|
|
Thread Tools | Display Modes |
#21
|
|||
|
|||
Doppler Tests on Local Stars
On Mar 1, 12:43 pm, Oh No wrote:
Thus spake Kent Paul Dolan "Oh No" wrote restricting to stars ... within 100pc of the Sun By doing so you've selected this tiny ball of stars (compared to the size of the galaxy) all in essentially the same part of the galaxy, all going essentially in the same direction around the center of the galaxy. I am looking at the essentially random differences in orbit, due largely to differences in eccentricity and the alignments of the axes. It seems to me, then, that essentially _all_ you are seeing is proper motion of those stars with respect to the sun, I am not sure if you know what proper motion is. It is the visible movement of a star over time, measured in milliarcsecs per year. I am converting that, together with radial velocity measurements into velocities in km/s relative to the Sun. Now there is no a priore reason why, on any axis we look out into space, there should be a stronger alignment of velocities along that axis than there is perpendicular to it, both for stars approaching and for stars going away, but that is what must be happening if the standard model is right. I've been studying, http://arxiv.org/abs/gr-qc/0604047 and focused on the "Alf & Beth" diagrams therein, very clear, and see the cosmological expansion factor in Eq.(2.5), that is the basis of "teleconnection". ((correct me if I'm wrong)). You further stipulate Alf & Beth are in communication, via photons. Let's suppose Alf & Beth are at relative rest, defined as the Number of wavelengths in that communication is constant. That's basically how the interferometry of the LIGO apparatus works, so let's permit a hypothetical "arm" of an interferometer to span from Alf to Beth. For some rigority, that Number of wavelengths or cycles can be defined by a "proper time" invariant like S^2 = g_uv x^u x^v, with S being that Number. So here's what I understand, while N remains constant, the frequency of that light used to communicate between Alf & Beth will reduce, and thus the wavelength increases, due to the hypothetical cosmological expansion. Is that ok with you? Regards Ken S. Tucker |
#22
|
|||
|
|||
Doppler Tests on Local Stars
Thus spake Ken S. Tucker
I've been studying, http://arxiv.org/abs/gr-qc/0604047 and focused on the "Alf & Beth" diagrams therein, very clear, and see the cosmological expansion factor in Eq.(2.5), that is the basis of "teleconnection". ((correct me if I'm wrong)). You further stipulate Alf & Beth are in communication, via photons. Let's suppose Alf & Beth are at relative rest, defined as the Number of wavelengths in that communication is constant. That's basically how the interferometry of the LIGO apparatus works, so let's permit a hypothetical "arm" of an interferometer to span from Alf to Beth. For some rigority, that Number of wavelengths or cycles can be defined by a "proper time" invariant like S^2 = g_uv x^u x^v, with S being that Number. So here's what I understand, while N remains constant, the frequency of that light used to communicate between Alf & Beth will reduce, and thus the wavelength increases, due to the hypothetical cosmological expansion. More or less, but to clarify, this was a one way communication from Alf to Beth across cosmological distances. The cosmological expansion is not hypothetical. It is a standard prediction of general relativity and red shift is measured in practice. The thing I find is a different amount of red shift than standard general relativity. Regards -- Charles Francis moderator sci.physics.foundations. substitute charles for NotI to email |
#23
|
|||
|
|||
Doppler Tests on Local Stars
Thus spake Steve Willner
Oh No wrote: They use VLBI to determine the motion. Actually, they use VLBI to determine the position on the sky. The change in position over several years determines the motion. they are counting interference fringes, and it is still a quantum effect. You mean in the teleconnection model? In standard theory, radio interferometry is all classical: good old Maxwell's equations. Indeed, that is the standard theory. Quantum theory has a way of being much more inexplicable and bizarre. My expectation is that whatever the overstatement in velocity we get from Doppler measurement of globular clusters, we will get the same overstatement from any other method which depends on quantum wave effects. Quasar positions measured by VLBI agree with those measured by classical astrometry. Yes, but in quantum theory when you do a classical measurement the wave function collapses. There is a discontinuity in the description of motion at the time of measurement. I am also expecting a discontinuity in VLBI measurements when carried out over a sufficient time that classical astronometry becomes possible. Whether the apparent discontinuity in motion of IM Pegasi is an instance of that, I would not like to say. Regards -- Charles Francis moderator sci.physics.foundations. substitute charles for NotI to email |
