THE MALTA COSMOLOGY TEMPLATE



Chapter 06 - Photons






PARTS

Part 0600
Photons
Home


Part 0601
Cosmic

Photon
Creation

Part 0602
Photon

Mechanics

Part 0603
Cosmic

Microwave
Background

Photon
Selfproofs



















Photon Selfproofs

SELFPROOF 0608 - DOPPLER COLOURSHIFTING

CURRENT PARADIGM
  • The DOPPLER EFFECT is the change in frequency or wavelength of a wave (or other periodic event) for an observer moving relative to its source.      .....     The Doppler effect for electromagnetic waves such as light is of great use in astronomy and results in either a so-called redshift or blueshift. It has been used to measure the speed at which stars and galaxies are approaching or receding from us; that is, their radial velocities.      .....     The use of the Doppler effect for light in astronomy depends on our knowledge that the spectra of stars are not homogeneous. They exhibit absorption lines at well defined frequencies that are correlated with the energies required to excite electrons in various elements from one level to another. The Doppler effect is recognizable in the fact that the absorption lines are not always at the frequencies that are obtained from the spectrum of a stationary light source. Since blue light has a higher frequency than red light, the spectral lines of an approaching astronomical light source exhibit a blueshift and those of a receding astronomical light source exhibit a redshift. (Wikipedia - 15 July 2016)
MALTA TEMPLATE
COMMENTARY

The Doppler Effect is a distortion in what an observer sees or hears caused either by the movement of the observer, by the movement of what is being observed, or by the movement of both the observer and the observed at the same time (in practice, everything in the Universe is moving relative to everything else, to a greater or lesser degree).

So far as photons are concerned, the Doppler Effect alters their gravitational colourshifting away from what it would be if the emitting object and observer were both stationary. The cause is the altering of the amount of time spent within the gravitysheath interface of either the emitter or the observer by the movement. Consider these examples:

EXAMPLE A
  • The emitter and the observer are diverging.
  • The emitter and the observer have the same mass and are adjacent so their gravitysheaths abut and are the same size. 
  • Photons leave the emitter and go to the observer at lightspeed. 
  • Because the emitter and the observer are diverging, photons spend less time in the gravitysheath of the emitter being redshifted than they do in the gravitysheath of the observer being blueshifted
  • Thus the observer sees extra blueshift.
EXAMPLE B
  • The emitter and the observer are converging.
  • The emitter and the observer have the same mass and are adjacent so their gravitysheaths abut and are the same size.
  • Photons leave the emitter and go to the observer at lightspeed.
  • Because the emitter and the observer are converging, photons spend more time in the gravitysheath of the emitter being redshifted than they do in thegravitysheath of the observer being blueshifted.
  • Thus the observer sees extra redshift. 
At first glance, these results run contrary to the conventional wisdom which is that a receding object appears redshifted and that an approaching object appears blueshifted - but they don't. In the above examples, the emitter and the observer are both of the same mass. In real life, when making observations from the surface of the Earth, everything seen outside the Solar System is substantially more massive than is our planet and so gravitational colourshifting is the major factor in any such observation.

Having said that, the colourshifting of a photon away from the wavelength at which it first stabilised is a multiprocess. In assessing the reasons for the colourshift in an observed photon the following factors, at the very least, need to be considered:
  • The mass of the emitting object.
  • The mass of the observing object.
  • The direction and speed of the emitting object.
  • The direction and speed of the observing object. 
  • The position within the Universe sphere from where the photon was emitted.
  • The moment in the life of the Universe when the photon was emitted.
  • The position within the Universe sphere where the photon is observed.
  • The moment in the life of the Universe when the photon is observed. 
  • The timescale of the expansion of the Universe, bearing in mind that the rate of that expansion is not a constant.
  • The disposition of the mass of the Universe, bearing in mind that the disposition of that mass has varied over its lifetime. 
  • The track of the photon from its emission to its observation and thus the gravitypulls it has experienced and the gravitonstreams through which it has passed.






Comments and suggestions:  peter.ed.winchester@gmail.com

Copyright 2013 Peter (Ed) Winchester



REVISIONS

19 Jul 2014 - page revised to 3-section format.
16 Jul 2016 - revisions to layout and content.

23 Apr 2017 - changed teels to gravitons.