Nonlinear gravity as a classical field theory

In summary, nonlinear gravity is a classical field theory that describes the gravitational force as a field in spacetime, incorporating the principles of Einstein's general theory of relativity. It differs from linear gravity in that it takes into account the curvature of spacetime, meaning the force of gravity is influenced by the geometry of spacetime rather than solely by mass and distance. This has significant implications for our understanding of the universe, as it can explain phenomena such as black holes and gravitational waves. Nonlinear gravity is primarily tested and validated through observations and experiments, and while it is mainly a theoretical framework, it has practical applications in fields such as astrophysics and cosmology. Additionally, it has potential applications in engineering, such as improving space travel methods.
  • #1
spaghetti3451
1,344
33

Homework Statement



In this problem, you will calculate the perihelion shift of Mercury simply by dimensional analysis.

(a) The interactions in gravity have

##\mathcal{L}=M^{2}_{Pl}\Big(-\frac{1}{2}h_{\mu\nu}\Box h_{\mu\nu}+(\partial_{\alpha}h_{\mu\nu})(\partial_{\beta}h_{\mu\alpha})h_{\nu\beta}+\cdots\Big)-h_{\mu\nu}T_{\mu\nu},\qquad\qquad (1)##

where ##M_{Pl}=\frac{1}{\sqrt{G_{N}}}## is the Planck scale. Rescaling ##h##, and dropping indices and numbers of order ##1##, this simplifies to

##\mathcal{L}=-\frac{1}{2}h\Box h+(M_{Pl})^{a}h^{2}\Box h-(M_{Pl})^{b}hT.\qquad\qquad (2)##

What are ##a## and ##b## (i.e. what are the dimensions of these terms)?

(b) The equations of motion following from this Lagrangian are (roughly)

##\Box h = (M_{Pl})^{a}\Box (h^{2})-(M_{Pl})^{b}T.\qquad\qquad (3)##

For a point source ##T=m\delta^{(3)}(x)##, solve Eq. (3) for ##h## to second order in the source ##T## (or equivalently to third order in ##M_{Pl}^{-1}##). You may use the Coulomb solution we already derived.

(c) To first order, ##h## is just the Newtonian potential. This causes Mercury to orbit. What is Mercury's orbital frequency, ##\omega=\frac{2\pi}{T}##? How does it depend on ##m_{\text{Mercury}}##, ##m_{\text{Sun}}##, ##M_{Pl}## and the distance ##R## between Mercury and the Sun?

(d) To second order, there is a correction that causes a small shift Mercury's orbit. Estimate the order of magnitude of the correction to ##w## in arcseconds/century using your second-order solution.

(e) Estimate how big the effect is of other planets on Mercury's orbital frequency. (Dimensional analysis will do - just get the right powers of masses and distances.)

(f) Do you think the shifts from either the second-order correction or from the other planets should be observable for Mercury? What about for Venus?

(g) If you derive Eq. (3) from Eq. (2), what additional terms do you get? Why is it OK to use Eq. (3) without these terms?

Homework Equations



The Attempt at a Solution



(a) I understand what it means to rescale ##h## and drop indices.

In particular, for the first term, ##h\Box h = M^{2}_{Pi}h_{\mu\nu}\Box h_{\mu\nu}## so that ##h=M^{2}_{Pi}h_{\mu\nu}.##

Therefore, for the third term, ##h_{\mu\nu}T_{\mu\nu}=(M_{Pl})^{b}hT## which implies ##h_{\mu\nu}T_{\mu\nu}=(M_{Pl})^{b}(M_{Pl}h_{\mu\nu})T## so that ##b=-1.##What does it mean to drop numbers of order ##1##? What are the numbers of order ##1## here anyway?
 
  • #3
failexam said:

Homework Statement



In this problem, you will calculate the perihelion shift of Mercury simply by dimensional analysis.

(a) The interactions in gravity have

##\mathcal{L}=M^{2}_{Pl}\Big(-\frac{1}{2}h_{\mu\nu}\Box h_{\mu\nu}+(\partial_{\alpha}h_{\mu\nu})(\partial_{\beta}h_{\mu\alpha})h_{\nu\beta}+\cdots\Big)-h_{\mu\nu}T_{\mu\nu},\qquad\qquad (1)##

where ##M_{Pl}=\frac{1}{\sqrt{G_{N}}}## is the Planck scale. Rescaling ##h##, and dropping indices and numbers of order ##1##, this simplifies to

##\mathcal{L}=-\frac{1}{2}h\Box h+(M_{Pl})^{a}h^{2}\Box h-(M_{Pl})^{b}hT.\qquad\qquad (2)##

What are ##a## and ##b## (i.e. what are the dimensions of these terms)?

