The sign of the cosmological term

In summary, the cosmological term in the Einsetin equation is a combination of two different types of energy (positive and negative) and represents the pressure of the universe.
  • #1
sweet springs
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I want to know the sign of the cosmological term. It seems that in the left hand side of the Einsetein equation the cosmological term is [itex]-\Lambda g_{ik}[/itex] for (+---) convetion or [itex]+\Lambda g_{ik}[/itex] for (-+++) convetion. Right?
Best
 
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  • #2
That makes intuitive sense to me. I hope someone shows up who can confirm this more authoritatively. The reason it makes sense to me as a non-expert is that Λ shows up with a minus sign in the Friedmann equation in cosmology. The Friedmann is supposed to be derived from the "0 0" component of the GR equation , that is from the "t t" components term by term. And the Friedmann equation looks like this:
H2 - Λc2/3 = [constant] ρ

where H is a fractional growth rate with dimension Time-1 so H2 has dimension Time-2, and rho is the density.
Λ has dimension Length-2 so Λc2 also has dimension Time-2, so that is consistent.
And Λc2/3 = H2 the square of the longterm Hubble expansion rate to which H(t) is converging.

So I think of Λ as appearing with a + sign on the left side of the GR equation, in the (-+++) convention and therefore appearing with a - sign on the left side of the Friedmann.
 
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  • #4
Ibix said:
Misner, Thorne and Wheeler classify eight different conventions
Could you tell which section?
 
  • #5
Shyan said:
Could you tell which section?
The very first page (it's red in my copy) is a table of sign convention by author. There are eight possibilities in their classification scheme; I haven't actually checked that they have an example of every one in use.

Edit: The above isn't directly related to the OP's question - it was more in the vein of a general caution.
 
  • #6
Thanks for your enlightenmental replies. I would likt to know more about dark energy, i.e. cosmological term transposed to right hand side, reffering

sweet springs said:
It seems that in the left hand side of the Einsetein equation the cosmological term is [itex]-\Lambda g_{ik}[/itex] for (+---) convetion or [itex]+\Lambda g_{ik}[/itex] for (-+++) convetion.

i.e. [itex]\Lambda g_{ik}[/itex] for (+---) convetion or [itex]-\Lambda g_{ik}[/itex] for (-+++) convetion. The positive energy and the negative momentum are not usual.
I would like get some interpretation or explanation of this combination. If you know something good please let me share it.
Best.
 
  • #7
sweet springs said:
The positive energy and the negative momentum are not usual.

It's negative pressure, not negative momentum. The momentum three-vector is a vector, so it doesn't make sense to talk about whether it's positive or negative.
 
  • #8
Is pressure the momentum flux? Force/area = Momentun density * velocity of fluid = momentum flux
 

FAQ: The sign of the cosmological term

What does the cosmological term represent in the study of cosmology?

The cosmological term, also known as the cosmological constant, represents the energy density of empty space in the universe. It is a fundamental parameter in the mathematical equations used to describe the expansion of the universe.

How does the cosmological term affect the expansion rate of the universe?

The cosmological term has a repulsive effect on the expansion of the universe, causing it to accelerate. This is because it acts as a form of energy that counteracts the gravitational pull of matter, leading to an overall increase in the expansion rate.

Is the value of the cosmological term constant or does it change over time?

The value of the cosmological term is believed to be constant, meaning it does not change over time. This is based on current observations and theoretical models, but further research is still being conducted to better understand the nature of the cosmological term.

How does the cosmological term relate to dark energy?

The cosmological term is often used interchangeably with the term "dark energy". This is because dark energy is thought to be responsible for the observed acceleration of the universe, and the cosmological term is the mathematical representation of this energy.

What are the implications of the cosmological term for the fate of the universe?

The value of the cosmological term has significant implications for the future of the universe. If the value is large enough, it could lead to a "Big Rip" scenario where the universe expands at an ever-increasing rate, tearing apart all structures and eventually leading to a cold, empty universe. If the value is smaller, the universe may continue to expand at a slower rate or even eventually collapse in a "Big Crunch" scenario.

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