Time after big bang we can observe, uncertainty principle

In summary, the Planck wavelength and event horizon are used to determine the uncertainty in what we can see if we were to look back in time to the big bang. We can only see back to 10^-43 seconds after the big bang, so the Compton wavelength and Schwarzschild radius are important to understand.
  • #1
Finestructure
5
0
Can someone explain why the compton wavelength and event horizon are used to determine the uncertainty in what we can see if we were to look back in time to the big bang. (We can only see back to 10^-43 seconds after the big bang.)

Here's a website that derives this time (Planck time)

http://hyperphysics.phy-astr.gsu.edu/HBASE/astro/planck.html
 
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  • #2
Finestructure said:
Can someone explain why the compton wavelength and event horizon are used to determine the uncertainty in what we can see if we were to look back in time to the big bang. (We can only see back to 10^-43 seconds after the big bang.)

Here's a website that derives this time (Planck time)

http://hyperphysics.phy-astr.gsu.edu/HBASE/astro/planck.html

"Fine"; we can't see back in time. Sorry to burst your bubble.
 
  • #3
Ah, yes we can. We do it every day. In fact, right at this very instant I am studying an object as it was 3.5 billion years ago. I used a radio telescope to look back in time and see what it looked like then...
 
  • #4
The Compton wavelength of the Planck mass is equal to it’s Schwarzschild radius. The Planck mass or the Planck units provide a scale for which quantum phenomena of gravitational fields should become important. As there is still no completely successful theory of quantum gravitation those phenomena remain a mistery. To see how these both quantities set this quantum gravity scale consider a black hole for which the Compton wavelength and the Schwarzschild radius are roughly the same. In that case the radius of the event horizon and the uncertainty in the position of the object are similar. This questions the existence of the singularity and therefore the validity of general relativity.
 
  • #5
hellfire said:
The Compton wavelength of the Planck mass is equal to it’s Schwarzschild radius.

Thanks, I did not know that the Compton wavelength was associated iwth the Planck mass.
 
  • #6
Finestructure said:
Thanks, I did not know that the Compton wavelength was associated iwth the Planck mass.


The Compton wave formula is just a function of mass; put any mass in and get a wavelength (a certain length) out. The Schwartzschild radius formula from GR is another example of a function of mass that returns a length. Set 'em equal and solve for the mass, and it comes out the Planck mass. And you know what else? The common length that comes out (equal lengths by your assumption) is the Planck length. Is that significant or just a mathematical trick? Nobody knows.
 
  • #7
Not a trick IMO, SA. Just a cold, hard fact. Glad you brought that up. I see too many 'precendental' papers these days on arxiv these days that conveniently ignore this constraint [or abuse the **** out of it].
 

FAQ: Time after big bang we can observe, uncertainty principle

What is the "time after big bang" that we can observe?

The "time after big bang" refers to the time period after the Big Bang, which is believed to have occurred approximately 13.8 billion years ago. This is the moment when the universe is thought to have begun expanding rapidly and the laws of physics as we know them today began to take shape. We can observe the effects of the Big Bang through various astronomical observations and experiments.

How far back in time can we observe using the uncertainty principle?

The uncertainty principle, also known as Heisenberg's uncertainty principle, is a fundamental principle in quantum mechanics that states that there is a limit to the precision with which certain pairs of physical properties of a particle can be known simultaneously. This principle applies to all particles, including those that existed at the time of the Big Bang. Therefore, we can observe the effects of the uncertainty principle in the earliest moments of the universe's existence.

What is the significance of the "time after big bang" that we can observe?

The time after the Big Bang that we can observe is significant because it provides us with a glimpse into the earliest moments of the universe's existence. By studying the effects of the Big Bang and the uncertainty principle, we can gain a better understanding of the laws of physics and the evolution of the universe over time.

How does the uncertainty principle impact our understanding of the Big Bang?

The uncertainty principle plays a crucial role in our understanding of the Big Bang. It helps explain the origins of the universe and the behavior of particles in the early stages of the universe's existence. Without the uncertainty principle, our current understanding of the Big Bang and the evolution of the universe would be incomplete.

What advancements have been made in our understanding of the "time after big bang" and the uncertainty principle?

Thanks to advancements in technology and scientific research, our understanding of the time after the Big Bang and the uncertainty principle has greatly improved. Scientists continue to study the early universe and the behavior of particles, providing us with new insights and discoveries that contribute to our understanding of the universe's origins.

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