Time dilation, magnitude, and redshift of Type Ia SNe #235
Replies: 6 comments 63 replies
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I don't see how you are getting that the brighter ones are at higher redshift. The figures are from a short popular article by Perlmutter in 2003. I have attached it for convenience. The purpose of the figures is to show how they can weed out "outliers" (the brighter and dimmer ones) to get a true set of standard candles. There is no mention of different redshifts for these SN. |
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Here's a python notebook that downloads the Pantheon+SH0ES data and takes distance modulus, magnitudes, and z: https://github.com/mikehelland/hubbles-law/blob/master/other/python/snmags.ipynb Here's mB and m_b_corr: mB - SALT2 uncorrected brightness https://github.com/PantheonPlusSH0ES/DataRelease/tree/main/Pantheon%2B_Data/4_DISTANCES_AND_COVAR If you subtract the distance modulus from the (apparent) magnitudes, you should get absolute magnitude: So from this you can see they just set each SN to -19.25 for absolute magnitude. |
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Posting this here for completeness: https://www.youtube.com/watch?v=1vfo-JFc-Io DES Supernovae - Precisely Measured Time Dilation from Universe's Expansion (White & Davis) |
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Time dilation isn't a feature of high redshift. Redshifted light is time
dilated light.
Take light, time dilate it. Its frequency goes down. Walla.
…On Thu, Jun 27, 2024, 9:26 AM Matt Edwards ***@***.***> wrote:
@mikehelland <https://github.com/mikehelland>
But it seems Crawford is in a similar boat to this Jensen fellow, intent
on making the time dilation go away in order to keep tired light viable.
I noticed that Gupta did a study comparing numerous models on how they
predict the SN light curves: https://doi.org/10.3390/universe5050102
<http://url>
He mentions TL models and also Crawford's model, which he considered TL
also. He writes:
Generally accepted flux loss phenomena are as follows [14]: (a) Increase
in the wavelength causes the flux loss proportional to 1/(1 + z), and (b)
In an expanding universe, an increase in detection time between two
consecutive photons emitted from a source leads to a reduction of flux,
also proportional to 1/(1 + z). Therefore, in an expanding universe the
necessary flux correction required is proportional to 1/(1 + z)2, whereas
in a non-expanding universe the correction required is proportional only to
1/(1 + z).
He ends up concluding that the LCDM model is the second best fit, an
Einstein-deSitter model being the best. He does not mention SALT.
What I am confused about is why Crawford and @LifeIsStrange
<https://github.com/LifeIsStrange> are so intent on removing the extra (1
+ z) time dilation component, when that term is needed to make a good fit.
On the other hand, I have read numerous times that TL models *do* explain
the SN light curves adequately. Can you or anyone here shed light on this?
Earlier you advanced a hypothesis where time dilation is just a feature of
high redshift. I think this could fit with my shell model, since the Hubble
redshift then becomes a gravitational redshift due to the shell. (It's more
complicated than this, as new expressions of GR are necessary). The crazy
other part is that we naturally tend to think of the gravitational redshift
as not being a TL redshift. In my model, it can be. It goes back to the
question of whether energy is lost by a photon in the gravitational
redshift. Everyone in ACG except for me thought that it is not lost. I
think that it is lost, and this lost energy is what gives rise to gravity.
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@HanDeBruijn the analysis done by @mikehelland in thread 225 seems to use the results from the papers from Pantheon+SH0ES, in which the luminosity distance would have been calculated from observations using LCDM. (Is that correct Mike?) If you want a good value for Since the units [km/s] imply a recession velocity due to space expansion, it would be better to divide by If you don't have enough graduate student (i.e. slaves) working for you, a less accurate method (but much easier) would be to convert "LCDM luminosity distances" to redshift with the cosmological parmeters It's possible that neither 70.5 nor 73.4 is correct, but my "intuitive guess" is that |
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Let's recapitulate from thread 216 with this picture. Again and again, Hubble tensions are observed. Now suppose that people are all wrong and that (my version of) the Variable Mass Theory (VMT) is right (-: just an ambitious assumption). Then, with a piece of that theory, the Hubble parameter is linked to age on one hand and to a characteristic time for Exponential growth on the other hand. Let This would mean that the value the Hubble parameter depends on the "age" of the phenomenon that people are observing. An extreme example is the Hubble parameter that can be attached to the age of the Earth (in orbital time of course). Calculation:
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Follow-up to this question by @ExpEarth:
Based on another conversation with @LifeIsStrange, I pointed to this:
https://physics.stackexchange.com/questions/300365/time-dilation-of-distant-cosmic-events-what-is-it
Which contains this image:
Here the broader light curves are more time dilated, but also appear to have brighter magnitudes with redshift. For a standard candle, that's peculiar.
Am I reading that wrong? It looks like magnitudes are brighter with redshift. Similar to quasar magnitudes discussed in #210 .
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