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Chapter 16
A Steady-State Universe
a Steady-State Universe
After the "Big Bang"
"While an actual physical expanding universe is, indeed, the popular view, it is not the accepted scientific view." Britannica CD, 1997
Gamow-Hoyle debate
Gamow's Big Bang
Lemaître-Gamow Expanding universe
Arthur Wellesley the 1st, Duke of Wellington
that great battle with Napoleon at Waterloo
Tensors
The universe is homogeneous and isotropic.
This universe would be finite yet have no borders or edges.
Einstein did hesitate in using this 1917 "cosmological constant.
The de Broglie wavelength of an electron can vary with acceleration.
Talking about the de Broglie wavelength now. It is blue shifted with acceleration.
blitzseit
the de Broglie wavelength gets shorter with an increase of either mass or acceleration
The de Broglie wavelength only gets shorter with mass and/or acceleration in the microcosm.
giant Virgo super-cluster
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These links, on left hand side of page, will cover what you will be reading in Chapter 16.
Links that are actually in the book will be in bold print.
Click Links below for each paragraph you are reading in
"Universities Asleep at the Switch".
Chapter 1 links
Chapter 2 links
Chapter 3 links
Chapter 4 links
Chapter 5 links
Chapter 6 links
Chapter 7 links
Chapter 8 links
Chapter 9 links
Chapter 10 links
Chapter 11 links
Chapter 12 links
Chapter 13 links
Chapter 14 links
Chapter 15 links
Chapter 17 links
Chapter 18 links
Chapter 19 links
Chapter 20 links
Chapter 21 links
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