Question regarding pre-bigbang detection.

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Discussion Overview

The discussion revolves around the possibility of detecting phenomena from the pre-Big Bang era, particularly focusing on the coupling of matter and radiation in the early universe. Participants explore theoretical approaches to capturing images or signals from this opaque phase, including the roles of neutrinos and gravitational waves.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions whether it is possible to capture an image of the coupling of matter and radiation before the universe became transparent, suggesting that theoretical particles might be detectable.
  • Another participant explains that photons could not escape the early universe due to its density, while neutrinos could penetrate this "fog" shortly after the Big Bang, although constructing a neutrino telescope poses significant challenges.
  • There is a suggestion that gravity also penetrated the primordial soup, and efforts to detect primordial gravitational waves are ongoing and considered more feasible.
  • Some participants propose that if gravity and neutrinos can penetrate the early universe, it implies that the universe is much larger than what is currently visible, with estimates potentially based on the propagation rates of gravitational waves compared to light.
  • One participant agrees that the universe is indeed larger than the visible part and suggests that detecting primordial gravitational waves could provide insights into this larger region.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the detection of pre-Big Bang phenomena, with no consensus on the feasibility of capturing images or signals from that era. The implications of gravity and neutrinos penetrating the early universe are acknowledged, but the discussion remains unresolved.

Contextual Notes

The discussion includes assumptions about the nature of the early universe and the challenges associated with detecting certain particles and waves. There are unresolved questions regarding the methods and technologies needed for such detections.

moniz
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Hi,

I'm not a physicist although I've studied it to first year degree level in the UK many many years ago. I was just reading an article today on the BBC about a new image that's been captured of the visible universe.

The following quote got me thinking and I wondered if your expert knowledge may be able to answer a question for me.

"The CMB is the "first light". It is the light that was finally allowed to move out across space once a post-Big-Bang Universe had cooled sufficiently to permit the formation of hydrogen atoms.

Before that time, scientists say, the cosmos would have been so hot that matter and radiation would have been "coupled" - the Universe would have been opaque."http://news.bbc.co.uk/1/hi/science_and_environment/10501154.stm

It begs the question has anyone tried to capture some sort of image of this coupling? I know it sounds like a crazy suggestion. Can a sort of matter image can be constructed in some way, might any such theoretical particles be detectable? I mean matter is energy (De Broglie particle waves etc). The Universe may be opaque but only to light. Apologies as my knowledge of physics is absolutely terrible at the moment. It's been about 20 years since I studied anything and I didn't go beyond special relativity and Newtonian mechanics.
 
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Photons could not escape from the early universe because it was too dense. It took about 400,000 years for it to dilute sufficiently to become transparent to photons. This, of course, was not an issue for neutrinos.They were able to penetrate the fog shortly after the big bang. Constructing a neutrino telescope is, however, a formidable challenge. Gravity was also able to penetrate the primordial soup. Efforts to detect primordial gravity waves is an active [and more feasible] area of interest in modern astrophysics.
 
Chronos said:
Photons could not escape from the early universe because it was too dense. It took about 400,000 years for it to dilute sufficiently to become transparent to photons. This, of course, was not an issue for neutrinos.They were able to penetrate the fog shortly after the big bang. Constructing a neutrino telescope is, however, a formidable challenge. Gravity was also able to penetrate the primordial soup. Efforts to detect primordial gravity waves is an active [and more feasible] area of interest in modern astrophysics.

If gravity and neutrinos are able to penetrate the early universe, surely this implies that the current universe is a lot bigger than that which is visible? A lot bigger. And this perhaps could be estimated by the rate of propagation of gravity waves as compared to light multiplied by the number of years.
 
moniz said:
If gravity and neutrinos are able to penetrate the early universe, surely this implies that the current universe is a lot bigger than that which is visible? A lot bigger. And this perhaps could be estimated by the rate of propagation of gravity waves as compared to light multiplied by the number of years.
Yes, our universe is a lot bigger than just the visible part. If we ever get to the point where we can directly detect primordial gravitational waves, for instance, we will have a window into a vastly larger region of the universe.
 

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