Solving Freidmann Equation: Understand Calculations & Cosmology

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In summary, the conversation is about seeking help understanding the Friedmann equation and its components, including the dot symbol representing a time derivative and the k symbol representing the spatial curvature of the Universe. The conversation also mentions the importance of learning physics from the ground up rather than starting with a complex equation. The expert recommends starting with the Wikipedia article on the Friedmann equations for further reading.
  • #1
AleksanderPhy
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Hello there I may have physical mistakes and stupid question so say if I have something wrong. But I want to get help on Freidmann equation.It looks like this:
lamfried.gif
So first I want to know what that What you can calculate with this equation. Second question is what's the little point on capital r. And what's the k ?

PS! Can I get some webpages where I can read about cosmology.
 
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  • #2
Honestly, taking an equation you do not understand out of its context and trying to understand it is not the best way to learn physics. You need to work from the ground up, not the other way around.

The dot represents a time derivative, the k is the spatial curvature of the Universe, and the Friedmann equation is used to compute how the universe expands.
 
  • #3
Thanks
 
  • #5
Ok thanks(;
 

FAQ: Solving Freidmann Equation: Understand Calculations & Cosmology

What is the Friedmann equation and why is it important in cosmology?

The Friedmann equation is a fundamental equation in cosmology that describes the evolution of the universe. It relates the expansion rate of the universe to its energy content and curvature. It is important because it allows us to understand the dynamics of the universe and make predictions about its future.

How is the Friedmann equation derived?

The Friedmann equation is derived from Einstein's theory of general relativity, which describes the relationship between the curvature of space-time and the distribution of matter and energy. It involves solving a set of coupled differential equations that describe the evolution of the universe.

What are the key parameters in the Friedmann equation?

The key parameters in the Friedmann equation are the Hubble constant, which describes the expansion rate of the universe, the density of matter and energy in the universe, and the curvature of space-time. These parameters determine the overall evolution and fate of the universe.

How is the Friedmann equation used to understand the expansion of the universe?

The Friedmann equation is used to understand the expansion of the universe by calculating the Hubble parameter at different times in the past and future. This allows us to determine the rate of expansion and how it changes over time, providing insight into the overall expansion history of the universe.

How does the Friedmann equation relate to dark energy and dark matter?

The Friedmann equation includes terms for both dark energy and dark matter, which are two of the main components of the universe that cannot be directly observed. These terms play a crucial role in shaping the expansion of the universe and are essential in understanding its overall evolution.

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