Gravitational Redshift Contribution to Quasar Redshift: Explaining Hubbles Law

In summary: The redshift due to the gravitational redshift is so small, it's essentially indistinguishable from the broadening due to emission from material closer to the black hole.- Quasar spectra show that there is a significant contribution from gravitational redshift. - This gravitational redshift is smaller than the wavelength resolution of any spectroscope that has been used to obtain quasar spectra. - The gravitational redshift is effectively zero; it's certainly smaller than the wavelength resolution of any spectroscope that is currently available. - The EM we see comes from regions far enough from the SMBH at the heart of a quasar that redshift due to its depth in the SM
  • #1
talksabcd
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Does anyone know how much percentage of the total redshift of a quasar is contributed by Gravitational redshift considering light from the Quasar is emitted by heavy active galactic nuclei ?

If there is a significant contribution from gravitational redshift then how will the Hubbles law hold true for calculating distance of a Quasar based on redshift ? Are we removing Gravitational redshift contribution before calculating its distance ?

Pls explain.
 
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  • #2
In the spectra of quasars - no matter what waveband - the gravitational redshift component is effectively zero; it's certainly smaller than the wavelength resolution of any spectroscope that I know of that's been used to obtain quasar spectra.

It's pretty easy to see why this is so: the EM we see comes from regions far enough from the SMBH at the heart of a quasar that redshift due to its depth in the SMBH's gravitational well is negligible ... if it didn't (come from such regions), then at least the line profiles would be quite different than what we actually observe.

AFAIK (as far as I know), the only gravitational redshifts, due to SMBH, that have been observed are some x-ray line profiles, and those are from normal, nearby galaxies (gravitational redshift due to SgrA* may also have been observed).
 
  • #3
As Nereid noted, radiation emitted near enough to a black hole to be noticeably gravitationally redshifted would be swamped by radiation emitted by infalling particles too distant from the black hole to be gravitationally redshifted. Visualize the black hole as an intensely hot speck of matter surrounded by a diffuse cloud of matter. Most of the matter would 'burn up' far from the hot spark at the center. Near the center, mostly ashes would remain with very little mass left to convert to energy. It would be carried off in the form of extremely energetic photons, meaning far fewer photons are needed to carry off the same amount of mass as reactions occurring at distances where gravitational redshift is negligible. A candle flame is a fair analogy. The center of the flame is hotter, yet far dimmer than the plasma envelope.
 
  • #4
Thanks for explaining. If the entire redshift is attributed to its distance then why time dilation has not been observed similar to 1a supernova ? Is there something fundamental with Qusars that we didnt understand ?
 
  • #5
talksabcd said:
Thanks for explaining. If the entire redshift is attributed to its distance then why time dilation has not been observed similar to 1a supernova ? Is there something fundamental with Qusars that we didnt understand ?
How would you know you were observing time dilation in the light curve of a quasar? Or even in the light curves of a million quasars?

Perhaps one way to answer this is by comparing quasars with Type1a SNe; how do we observe time dilation in such?

By comparing an observed characteristic time with the 'rest frame' equivalent. What 'characteristic time'? Let's call it the decay of a radioisotope of iron* - we know it's x days, here on Earth; we observe it to be y days, in a particular Type 1a SNe ... we attribute the difference to time dilation.

Is there something similar in quasars? Unfortunately, AFAIK, no.

For a start, quasars are, to all intents and purposes, point sources. However, their spectra tell us that the light (EM in general) comes from at least four different physical regimes - an accretion disk, jets, a broad line region, a narrow line region, and (for some wavebands) a dusty torus. On top of that, we expect at least a component of the variability of quasars to be due to microlensing, of the accretion disk (say) by stars in the galaxy surrounding that disk. How to tease apart an apparent magnitude vs time curve into intrinsic variability of any particular component?

It gets worse.

We also know that quasars evolve - not only were there more of them a few billion years ago, but their physical characteristics seem to have changed, over (cosmological) time. How to attribute any observed variability to the parts that are due to the particular evolutionary stage a quasar is at vs that due to time dilation?

(There's more, but that will do for now).

*it doesn't matter what it actually is, for the purposes of my explanation here, just so long as we have a high degree of confidence that there is an unambiguous characteristic time signature in the light curve.
 
  • #6
We can actually see evidence of gravitational redshift in QSO's. As pointed out above, the vast majority of the redshift is cosmological, however the gravitational redshifted in imprinted onto the shape of some of the emission lines of QSO's. There are lines that broadened, due to some material emitting radiation very close to the Black Hole having a greater gravitational shift than material further out.

This broadening is in addition to other broadening such as thermal effects, but theoretical models can piece the two apart, plus the broadening is not symmetric so has a tell tale shape.

So the position of various emission lines in a QSO in determine almost entirely by the cosmological redshift but we can see the evidence of gravitational redshift in the shape of some of those lines.
 
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  • #8
Errm doesn't your link show some nice spectra doing just that?

The confusion may lie in my sloppy use of terminology. I've never really grasped the difference between QSO's, Quasars and AGNs and use the terms interchangeably, though I'm sure this is not correct. Is this effect only seen in AGNs but not the others? By my understanding of these things I can't see why it would be only the AGNs but as I say, I've never understood the rationale for the difference boxes we like to put these things into.
 
