tag:blogger.com,1999:blog-416737812331434120.post8373586533056624309..comments2023-03-30T00:55:03.648-07:00Comments on theory: New numerology for dark energyUnknownnoreply@blogger.comBlogger8125tag:blogger.com,1999:blog-416737812331434120.post-80320578263560419842016-05-07T06:26:28.749-07:002016-05-07T06:26:28.749-07:00This was independently discovered by a Physics Sta...This was independently discovered by a Physics Stack Exchange user, <a href="http://physics.stackexchange.com/users/113705/bonkers" rel="nofollow">"bonkers"</a>, around 8 April 2016, but the post has been deleted. Mitchellhttps://www.blogger.com/profile/10768655514143252049noreply@blogger.comtag:blogger.com,1999:blog-416737812331434120.post-33607781072997781912013-08-31T05:50:41.256-07:002013-08-31T05:50:41.256-07:00You might appreciate the fact that this new dark-e...You might appreciate the fact that this new dark-energy fraction is approximated not only by 1-1/π, but also by ln 2 (the latter was noticed by A. Garces Doz). So ln 2 + 1/π is approximately 1, and these quantities also approximately correspond to "dark energy' and "everything else". <br /><br />Mitchellhttps://www.blogger.com/profile/10768655514143252049noreply@blogger.comtag:blogger.com,1999:blog-416737812331434120.post-76076747058283691062013-04-20T23:36:24.628-07:002013-04-20T23:36:24.628-07:00Another approach would be to focus on the 9:3:1 ra...Another approach would be to focus on the 9:3:1 ratio. Which is rather approximate, but then the estimated density fractions themselves are somewhat model-dependent. <br /><br />I can imagine a relatively mainstream model producing a ratio of the form x^2:x:1... Mitchellhttps://www.blogger.com/profile/10768655514143252049noreply@blogger.comtag:blogger.com,1999:blog-416737812331434120.post-37638285739745661962013-04-20T21:26:42.853-07:002013-04-20T21:26:42.853-07:00Although if Wetterich's shrinking universe is ...Although if <a href="http://arxiv.org/abs/1303.6878" rel="nofollow">Wetterich's shrinking universe</a> is possible (<a href="http://online.kitp.ucsb.edu/online/primocosmo13/wetterich/" rel="nofollow">talk</a>), <a href="http://vixra.org/abs/1304.0003" rel="nofollow">anything is possible</a>. Mitchellhttps://www.blogger.com/profile/10768655514143252049noreply@blogger.comtag:blogger.com,1999:blog-416737812331434120.post-18003849355796923172013-04-18T07:24:09.765-07:002013-04-18T07:24:09.765-07:00I see that I failed to record my own favorite Plan...I see that I failed to record my own favorite Planck-inspired (and Sheppeard-inspired) numerology, which is that that the density fractions for dark energy, dark matter, and baryonic matter, are approximately 2/3, 2/9, 2/27 (which are the Koide phases of s-c-b, e-mu-tau, and u-c-t respectively). <br /><br />But probably no version of these ideas makes sense, in anything like standard cosmology, because there, the density fractions evolve drastically with time. Mitchellhttps://www.blogger.com/profile/10768655514143252049noreply@blogger.comtag:blogger.com,1999:blog-416737812331434120.post-34649198408813880792013-04-02T07:23:24.908-07:002013-04-02T07:23:24.908-07:00The next thing I know, the answer to life, the uni...The next thing I know, the answer to life, the universe and everything will be not 42, but <a href="http://mathworld.wolfram.com/JennysConstant.html" rel="nofollow">Jenny's Constant.</a>andrewhttps://www.blogger.com/profile/08172964121659914379noreply@blogger.comtag:blogger.com,1999:blog-416737812331434120.post-82286919459195467262013-03-23T21:57:20.692-07:002013-03-23T21:57:20.692-07:00Interesting, and answers a question I recently ask...Interesting, and answers a question I recently asked of the new hmap data. I have always regarded the inverse of pi which I called inertial pi as a significant space value.<br /><br />L. Edgar Otto I wonder how Ms Riofrio will comment on this.L. Edgar Ottohttps://www.blogger.com/profile/00525169618204198073noreply@blogger.comtag:blogger.com,1999:blog-416737812331434120.post-89867016356268270282013-03-23T19:26:32.608-07:002013-03-23T19:26:32.608-07:00Incidentally, Louise Riofrio's value for the b...Incidentally, Louise Riofrio's value for the baryonic matter density fraction is 1 - 3/π, which would leave dark matter as 4/π - 1...Mitchellhttps://www.blogger.com/profile/10768655514143252049noreply@blogger.com