction from an inspiriling configuration of merging black holes, Physical Review Letters, 96:111102, 2006.
C. Talor J.H., and J.M. Weisberg, A new test of general relativity: Gravitational radiation and the binary pulsar PSR 1913+16. Astrophysical Journal 253:, 1982.
For some background information on LIGO before the actual detection see:
LIGO and the Detection of Gravitational Waves, Physics Today, Oct. 1999, pp. 44-50.
LIGO and Gravitational Waves
A Semi-Technical Summary
by MolaKule
Back in 2006, theorists predicted the basic shape and timing of these waves based upon the inspiriling and merger of two black holes. [B.]
Gravity waves are a necessary result of the field equations of Einsteins General Theory of Relativity [A. Einstein, Reports of the Physical-Mathematical Session of the Prussion Academy, 1916, p. 689 and 1918, p. 154].
Similar to the Maxwell equations that predicted radio waves, due to accelerating charges (electrons) on an antenna, Einsteins field equations predicted that accelerating masses should make waves in the fabric of space moving at the speed of light. Very compact but massive objects, such as Neutron Stars, would be the most likely subjects for verification of Gravity Waves.
The signals detected by LIGO suggested that two large but compact masses (Black Holes), about 36 and 29 Solar Masses, had merged to about 62 Solar Masses. Now 36 + 29 = 65 Solar Masses.
65 Solar Masses - 62 Solar Masses = 3 Solar Masses. So how do we account for the missing 62 Solar Masses?
The difference of 3 Solar Masses was radiated as gravity-wave energy. The gravity wave was emited not as light in the EM spectrum, but as gravity-wave energy in the gravity- wave spectrum. Knowing the "brightness" of the gravity-wave, the LIGO team was able to determine the distance of the Black Holes merger with respect to earth.
So another of Albert Einstein's gravitational field equations has been verified using modern detection equipment such as LIGO.
References:
A. Abbot, B.P, et. al., Observation of gravitational waves from a binary black hole merger, Physical Review Letters, 116:061102, 2016.
B. Baker, J.G., et. al., Gravitational-wave extraction from an inspiriling configuration of merging black holes, Physical Review Letters, 96:111102, 2006.
C. Talor J.H., and J.M. Weisberg, A new test of general relativity: Gravitational radiation and the binary pulsar PSR 1913+16. Astrophysical Journal 253:, 1982.
For some background information on LIGO before the actual detection see:
LIGO and the Detection of Gravitational Waves, Physics Today, Oct. 1999, pp. 44-50.
LIGO and Gravitational Waves
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