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Does Space Expand? |
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| Mar25-12, 04:14 PM | #154 |
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Does Space Expand?The the LCDM model scale factor is defined as: [tex]a(t) = \left[ \frac{\Omega_m}{\Omega_v} \sinh^2 \left( \frac{3}{2} \sqrt{\Omega_v} H_0 t \right) \right]^{\frac{1}{3}}[/tex] Differentiating the scale factor function with respect to t: [tex]\frac{d a(t)}{dt} = \frac{d}{dt} \left[ \frac{\Omega_m}{\Omega_v} \sinh^2 \left( \frac{3}{2} \sqrt{\Omega_v} H_0 t \right) \right]^{\frac{1}{3}} = \frac{ \Omega_m H_0 \cosh \left(\frac{3}{2} \sqrt{\Omega_v} H_0 t \right) \sinh \left(\frac{3}{2} \sqrt{\Omega_v} H_0 t \right)}{\sqrt{\Omega_v} \left(\frac{\Omega_m \sinh^2 \left(\frac{3}{2} \sqrt{\Omega_v} H_0 t \right)}{\Omega_v} \right)^{2/3}}[/tex] The scale factor derivative function: [tex]\boxed{\frac{d a(t)}{dt} = \frac{ \Omega_m H_0 \cosh \left(\frac{3}{2} \sqrt{\Omega_v} H_0 t \right) \sinh \left(\frac{3}{2} \sqrt{\Omega_v} H_0 t \right)}{\sqrt{\Omega_v} \left(\frac{\Omega_m \sinh^2 \left(\frac{3}{2} \sqrt{\Omega_v} H_0 t \right)}{\Omega_v} \right)^{2/3}}}[/tex] Is this equation correct? Attachments: plot a(t), plot a'(t) Reference: LambdaCDM geometry - mathematical details - Wikipedia |
| Mar25-12, 04:47 PM | #155 |
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I'm not good enough at the math to quickly check your solution but I believe there is no analytic solution when there is more than one phase involved. The graph is initially matter dominated but becomes energy dominated so I think you have to perform an integration to get the curve.
However, the section "mixtures" here suggests it can be solved: http://en.wikipedia.org/wiki/Friedma...eful_solutions The "Lecture notes on Astrophysics" looks comprehensive too, though beyond my level. |
| Mar26-12, 02:04 PM | #156 |
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i was thinking about light.
a particle and/or a wave ? but what about darkness.? does darkness move at the speed of light? does light move at the speed of darkness? does light really bend around corners or is it pulled around by darkness? in a dark universe, does the universe expand when light appears? does light "push" darkness away ? but what if the universe is in a "bubble"? would the darkness get squashed? is light a constant in the universe.? does the universe expand at different speeds at different times depending on how much is being added at that particular time? |
| Mar26-12, 05:19 PM | #157 |
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http://en.wikipedia.org/wiki/Universe http://en.wikipedia.org/wiki/Physical_cosmology |
| Mar26-12, 05:40 PM | #158 |
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darkness is nothing but the absence of light..... ooosh so what came first, the darkness or the light? but i thought we knew or at least thought ,that there is no such thing as nothing |
| Mar26-12, 06:52 PM | #159 |
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| Mar27-12, 07:42 AM | #160 |
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These are the scale factor equations that I reviewed from reference 1 and 2. Inflation Hubble parameter (end of inflationary epoch): 'ref. 1 p. 34 (167)' [tex]H_i = \frac{1}{t_{i}} = \frac{1}{10^{-32} \; \text{s}} = 10^{32} \; \text{s}^{-1}[/tex] [tex]\boxed{H_i = 10^{32} \; \text{s}^{-1}}[/tex] Inflation scale factor: 'ref. 1 p.35 (165)' [tex]a(t) \propto e^{H_i t} \tag{1}[/tex] Radiation scale factor: 'ref. 1 p. 22 (119)' [tex]a(t) = (2 H_0)^{\frac{1}{2}} \cdot t^{\frac{1}{2}} \tag{2}[/tex] Matter scale factor: 'ref. 1 p. 21 (115)' [tex]a(t) = \left( \frac{4 H_0}{2} \right)^{\frac{2}{3}} \cdot t^{\frac{2}{3}} \tag{3}[/tex] LCDM matter scale factor: 'ref. 2' [tex]a(t) = \left[ \frac{\Omega_m}{\Omega_v} \sinh^2 \left( \frac{3}{2} \sqrt{\Omega_v} H_0 t \right) \right]^{\frac{1}{3}} \tag{4}[/tex] Equations 2 and 3 appear to be describing a universe that is much younger. Attachments: plot 1, plot 2,3,4 Reference: Friedmann equations - useful solutions - Wikipedia Northern Illinois University - Physics 652 - Astrophysics LambdaCDM - geometry - mathematical details - Wikipedia |
| Mar27-12, 09:46 AM | #161 |
