Garth
Science Advisor
Gold Member
- 3,580
- 107
The point you are missing sd01g is the difference between an object's speed within space-time and the cosmological velocity of recession due to the expansion of space itself, which carries an embedded object along with it, within space-time.
The caveat is, though, that we have to define what we actually mean by that cosmological recession; i.e. how do we measure it?
Ans. The measurement we are talking about is that of cosmological (Hubble) red shift, but that itself then has to be interpreted according to a convention of definition of length and time over cosmological distances.
If particle (rest) masses are constant then rulers are 'fixed' and clocks are 'regular' and cosmological red shift is interpreted as a Doppler effect of velocity of recession. But if particle rest masses are not constant then the red shift is open to other interpretation as in Fred Hoyle's paper "On the Origin of the microwave background" Ap.J. 196 pg661-670 1975.
If this seems maverick in the extreme then note this comment about Fred Hoyle, one of my heroes:
The caveat is, though, that we have to define what we actually mean by that cosmological recession; i.e. how do we measure it?
Ans. The measurement we are talking about is that of cosmological (Hubble) red shift, but that itself then has to be interpreted according to a convention of definition of length and time over cosmological distances.
If particle (rest) masses are constant then rulers are 'fixed' and clocks are 'regular' and cosmological red shift is interpreted as a Doppler effect of velocity of recession. But if particle rest masses are not constant then the red shift is open to other interpretation as in Fred Hoyle's paper "On the Origin of the microwave background" Ap.J. 196 pg661-670 1975.
If this seems maverick in the extreme then note this comment about Fred Hoyle, one of my heroes:
From the Prologue of Simon Mitton's book “Fred Hoyle - A life in science.”What is extraordinary about Fred Hoyle's science is that his impact derives equally from instances when he was right and others when he was wrong! Generally within academia, an erroneous paper is quietly forgotten: it receives the silent treatment. Hoyle's contribution to the advancement of science derived much of its impetus from the way in which his colleagues recoiled at his notions. His opponents deployed enormous resources to wrong-foot him. In the twentieth century, no other figure in astronomy had to withstand for such a long period the criticisms of both the invisible college of astronomers worldwide and the parochial college of Cambridge practitioners. Hoyle’s scientific life was truly unparalleled, and unforgettable.
Last edited: