4 • 993 Ratings
🗓️ 16 August 2023
⏱️ 23 minutes
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0:00.0 | ID the future, |
0:05.0 | future, a podcast about evolution and intelligent design. |
0:10.0 | Welcome to ID the future. I am your host Brian Miller. This is part two of my |
0:17.4 | interview with Rabbi Aaron and Zimmer and Rabbi Ellie Feder about their |
0:21.8 | podcast Physics to God which can be found at Physics to God.com. |
0:27.0 | Do either of you have a favorite example of fine tuning that you like to quote? Is there particularly one that you find really makes this point very clear? |
0:36.7 | You know, the one that really impacted the scientific world was the cosmological constant. |
0:41.8 | It was in 1998 when scientists met the the |
0:43.2 | cosmological constant. It was in 1998 when scientists met the distant supernovae and they realized |
0:46.7 | that the universe is in fact not only expanding but it's actually accelerating. |
0:50.6 | And this was really due to a constant in general relativity called the cosmological constant. And it turns out that this constant has to be fine tuned to about 120 decimal places. |
1:02.5 | And if had it been different by a couple |
1:04.8 | decimal places less or more, the universe |
1:07.3 | would have contracted right away after the Big Bang. |
1:10.0 | You never have galaxies developed, |
1:12.0 | or would have expanded way too quickly. Again, you would never have galaxies developed or would have expanded way too quickly. |
1:13.7 | Again you never have galaxies developed or or anything else for that matter. |
1:18.3 | So until this point there was a lot of other constants that were kind of fine-tuned. |
1:23.0 | And as scientists gained more and more knowledge about the constants, |
1:26.0 | they started to realize they're more and more fine-tuned. |
1:28.0 | But it wasn't until 1998 where the cosmological constant was measured, |
1:32.0 | and they realized that this was |
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