(b) The equations of motion following from this Lagrangian are (roughly)

##\Box h = (M_{Pl})^{a}\Box (h^{2})-(M_{Pl})^{b}T.\qquad\qquad (3)##

For a point source ##T=m\delta^{(3)}(x)##, solve Eq. (3) for ##h## to second order in the source ##T## (or equivalently to third order in ##M_{Pl}^{-1}##). You may use the Coulomb solution we already derived.

(c) To first order, ##h## is just the Newtonian potential. This causes Mercury to orbit. What is Mercury's orbital frequency, ##\omega=\frac{2\pi}{T}##? How does it depend on ##m_{\text{Mercury}}##, ##m_{\text{Sun}}##, ##M_{Pl}## and the distance ##R## between Mercury and the Sun?

(d) To second order, there is a correction that causes a small shift Mercury's orbit. Estimate the order of magnitude of the correction to ##w## in arcseconds/century using your second-order solution.

(e) Estimate how big the effect is of other planets on Mercury's orbital frequency. (Dimensional analysis will do - just get the right powers of masses and distances.)

(f) Do you think the shifts from either the second-order correction or from the other planets should be observable for Mercury? What about for Venus?

(g) If you derive Eq. (3) from Eq. (2), what additional terms do you get? Why is it OK to use Eq. (3) without these terms?

Homework Equations



The Attempt at a Solution



(a) I understand what it means to rescale ##h## and drop indices.

In particular, for the first term, ##h\Box h = M^{2}_{Pi}h_{\mu\nu}\Box h_{\mu\nu}## so that ##h=M^{2}_{Pi}h_{\mu\nu}.##

Therefore, for the third term, ##h_{\mu\nu}T_{\mu\nu}=(M_{Pl})^{b}hT## which implies ##h_{\mu\nu}T_{\mu\nu}=(M_{Pl})^{b}(M_{Pl}h_{\mu\nu})T## so that ##b=-1.##What does it mean to drop numbers of order ##1##? What are the numbers of order ##1## here anyway?
They mean the terms of order ##M_{Pl}^0 ##, i.e. with no factors of the Planck mass. These would appear if one would include more of the terms that are not shown (where the three dots are). These three dots contain terms that contain factors ##\frac{1}{M_P^2}, \frac{1}{M_P^4} ## and so on. Since they get multiplied by ##M_P^0##, they start at order ##M_P^0##. They therefore basically mean that one should neglect all the terms that are implicitly contained in the three dots.
 

1. What is nonlinear gravity as a classical field theory?

Nonlinear gravity as a classical field theory is a theoretical framework that describes the gravitational force as a field in spacetime, similar to other fundamental forces such as electromagnetism. However, unlike linear gravity, which follows the laws of classical mechanics, nonlinear gravity incorporates the principles of Einstein's general theory of relativity, which accounts for the curvature of spacetime.

2. How does nonlinear gravity differ from linear gravity?

Linear gravity is based on Newton's laws of motion, which describe the force of gravity as a linear function of mass and distance. Nonlinear gravity, on the other hand, incorporates the curvature of spacetime, meaning that the force of gravity is not directly proportional to mass and distance, but rather is influenced by the geometric properties of spacetime itself.

3. What are the implications of nonlinear gravity on our understanding of the universe?

The incorporation of nonlinear effects in gravity has significant implications for our understanding of the universe. It allows for the explanation of phenomena such as black holes, gravitational waves, and the expansion of the universe, which cannot be fully explained by linear gravity alone.

4. How is nonlinear gravity tested and validated?

Nonlinear gravity is primarily tested and validated through observations and experiments, particularly in the study of astronomical phenomena. For example, the detection of gravitational waves by the LIGO experiment provided strong evidence for the existence of nonlinear effects in gravity.

5. Are there any practical applications of nonlinear gravity?

While nonlinear gravity is primarily a theoretical framework, it has practical applications in fields such as astrophysics and cosmology. It also has potential applications in engineering, such as the development of more accurate and efficient space travel methods.

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