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Big Bang Theory and Matter |
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| Mar29-12, 04:29 AM | #1 |
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Big Bang Theory and Matter
How does the BB theory allow for the creation of matter. Bt this I mean the sub atomic particles that make up atoms i.e. the quarks and electrons. From what I have read it seems to assume that they already pre-existed and condensed out of the fireball to form atoms.
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| Mar29-12, 08:08 AM | #2 |
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The big bang model does not address the origin of matter/energy in the universe.
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| Mar29-12, 10:54 AM | #3 |
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"Big Bang" really mean two different things (1) the singularity / t=0 / the "big bang event" --- this is the place where our theories totally break down and current science has no idea what happened here. (2) The evolution of the universe starting one Plank Time AFTER the singularity. At this starting point, the universe was WAY more dense and hot than it is now, although that does NOT imply that it was finite. Lots of stuff happened. Over time, energy coalesced into matter. I commend to your reading "The First Three Minutes" by Weinberg. |
| Mar29-12, 12:28 PM | #4 |
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Big Bang Theory and Matter |
| Mar29-12, 12:36 PM | #5 |
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| Mar29-12, 02:38 PM | #6 |
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I wasn't talking about virtual particle production (i.e. vacuum fluctuations) at all, just boring old particle physics. |
| Mar29-12, 02:40 PM | #7 |
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| Mar29-12, 03:52 PM | #8 |
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The original big bang theory formulated by Lemaitre and Friedman did indeed assert that all of the matter had being compressed into a singularity, but today we've improved upon this. The standard model of the origin of the universe is known as inflation. In very simple terms, inflation speculates that the universe is filled with an inflaton field. This field would have been at a very high energy at the beginning of the universe, violently fluctuating between different values. Eventually, it would fall down into a false vacuum. In order to reach a true vacuum, it would need to exert a huge force, resulting in an enormous negative pressure. In general relativity, negative pressures result in repulsive gravity, expanding the universe by a factor near 100100, for about 10-35 seconds. Now, imagine a car trying to drive, but it is held back by an extraordinarily tense rubber band. As it continued to try to break free, it would pass it's energy to the rubber band holding it in place. Similarly, imagine a rocket trying to escape from a huge gravitational field. The gravity would build up huge amounts of energy. During inflation, something similar happened with gravity. It built up enormous emounts of energy, and then at the end of inflation, dumped large amounts of energy into the universe. Since energy and mass are related through E=mc2, we know this energy would eventually manifest as matter. |
| Mar30-12, 01:08 AM | #9 |
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1. Our universe, at very early times, was incredibly, unbelievably hot (as in hotter than the temperatures available in the collisions at the LHC). This extremely high temperature meant that particles were continuously colliding with one another, producing new matter/anti-matter particle pairs. So the universe was this giant jumble of matter and anti-matter. 2. One or more of the heavier particles that existed at this time tended to decay just a little bit more into matter than anti-matter. This meant that at very early times, there was a teeny tiny bit more matter than anti-matter (around one part in a billion, if memory serves). 3. As our universe cooled, the matter and anti-matter annihilated, eventually leaving behind the tiny excess of normal matter that built up when our universe was much hotter. Please understand that step (2) here is not currently known in detail. If we're lucky, the LHC will shed some light on this issue. |
| Mar30-12, 12:35 PM | #10 |
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A couple of points regarding answers.
Mark if gravity was involved at the start then at the singularity it would have been infinite re black holes so how could anything escape?. Regarding baryogenisis 1 billion antimatter + 1 billion and 1 matter = 2 billion and 1 universes coming out of the BB (2 billion anhilated) that is a lot to come out of a singularity. The obvious other question is is it reasonable to think that all that temperature and energy spontainiously came into being. Has anyone ever tried to create matter out of energy, we create energy from matter in neuclear reactions but is it possible to reverse the process? |
| Mar30-12, 12:50 PM | #11 |
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| Mar30-12, 02:05 PM | #12 |
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Did you happen to see this paper of Leonard Parker and a PhD student of his named Ivan Agullo? If so I'd really like to know what you think about it. There's an earlier more technical account in Physical Review D, but this is their essay for wider audience: http://arxiv.org/abs/1106.4240 Stimulated creation of quanta during inflation and the observable universe Ivan Agullo, Leonard Parker (Submitted on 21 Jun 2011) Inflation provides a natural mechanism to account for the origin of cosmic structures. The generation of primordial inhomogeneities during inflation can be understood via the spontaneous creation of quanta from the vacuum. We show that when the corresponding stimulated creation of quanta is considered, the characteristics of the state of the universe at the onset of inflation are not diluted by the inflationary expansion and can be imprinted in the spectrum of primordial inhomogeneities. The non-gaussianities (particularly in the so-called squeezed configuration) in the cosmic microwave background and galaxy distribution can then tell us about the state of the universe that existed at the time when quantum field theory in curved spacetime first emerged as a plausible effective theory. Comments: Awarded with the First Prize in the Gravity Research Foundation Essay Competition 2011 We're familiar with other cases where geometric circumstances create real (not virtual) particles e.g. Hawking radiation at BH horizon and Unruh radiation caused by acceleration or felt by an accelerated observer. So it seems that expansion of geometry itself, especially inflation, can produce matter. And Leonard Parker seems to consider this significant. Ivan Agullo is giving an invited talk about this next week at the Atlanta APS meeting. So I'm kind of excited and would be interested if you have a comment. |
| Mar30-12, 02:45 PM | #13 |
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Thanks Marcus. I will happily check it out. You mention that
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| Mar30-12, 03:34 PM | #14 |
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| Mar30-12, 04:37 PM | #15 |
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i.e. if the imbalance was on the order of 1/100th of a %, and that left behind a universe of 1060 particles, then the original number of particles must have been 2x1064. |
| Mar30-12, 06:23 PM | #16 |
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| Mar30-12, 10:43 PM | #17 |
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http://meetings.aps.org/Meeting/APR12/Event/170160 Beyond the standard inflationary paradigm The inflationary paradigm provides a compelling argument to account for the origin of the cosmic inhomogeneities that we observe in the CMB and galaxy distribution. In this talk we introduce a completion of the inflationary paradigm from a (loop) quantum gravity point of view, by addressing gravitational issues that have been open both for the background geometry and perturbations. These include a quantum gravity treatment of the Planck regime from which inflation arises, and a clarification of what the trans-Planckian problems are and what they are not. In addition, this approach provides examples of effects that may have observational implications, that may provide a window to test the basic quantum gravity principles employed here. ========= This abstract leaves me puzzled. But the same research is the subject of a recorded online talk by William Nelson. It's about a paper by Ashtekar, Agullo, Nelson that has not come out yet. It uses the Parker and Agullo results about *stimulated* fluctuations. I get the impression their idea is that inflation does not wipe the slate clean. Somehow earlier inhomogeneities might come through. So I'm puzzled, but also excited by what I'm hearing about.: |
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