Skip to main content

All Questions

Tagged with or
-7 votes
0 answers
88 views

I have a 7 page document that outlines the current 4 major anomalies. Universal expansion (dark matter), voids, early star formation, and local galactic environment) and a possible radical explanation ...
tony haigh's user avatar
2 votes
0 answers
101 views

Please excuse if this question sounds naïve — my aim is simply to understand the different kinds of gravity models. In Wikipedia there is this animation about galaxy rotation curves: without dark ...
Scibo's user avatar
  • 87
1 vote
0 answers
90 views

For the cubic gravity with Lagrangian $$ \sqrt{-g} \left(R+\frac{1}{\Lambda^4}R_{\mu \nu}{ }^{\alpha \beta} R_{\alpha \beta}{ }^{\gamma \sigma} R_{\gamma \sigma}{ }^{\mu \nu}\right), $$ where $\Lambda$...
Thomas's user avatar
  • 11
0 votes
0 answers
91 views

To explain observed “flat” rotation curves of galaxies, “Milgrom’s Law” Modified Newtonian Dynamics (MOND) “kicks in” at gravitational accelerations below $a_0 \sim 10^{-10}~\mathrm{m/s^2}$. But ...
Jere's user avatar
  • 19
1 vote
1 answer
110 views

(re-typing this question because screenshots aren't welcome) Hello, I am currently studying Compact Stars in the $R + \alpha R^2$ model of gravity. In this model, our field equations take the ...
varun's user avatar
  • 13
0 votes
0 answers
138 views

The Brans-Dicke theory is a scalar-tensor theory of gravity that introduces a scalar field $\phi$ to account for a varying gravitational constant. It is a generalization of general relativity. In the ...
John Eastmond's user avatar
1 vote
1 answer
86 views

Can anyone point me to a paper where they give the field equations for the following modified Brans-Dicke action with non-minimal coupling to matter $$S = \frac{1}{16 \pi}\int d^4x\sqrt{-g} \left(\phi ...
0 votes
0 answers
99 views

The Brans-Dicke action is generally given by: $$S = \frac{1}{16 \pi}\int d^4x\sqrt{-g} \left(\phi R - \frac{\omega}{\phi}\partial_a\phi\partial^a\phi\right) + \int d^4 x \sqrt{-g} \,\mathcal{L}_\...
John Eastmond's user avatar
0 votes
1 answer
120 views

If we model the fall-off of gravity as $1/r^e$, the newtonian model has $e=2$, giving the well know $1/r^2$. This yields a steady state elliptical orbit. How would the orbit change for $e<2$ (which ...
River Model's user avatar
1 vote
0 answers
90 views

I'm currently going through John D. Barrow and S. Cotsakis' 1988 paper "INFLATION AND THE CONFORMAL STRUCTURE OF HIGHER-ORDER GRAVITY THEORIES" (https://doi.org/10.1016/0370-2693(88)90110-4)....
PhysicsPanda's user avatar
2 votes
0 answers
57 views

I attended a seminar today about modified gravity theories - broadly things like $f(R)$ gravity. The speaker talked through screening mechanisms and how they could depend on the local density and, in ...
Kyle Oman's user avatar
  • 19k
0 votes
0 answers
87 views

I am considering the action (inspired by MOND) given by $$\mathcal{L} = f( (\nabla^\mu \phi \nabla_\mu \phi)^2 )$$ where $f$ is an arbitrary function. But I want to get it from a Newtonian ...
bob's user avatar
  • 397
1 vote
1 answer
128 views

According to Wikipedia, Standard Newtonian gravity might not hold for smaller than $10^{-10}\ \mathrm{m/s^2}$ accelerations and Modified Newtonian Dynamics might explain the differences. If I ...
DrMushroom's user avatar
6 votes
1 answer
215 views

MOND attempts to solve the rotation curve problem of galaxies by modifying the law of gravitation. However, there are galaxies (notably NGC 1277) where the rotation curves do more-or-less agree with ...
H. de Gracht's user avatar
1 vote
0 answers
100 views

I get below the following contours of a MCMC run with the main cosmological parameters for Brans-Dickce's theory without introducing a cosmological constant ($\Lambda=0$) and considering only baryonic ...
guizmo133's user avatar

15 30 50 per page
1
2 3 4 5
13