What is the significance of systematic redshift and Mg II in astrophysics?

Click For Summary

Discussion Overview

The discussion centers around the significance of systematic redshift and the role of Mg II in astrophysics, particularly in the context of measuring variations in the fine-structure constant (alpha) using quasar absorption lines. Participants explore the definitions and implications of systematic redshift, the use of Mg II transitions as a baseline for measurements, and the interpretation of results from recent studies regarding alpha's variability.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants seek clarification on the meaning of systematic redshift and its distinction from other types of redshift.
  • It is proposed that Mg II transitions are used as a stable reference point for measuring redshift due to expansion, allowing for the isolation of changes in alpha.
  • Concerns are raised regarding the interpretation of results from studies that report no variation in alpha, questioning the meaning of "null result" and its implications for the hypothesis of alpha's variability.
  • Participants discuss the statistical interpretation of results, noting that a null result does not imply that alpha is equal to zero, but rather that there is insufficient evidence to support the hypothesis of variability.
  • There is a debate about the significance of the reported values and error margins in relation to the hypothesis being tested.

Areas of Agreement / Disagreement

Participants express varying interpretations of statistical results and the implications of null results, indicating that multiple competing views remain regarding the significance of findings related to alpha's variability.

Contextual Notes

Participants highlight the complexity of interpreting statistical results, including the role of error margins and the definitions of null results, which may depend on the specific hypotheses being tested.

Who May Find This Useful

This discussion may be of interest to those studying astrophysics, particularly in observational methods and the implications of fine-structure constant measurements, as well as those engaged in statistical analysis within scientific research.

shadishacker
Messages
28
Reaction score
0
Hi everyone,

I am new to observations and observational terms!
I am reading the paper "constraining the time variation of the fine-structure constant" by Srianand et. al
in the section "constraining alpha with QSO absorption lines" there is a sentence saying "... rest wavelengths of MG II ... thereby providing a good anchor for measuring the systematic redshift."

- What does the systematic redshift mean?
- What do they use Mg II for?
 
Space news on Phys.org
shadishacker said:
- What does the systematic redshift mean?
The redshift due to the expansion, as opposed to what they want to measure - i.e. changes in alpha.

shadishacker said:
- What do they use Mg II for?
You want to first identify transitions that would not vary much with changes to fine structure constant, and use these as the baseline for deducting the redshift due to expansion from your observables. The changes in transition energies that are left then can be interpreted as due to varying alpha.
 
Thanks a lot for the clear reply.
I'd like to ask two other questions:

- About this variation, in recent papers like " High-precision limit on variation in the fine-structure constant from a single quasar absorption system " by Kotus et. al mention that the measured variation for alpha is consistent with no variations.
But by the limits they say -1.4\pm 0.55 \pm 0.65 ppm, the term "no variation" is not fixed! I mean there are constraints on varying alpha, that 0 is one of them; but still it is not rejected.
As I right?

- In "CONSTRAINING THE VARIATION OF THE FINE-STRUCTURE CONSTANT WITH OBSERVATIONS OF NARROW QUASAR ABSORPTION LINES" by Songaila et. al, they used the sentence:
"We find a null result of ..."
what do they mean? They are reporting the probability of small variations in alpha, but they are using the term null result!
What does it mean?!
 
shadishacker said:
they are using the term null result!
What does it mean?!
It means that the result does not support the hypothesis. Here, the hypothesis is something like 'alpha varies with time'. If your experiment, designed to find this variation, nets you a range of possible values that includes 0 (no variation), and is not statistically leaning to one side (e.g. 0 is at the extreme end of the range), then your experiment has failed to find evidence of the proposed variation.
Alternatively, you can say that your experiment is consistent with the null hypothesis - here, the null hypothesis is that alpha does not vary in time.

This methodology is used in all science. It's simply a codified way of following the rule that 'you need extraordinary evidence for extraordinary claims'. A null result is a result of no consequence (which doesn't mean it was a waste of time!).

I believe this also answers your other question.
 
But how this "null result" given in this number? $\Delta \alpha/ \alpha = (-0.01\pm0.26) \times 10^{-5}$ which is for instance given in CONSTRAINING THE VARIATION OF THE FINE-STRUCTURE CONSTANT WITH OBSERVATIONS OF NARROW QUASAR ABSORPTION LINES" by Songaila et. al ?
I mean, how is 0 at the extreme end of the range?
 
shadishacker said:
But how this "null result" given in this number? $$\Delta \alpha/ \alpha = (-0.01\pm0.26) \times 10^{-5}$$ which is for instance given in CONSTRAINING THE VARIATION OF THE FINE-STRUCTURE CONSTANT WITH OBSERVATIONS OF NARROW QUASAR ABSORPTION LINES" by Songaila et. al ?
I mean, how is 0 at the extreme end of the range?
It isn't. That's the point. It's smack dab in the middle of the range. Hence you can't conclude that you've found evidence of variability. The result does not support it (= it's null).
 
Bandersnatch said:
It isn't. That's the point. It's smack dab in the middle of the range. Hence you can't conclude that you've found evidence of variability. The result does not support it (= it's null).

Am I missing something? Isn't the middle of the range -0.01?
 
Yeah, with error bars +/- 0.26.
 
Bandersnatch said:
Yeah, with error bars +/- 0.26.
So zero is not smack dab in the middle of the range, but it is -0.01. right?
do they conclude the variation is zero because of -0.01 is a small number near 0?
 
  • #10
They don't conclude the variation is 0! They conclude that they found no evidence that it isn't.

And of course -0.01 and 0 are not the same.

Perhaps there's a thread level mismatch. You've marked this thread as A = graduate level. Haven't you taken statistical methods? Done some lab work?

Look, if they found the result being e.g. -0.010 +/- 0.002, then they would have found evidence of variability. Same if it were e.g. 0.80 +/- 0.26. This is because both would exclude the possibility of there being no variation.
But the results they did get do not exclude 0, nor do they exclude anything between 0.25 and -0.27. The actual value can be anything in that range, with values around -0.01 being the most likely. Somebody would have to devise a better experiment to narrow the error bars even more, but as long as the new experiment results include 0, the results will be null.

An in case this is also causing confusion, 'null result' does not mean 'equal to zero'. It means 'of no consequence', or 'not sufficient to support the hypothesis'.
 
  • #11
Dear Bandersnatch,
Sorry if I marked the level wrong.

Anyway, thanks for the explanations.
I get the point now.
 

Similar threads

  • · Replies 124 ·
5
Replies
124
Views
24K
  • · Replies 8 ·
Replies
8
Views
4K
  • · Replies 7 ·
Replies
7
Views
3K
  • · Replies 8 ·
Replies
8
Views
4K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 1 ·
Replies
1
Views
4K
Replies
11
Views
10K
  • · Replies 96 ·
4
Replies
96
Views
12K
  • · Replies 1 ·
Replies
1
Views
3K