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if light was more abundant than darkness at the start where as the reverse is true now, am i to believe then that the universe is getting smaller? what if it was expanding and contracting i ask about light "pushing" darkness (light pressure) clearing a path . so if we had darkness first with energy, then light energy appears,room has to be made for this light. could light then clear this "room" creating a vacuum redundant of energy once this light has lost its energy and gone..this then takes time to rebuild itself with dark energy matter, un til it over crowds sparking another light source and repeats the process. this would mean light energy is finite but that does not mean the universe cannot expand.. i could be way off and have no idea what im on about.but ive read some say that the universe is expanding fast than light... how do we measure this.do we measure it with light? if light is "pushing" then light will always be behind therefore it could be seen that anything infront of it is moving fast when really its not |
| Mar27-12, 12:07 PM | #162 |
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| Mar27-12, 12:52 PM | #163 |
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Also, the expansion of the universe is a "rate", not a measurement of velocity. What this means is that objects further away will accelerate away from us quicker than objects closer to us will. The speed at which objects move away from us is called the recession velocity. Currently our measurements show that this recession velocity increases by about 70 km/s per megaparsec (3.26 million light-years) in distance that an object is from us. So a galaxy at 2 megaparsecs in distance from us would be receding at about 140 km/s, while a galaxy at 20 megaparsecs would recede at 1400 km/s. If the rate of expansion were higher, the recession velocity would increase by a larger amount per distance, such as being 100 km/s per megaparsec. |
| Mar27-12, 12:53 PM | #164 |
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sorry . i did mean to use the word "front" lightly .ooosh pun ,not so poetic...
yes theres no front, back, middle, only edges,curves,surrounding, enclosed ,in a tomb of darkness.. the further we look back the brighter it gets. its logic for it to be so. but is it logic to think that what one is looking at is not the beginning but a random? thanks for the reply ... also how far can my eyes see. meaning when i see light that has come from a far distance.at what distance am i seeing it.? am i seeing the light from the distance of my eye or am i seeing the light light years away. my eyes can see distances.so i ask is it possible to travel down the light to the source and bring it nearer? i no i may like a fruit loop hope you dont mind.. my question is this. is the light seeing me or am i seeing it? also i went to the optitions today.he put a light in my eye .when this light was taken away i had a dark line of vision.i asked why. he said its because the light removes something or other ,sorry cant remember exactly,so there was an empty space .but over time the energy recovers and bring the light back to this dark spot...can space work the same? meaning does light remove matter then once the light has gone this matter returns over a time period... |
| Mar27-12, 01:09 PM | #165 |
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After this recombination, atoms could finally start to collapse under gravitational attraction to form the first stars and galaxies. Whether the universe is "brighter" now or then is unknown to me. I don't know what your asking with the 3rd sentence. |
| Mar27-12, 01:50 PM | #166 |
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im now confused. one of you is saying the further you go back the brighter it gets,and the other is saying not so...
the problem may stem from the "no matter which direction we look ,it all looks the same" on a large scale not small... so how do we get around this.? its like looking at a field full of sheep and guessing which one came first. neutrinos collide with things at random points at random times......this to me is very important. |
| Mar27-12, 02:09 PM | #167 |
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And may I request that you make specific questions. Much of your posts seem to be ramblings that don't make any sense and don't seem to be asking anything. It would help both us and yourself if you could trim your posts down to clear, concise questions. |
| Mar27-12, 02:13 PM | #168 |
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| Mar27-12, 02:53 PM | #169 |
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i see. thank you. the light turns them into something else.....1+1 = 3 |
| Mar27-12, 04:49 PM | #170 |
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