lpetrich
Contributor
Troubled Times for Alternatives to Einstein’s Theory of Gravity | Quanta Magazine
Only adding to what they have already suffered: The Confrontation between General Relativity and Experiment | SpringerLink. Here is a rundown.
An important feature of gravity is its independence of composition. This makes gravity look like acceleration, and Albert Einstein had proposed that they are fundamentally identical: his Equivalence Principle. This led him to conclude that gravity is due to space-time being curved, and he also developed a theory for the origin of that curvature: general relativity. Here are versions of the EP:
Violations of the EP may be interpreted as the result of a "fifth force", so these upper limits also place upper limits on such possible interactions.
Even if gravity is due to space-time curvature, there is still the question of how that curvature is related to mass density, or more precisely, mass/energy/momentum density/flux and pressure. General relativity is a simple possible relation, but still only one possible relation, and various physicists have devised a variety of others. These are all adjusted to give the correct Newtonian limit, but they differ when one expands in a series beyond that. The first step in this expansion is called post-Newtonian, the second step post-post-Newtonian, etc. One can capture the predictions of general relativity and most proposed alternatives by using 10 parameters in the "parametrized post-Newtonian" formalism.
Five of these parameters are for violation of conservation of energy, linear momentum, and angular momentum, and three of them for preferred-frame effects, with one parameter shared. Constraints on them vary from around 0.02 to 4*10^(-20), with a median of 4*10^(-5).
Here are the remaining three parameters.
Parameter (gamma) is the ratio of (space distortion by gravity) / (time distortion by gravity). For slow-moving objects, one only sees a time-distortion effect, and this effect only indirectly as Newton's law of gravity. This time-distortion effect is more readily observable as gravitational redshift. But for anything traveling at c, space distortion will have an effect on its travels that is (gamma) times the time-distortion effect, giving
(value) = (1 + (gamma)) * (Newtonian value)
General relativity predicts (gamma) = 1, and that is why GR's deflection of light is twice as large as Soldner's Newtonian value.
For deflection of visible light, this parameter's departure from 1 is less than 0.01. For deflection of radio waves, it is less than 10^(-4), and for delay of radio waves, it is less than 10^(-5).
(beta) is the relative amount of nonlinearity in the time-distortion effect as a function of the Newtonian gravitational potential. It enters into the pericenter precession of an object in an orbit. In the Solar System, Mercury has the largest effect of any planet, and one that was discovered as an excess over what was predicted from Newtonian gravity. It was first attributed to an intra-Mercurian planet or planets or asteroid belt, but such intra-Mercurian objects were never convincingly observed.
From Mercury's orbit, the departure of (beta) from GR's value, 1, is less than about 10^(-4).
(eta) is the relative size of the "Nordtvedt effect", the amount of violation of the Strong Equivalence Principle. It is the difference between the amount of gravity for gravitational self-energy and the amount of gravity for everything else. GR predicts zero difference, but many GR alternatives predict nonzero difference.
This effect has been searched for by tracking the motion of the Moon, and that gives an upper limit on |(eta)| of about 10^(-3).
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So it's remarkable what we have been able to do with Solar-System tests of general relativity. The main surviving alternative is something called the Generalized Brans-Dicke theory. It features an extra field, a scalar field, one without any built-in direction, and that field makes the gravitational constant vary. How much it does that is a free parameter in the theory, and one that can be made arbitrarily small. The parameter limits give that parameter an upper limit of about 10^(-5). Thus, GBD would have to be very close to GR.
Only adding to what they have already suffered: The Confrontation between General Relativity and Experiment | SpringerLink. Here is a rundown.
An important feature of gravity is its independence of composition. This makes gravity look like acceleration, and Albert Einstein had proposed that they are fundamentally identical: his Equivalence Principle. This led him to conclude that gravity is due to space-time being curved, and he also developed a theory for the origin of that curvature: general relativity. Here are versions of the EP:
- Weak EP: all nongravitational mass makes the same gravity
- Einstein EP: the WEP with Local Lorentz Invariance (velocity invariance) and Local Position Invariance
- Strong EP: the EEP where all mass makes the same gravity, including gravitational self-energy
Violations of the EP may be interpreted as the result of a "fifth force", so these upper limits also place upper limits on such possible interactions.
Even if gravity is due to space-time curvature, there is still the question of how that curvature is related to mass density, or more precisely, mass/energy/momentum density/flux and pressure. General relativity is a simple possible relation, but still only one possible relation, and various physicists have devised a variety of others. These are all adjusted to give the correct Newtonian limit, but they differ when one expands in a series beyond that. The first step in this expansion is called post-Newtonian, the second step post-post-Newtonian, etc. One can capture the predictions of general relativity and most proposed alternatives by using 10 parameters in the "parametrized post-Newtonian" formalism.
Five of these parameters are for violation of conservation of energy, linear momentum, and angular momentum, and three of them for preferred-frame effects, with one parameter shared. Constraints on them vary from around 0.02 to 4*10^(-20), with a median of 4*10^(-5).
Here are the remaining three parameters.
Parameter (gamma) is the ratio of (space distortion by gravity) / (time distortion by gravity). For slow-moving objects, one only sees a time-distortion effect, and this effect only indirectly as Newton's law of gravity. This time-distortion effect is more readily observable as gravitational redshift. But for anything traveling at c, space distortion will have an effect on its travels that is (gamma) times the time-distortion effect, giving
(value) = (1 + (gamma)) * (Newtonian value)
General relativity predicts (gamma) = 1, and that is why GR's deflection of light is twice as large as Soldner's Newtonian value.
For deflection of visible light, this parameter's departure from 1 is less than 0.01. For deflection of radio waves, it is less than 10^(-4), and for delay of radio waves, it is less than 10^(-5).
(beta) is the relative amount of nonlinearity in the time-distortion effect as a function of the Newtonian gravitational potential. It enters into the pericenter precession of an object in an orbit. In the Solar System, Mercury has the largest effect of any planet, and one that was discovered as an excess over what was predicted from Newtonian gravity. It was first attributed to an intra-Mercurian planet or planets or asteroid belt, but such intra-Mercurian objects were never convincingly observed.
From Mercury's orbit, the departure of (beta) from GR's value, 1, is less than about 10^(-4).
(eta) is the relative size of the "Nordtvedt effect", the amount of violation of the Strong Equivalence Principle. It is the difference between the amount of gravity for gravitational self-energy and the amount of gravity for everything else. GR predicts zero difference, but many GR alternatives predict nonzero difference.
This effect has been searched for by tracking the motion of the Moon, and that gives an upper limit on |(eta)| of about 10^(-3).
-
So it's remarkable what we have been able to do with Solar-System tests of general relativity. The main surviving alternative is something called the Generalized Brans-Dicke theory. It features an extra field, a scalar field, one without any built-in direction, and that field makes the gravitational constant vary. How much it does that is a free parameter in the theory, and one that can be made arbitrarily small. The parameter limits give that parameter an upper limit of about 10^(-5). Thus, GBD would have to be very close to GR.