#24
|
|||
|
|||
Doppler Tests on Local Stars
Thus spake Steve Willner
Oh No wrote: They use VLBI to determine the motion. Actually, they use VLBI to determine the position on the sky. The change in position over several years determines the motion. they are counting interference fringes, and it is still a quantum effect. You mean in the teleconnection model? In standard theory, radio interferometry is all classical: good old Maxwell's equations. My expectation is that whatever the overstatement in velocity we get from Doppler measurement of globular clusters, we will get the same overstatement from any other method which depends on quantum wave effects. Quasar positions measured by VLBI agree with those measured by classical astrometry. It is probable others understand a lot more about VLBI than I do. When the position of SgrA* is measured do they have to take into account gravitational red shift of light emanating from the centre of the galaxy? Of course this would not affect distant quasars. In the standard model the contained mass in a given radius, r, including CDM, should be roughly given by v^2/r = GM/r^2 For a rotation speed of ~235km/s at 8kpc, as determined by Reid and Brunthaler, I think that gives a contained mass of a little over 100Bill Suns. What would the effect on the VLBI calculation of orbital motion be if there were only 55 Bill solar masses within that radius? Regards -- Charles Francis moderator sci.physics.foundations. substitute charles for NotI to email |
#25
|
|||
|
|||
Doppler Tests on Local Stars
Thus spake Martin Hardcastle
In article , Oh No wrote: A prediction of the teleconnection is that the reason for the flattening of galaxy rotation curves is that radial velocity measured using Doppler requires a correction due to cosmological expansion. If this is true then the orbital velocity of the sun about the Milky Way is ~160km/s, not ~220km/s as is usually stated You need to worry about how these results are consistent with the observed parallactic motion of the galactic centre -- see e.g. Reid & Brunthaler 2004 ApJ 616 872. Martin I think it worth remarking that Reid and Brunthaller get a figure for proper motion of SgrA* of 6.379+-0.024 mas/yr. That corresponds to an orbital velocity of the Sun of 241+-1km/s at a radius of 8kpc. Even allowing for the uncertainty of +-0.5kpc in the distance to SgrA*, it is a little high compared to other measurements of Solar velocity, usually about 220km/s, and noticeably high compared to the determination of the galactic rotation rate at the solar circle of Loktin and Beshenov from open clusters (Astronomy Reports, 2003, 47, 1, pp6-10), which comes to 197+-6.4km/s at 8kpc. There are other small inconsistencies in astronomical measurements within the Milky Way. The Hipparcos parallax distance of the Plaeides springs to mind. Possibly that is to be expected at the current state of the art, but I would love to be able to carry out a few of these calculations to find out whether the teleconnection gives greater consistency. Unfortunately for most of them it helps to be a trained astronomer, which I am not. Regards -- Charles Francis moderator sci.physics.foundations. substitute charles for NotI to email |
#26
|
|||
|
|||
Doppler Tests on Local Stars
Oh No wrote:
