Help me derive the relativistic equation of motion for the Universe

In summary, the equation adot^2 = Λc^2a^2/3 represents the relationship between the scale factor and the Hubble constant. To get a(t) = a(t0)e^Ht, we can use the fact that da/dt = Ha, which leads to dt/da = 1/Ha. By integrating, we can obtain the expression a = a(t0)e^(Ht), which showcases the accelerating expansion of the Universe.
  • #1
QuantumX
31
0
Guys,

My calculus is really rusty and I need help solving this equation using a time derivative (denoted with a dot) in order to get the relativistic equation of motion for the Universe

The equation is:

adot^2 = Λc^2a^2/3

where adot is the time derivative of the scale factor, lambda is a cosmological constant, and c is the speed of light.

The answer should be:

a(t) = a(t0)e^Ht

where H is Hubble's constant = sqrt(c^2Λ/3)

But I don't know how to get there. Any help is appreciated!
 
Astronomy news on Phys.org
  • #2
Hi QuantumX! Welcome to PF! :smile:

(try using the X2 button just above the Reply box :wink:)
QuantumX said:
adot2 = Λc2a2/3

So da/dt = √(Λc2/3)a = Ha :smile:
 
  • #3
Thanks Tiny-Tim,

So then the first equation is just the relationship between the scale factor and the Hubble constant...

So how do I then get a(t) = a(t0)e^Ht ? (that is for t>t0). That's what i need to ultimately arrive at. It's supposed to showcase that the Universe is accelerating in its expansion.
 
  • #4
tiny-tim said:
So da/dt = √(Λc2/3)a = Ha :smile:
QuantumX said:
So how do I then get a(t) = a(t0)e^Ht ?

da/dt = Ha

so dt/da = 1/Ha, so t = loga/H + constant

so loga = Ht + constant

so a = eHt + constant = econstanteHt

and the econstant is a(to)
 
  • #5
Thanks!
 

FAQ: Help me derive the relativistic equation of motion for the Universe

What is the relativistic equation of motion for the Universe?

The relativistic equation of motion for the Universe is known as the Friedmann equation, named after physicist Alexander Friedmann. It describes the dynamics of the expansion of the Universe in the context of Einstein's theory of general relativity.

How is the relativistic equation of motion derived?

The relativistic equation of motion is derived by applying the principles of general relativity to the Universe as a whole. This involves using Einstein's field equations, which relate the curvature of spacetime to the distribution of matter and energy, and solving for the metric tensor that describes the geometry of the Universe.

What factors does the relativistic equation of motion take into account?

The relativistic equation of motion takes into account the distribution of matter and energy, as well as the curvature of spacetime. It also considers the cosmological constant, which represents the energy density of the vacuum and plays a role in the expansion of the Universe.

Can the relativistic equation of motion be applied to all scales of the Universe?

Yes, the relativistic equation of motion can be applied to all scales of the Universe, from the smallest subatomic particles to the largest cosmic structures. It provides a comprehensive framework for understanding the dynamics of the Universe as a whole.

How does the relativistic equation of motion contribute to our understanding of the Universe?

The relativistic equation of motion is a fundamental tool for understanding the evolution and behavior of the Universe. It allows us to make predictions about the expansion rate, age, and future fate of the Universe, and has been confirmed by numerous observations and experiments. It also plays a crucial role in the development of theories such as inflation and dark energy.

Back
Top