Path: csiph.com!aioe.org!.POSTED!not-for-mail From: The Starmaker Newsgroups: sci.physics.relativity Subject: Re: Inflation Date: Sun, 11 Mar 2018 23:15:21 -0700 Organization: Aioe.org NNTP Server Lines: 18 Message-ID: <5AA61AF9.22CB@ix.netcom.com> References: Reply-To: starmaker@ix.netcom.com NNTP-Posting-Host: X9ItFNC7Zcz4l6MobL/YRA.user.gioia.aioe.org Mime-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1 Content-Transfer-Encoding: 8bit X-Complaints-To: abuse@aioe.org X-Notice: Filtered by postfilter v. 0.8.3 X-Mailer: Mozilla 3.04Gold (WinNT; U) X-Antivirus: Avast (VPS 180311-2, 03/11/2018), Outbound message X-Antivirus-Status: Clean Xref: csiph.com sci.physics.relativity:452402 David (Kronos Prime) Fuller wrote: > > Duration > A key requirement is that inflation must continue long enough to produce the present observable universe from a single, small inflationary Hubble volume. > > This is necessary to ensure that the Universe appears flat, homogeneous and isotropic at the largest observable scales. > > This requirement is generally thought to be satisfied if the Universe expanded by a factor of at least 10^26 during inflation. > > 1 / (((1 kg * G) / (c^2)) * 1e+26) = > 13.4663531 > > Maybe it is just (Energy /“Pocket Volume”) > > Maybe it was just “Worm Holes that only allow passage of a >wavelength of energy at Planck Temp or above” connecting Distant >parts of the universe evenly distributing the Energy resulting in a >homogeneous isotopic CMBR distribution. Haven't you heard...Inflation is ad-hoc.