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No dark matter wasn't enough in some scientists minds, that's why dark energy was added to the mix, whether dark energy exists is still a matter of scholarly debate.
The expansion rate of the universe is 71+/-3.5 km/sec/Mpc, this number is subject to quite a bit of uncertainty.
On large scales scientists believe the universe homogeneous, on our scale is certainly is not. Large scale homogeneity implies uniform expansion.
Here are links to a couple of segments for the excellent CBC radio science show Quirks and Quarks where dark matter and energy is discussed
"The inconsistency between his results and those of other astronomers has yet to be resolved. For the moment, most astronomers think there are more strengths to the theory of dark energy than there are weaknesses, but many are still uncomfortable with the idea that we know nothing about the most influential and powerful force in the universe. "
http://www.cbc.ca/quirks/media/2003-2004/mp3/qq-2004-01-31a.mp3
"Einstein's Telescope
Dr. Evalyn Gates has set herself a challenge. She wants to explain how she and her colleagues are going to learn about invisible energy by looking at invisible matter with an invisible telescope. In her new book, Einstein's Telescope: The Hunt for Dark Matter and Dark Energy in the Universe."
http://www.cbc.ca/quirks/media/2008-2009/mp3/qq-2009-03-14_01.mp3
Source(s):
http://www.astro.ucla.edu/~wright/cosmo_01.htm#CO
http://www.cbc.ca/quirks/archives/03-04/jan31.html
http://www.cbc.ca/quirks/archives/08-09/qq-2009-03-14.html
http://en.wikipedia.org/wiki/Cosmological_principle
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davepamn
The math is here if you can wrap your head around it. (Mine exploded)
http://en.wikipedia.org/wiki/Equation_of_State_(Cosmology)
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Answered Question
M$1
May 31, 2009 04:25 PM
Does Dark Matter adequately explain why the Universe is expanding at an accelerate rate?
How fast is the Universe accelerating?
Is the Universe homogenous and expanding uniformly?
Is the Universe homogenous and expanding uniformly?
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Best Answer Chosen by Asker
| May 31, 2009 09:29 PM |
The expansion rate of the universe is 71+/-3.5 km/sec/Mpc, this number is subject to quite a bit of uncertainty.
On large scales scientists believe the universe homogeneous, on our scale is certainly is not. Large scale homogeneity implies uniform expansion.
Here are links to a couple of segments for the excellent CBC radio science show Quirks and Quarks where dark matter and energy is discussed
"The inconsistency between his results and those of other astronomers has yet to be resolved. For the moment, most astronomers think there are more strengths to the theory of dark energy than there are weaknesses, but many are still uncomfortable with the idea that we know nothing about the most influential and powerful force in the universe. "
http://www.cbc.ca/quirks/media/2003-2004/mp3/qq-2004-01-31a.mp3
"Einstein's Telescope
Dr. Evalyn Gates has set herself a challenge. She wants to explain how she and her colleagues are going to learn about invisible energy by looking at invisible matter with an invisible telescope. In her new book, Einstein's Telescope: The Hunt for Dark Matter and Dark Energy in the Universe."
http://www.cbc.ca/quirks/media/2008-2009/mp3/qq-2009-03-14_01.mp3
Source(s):
http://www.astro.ucla.edu/~wright/cosmo_01.htm#CO
http://www.cbc.ca/quirks/archives/03-04/jan31.html
http://www.cbc.ca/quirks/archives/08-09/qq-2009-03-14.html
http://en.wikipedia.org/wiki/Cosmological_principle
| Asker's Rating: |
• Thanks, I listened to the Dark Energy lecture and found it interesting.
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davepamn
June 01, 2009 03:00 PM
I ordered Dr Gates book: "Einstein's telescope : the hunt for dark matter and dark energy in the universe"
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Other Answers (1)
May 31, 2009 05:38 PM
As the Universe expands, the density of dark matter declines more quickly than the density of dark energy and, eventually, the dark energy dominates. Specifically, when the volume of the universe doubles, the density of dark matter is halved but the density of dark energy is nearly unchanged (it is exactly constant for a cosmological constant). The math is here if you can wrap your head around it. (Mine exploded)
http://en.wikipedia.org/wiki/Equation_of_State_(Cosmology)
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