  • #9
Wallace said:
Errm doesn't your link show some nice spectra doing just that?

The confusion may lie in my sloppy use of terminology. I've never really grasped the difference between QSO's, Quasars and AGNs and use the terms interchangeably, though I'm sure this is not correct. Is this effect only seen in AGNs but not the others? By my understanding of these things I can't see why it would be only the AGNs but as I say, I've never understood the rationale for the difference boxes we like to put these things into.
You're right - if you consider Seyferts and quasars (and ...) as AGNs, then case closed.

However, historically, and still to some extent observationally, quasars and Seyferts are quite distinct classes of objects (and even today, SDSS, for example, makes a clear distinction between type 2 quasars - where the torus hides the accretion disk - and 'normal' quasars).

I suspect that the term 'quasars' is still quite widely understood to have its historical meaning of 'quasi-stellar object' (i.e. no resolved galaxy that it sits at/as the nucleus of). I took it that the 'quasar' talksabcd meant, in the OP, was this historical meaning.
 
  • #10
Nereid said:
I suspect that the term 'quasars' is still quite widely understood to have its historical meaning of 'quasi-stellar object' (i.e. no resolved galaxy that it sits at/as the nucleus of). I took it that the 'quasar' talksabcd meant, in the OP, was this historical meaning.

As an 'old hand' I always understood
QSO to mean 'Quasi-Stellar Object' and
Quasar to mean 'Quasi-Stellar Radio Object'.

When they were first discovered in the 1960's the QSO's were recognised as being point like objects with large red shift and Quasar's as being the same but with radio lobes. Often with a quasar it was the radio emission that was the first to be observed and noticed.

AGN's were observed as extended galactic objects that had high emissions in other parts of the spectrum from their nucleii.

Of course both quasars and QSOs are now known to be embedded in galaxies, but that came later.

Garth
 
  • #11
Garth said:
As an 'old hand' I always understood
QSO to mean 'Quasi-Stellar Object' and
Quasar to mean 'Quasi-Stellar Radio Object'.

When they were first discovered in the 1960's the QSO's were recognised as being point like objects with large red shift and Quasar's as being the same but with radio lobes. Often with a quasar it was the radio emission that was the first to be observed and noticed.

AGN's were observed as extended galactic objects that had high emissions in other parts of the spectrum from their nucleii.

Of course both quasars and QSOs are now known to be embedded in galaxies, but that came later.

Garth
Given the importance of SDSS to studies of quasars, it may be of interest to quote what http://www.sdss.org/dr5/products/general/target_quality.html#qso" ("The 2dF QSO Redshift Survey"):
The 2QZ is flux limited in the bJ band. Magnitudes were determined from APM scans of UKST photgraphic plates. The survey limits are 18.25<bJ<20.85, with the brighter 6dF QSO Redshift Survey (6QZ) being limited to 16.0<bJ<18.25, and observed with 6dF on the UKST. Colour selection was made in the u-bJ vs. bJ-r plane. In the plot below, QSO candidates are all those points below or left of the dotted line. Large blue points are previously known QSOs.
So, somewhere between the 2QZ and SDSS DR5, "QSOs" became "quasars"!
 
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1. What is the Gravitational Redshift Contribution to Quasar Redshift?

The Gravitational Redshift Contribution to Quasar Redshift refers to the phenomenon where the light emitted from a quasar (a type of active galactic nucleus) is redshifted due to the gravitational pull of the massive black hole at its center. This results in a shift towards longer wavelengths in the light spectrum, indicating that the quasar is moving away from us.

2. How does this contribute to Hubble's Law?

Hubble's Law states that the farther a galaxy is from us, the faster it appears to be moving away. The Gravitational Redshift Contribution to Quasar Redshift is one of the factors that contributes to this apparent motion, as it causes the light from distant quasars to be redshifted and appear to be moving away from us at high speeds.

3. What evidence supports this theory?

There is strong evidence for the Gravitational Redshift Contribution to Quasar Redshift, including observations of the redshifted light from quasars and mathematical models that predict the expected amount of redshift based on the mass of the black hole at the center of the quasar. Additionally, the overall trend of faster apparent motion with increasing distance, as predicted by Hubble's Law, is consistent with the contribution of gravitational redshift.

4. Are there any alternative explanations for Hubble's Law?

While the Gravitational Redshift Contribution to Quasar Redshift is one factor that contributes to Hubble's Law, there are other possible explanations such as the expansion of the universe and the effects of dark energy. However, these alternative explanations do not fully account for the observed redshifts of quasars and galaxies at extreme distances, making the Gravitational Redshift Contribution a crucial factor in understanding Hubble's Law.

5. How does this relate to our understanding of black holes?

The Gravitational Redshift Contribution to Quasar Redshift is a direct result of the intense gravitational pull of the black hole at the center of a quasar. This phenomenon provides valuable insights into the characteristics and behavior of black holes, which are still not fully understood by scientists. By studying the redshift of quasars, we can learn more about the properties and effects of these mysterious objects.

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