When the position of SgrA* is measured do they have to take into account gravitational red shift of light emanating from the centre of the galaxy? Of course this would not affect distant quasars. All that's measured (for a point source) is its instantaneous position on the sky. ("Instantaneous" means over the interval of observation, typically a few hours.) Gravitational redshift is irrelevant; the _received_ frequency is determined by the instrument setup, but the _emitted_ frequency could have been anything. The same applies to quasars. In the standard model the contained mass in a given radius, r, including CDM, should be roughly given by v^2/r = GM/r^2 If the mass distribution is spherically symmetric -- supposedly a good approximation for galactic haloes. For a rotation speed of ~235km/s at 8kpc, as determined by Reid and Brunthaler, I think that gives a contained mass of a little over 100Bill Suns. What would the effect on the VLBI calculation of orbital motion be if there were only 55 Bill solar masses within that radius? It wouldn't change the measurement at all. Presumably one would have to adopt a disk-like or at least flatter distribution of matter to be consistent with the measured speed. Whether theory could explain such a distribution would remain to be seen. It doesn't look easy, but theorists can be pretty clever when the data force to be. At the moment, there doesn't seem to be any reason to believe that the dark matter mass is so much lower than theory says. |
#27
|
|||
|
|||
Doppler Tests on Local Stars
"ON" == Oh No writes:
ON Thus spake Steve Willner Quasar positions measured by VLBI agree with those measured by classical astrometry. ON Yes, but in quantum theory when you do a classical measurement the ON wave function collapses. There is a discontinuity in the ON description of motion at the time of measurement. I am also ON expecting a discontinuity in VLBI measurements when carried out ON over a sufficient time that classical astronometry becomes ON possible. Whether the apparent discontinuity in motion of IM ON Pegasi is an instance of that, I would not like to say. You'll have to define your terms quantitatively. Brisken et al. (2003, AJ, 126, 3090) report observations of pulsars over a minimum time baseline of 7 years. At least one pulsar (B1237+25) has a proper motion in excess of 0.1 arcsec/year; over the course of their observations it moved a distance of about 0.8 arcseconds. Does 7 years and 0.8 arcseconds qualify as sufficient for "classical" astrometry? If not, what does? -- Lt. Lazio, HTML police | e-mail: No means no, stop rape. | http://patriot.net/%7Ejlazio/ sci.astro FAQ at http://sciastro.astronomy.net/sci.astro.html |
#28
|
|||
|
|||
Doppler Tests on Local Stars
"ON" == Oh No writes:
ON It is probable others understand a lot more about VLBI than I ON do. When the position of SgrA* is measured do they have to take ON into account gravitational red shift of light emanating from the ON centre of the galaxy? Of course this would not affect distant ON quasars. No, for two reasons. First, the VLBI observations of Sgr A* are continuum measurements. They observe at 43 GHz with several 8-MHz bandwidths, processing everything within each 8-MHz bandwidth. For the sake of illustration, suppose that one of these bands is 43.0 GHz to 43.008 GHz. Pick your favorite value for the expected redshift, z, from the environment of Sgr A*. Provided that Sgr A* emits between 43.0*(1+z) and 43.008*(1+z), their analysis is unchanged. Given that Sgr A* is seen at frequencies much higher than 43 GHz, ignoring z in this case is not a problem. Second, assuming that general relativity is correct (or approximately so), the radiation we see as Sgr A* of course does not come from the black hole itself but its environment. I'm not sure we know the actual distance, but my vague recollection is that it must be several tens if not a few hundred gravitational radii away from the hole. Without plugging in the numbers, I suspect that the gravitational redshift at several tens of gravitational radii from a black hole is not all that large. ON In the standard model the contained mass in a given radius, r, ON including CDM, should be roughly given by ON v^2/r = GM/r^2 ON For a rotation speed of ~235km/s at 8kpc, as determined by Reid ON and Brunthaler, I think that gives a contained mass of a little ON over 100Bill Suns. What would the effect on the VLBI calculation ON of orbital motion be if there were only 55 Bill solar masses ON within that radius? Note that the VLBI calculation is the reverse. The measured quantity is (v/r). There are a variety of estimates for r, but 8 kpc is a reasonable value. In order to obtain your value of M, they would have had to have made a serious error in their analysis. -- Lt. Lazio, HTML police | e-mail: No means no, stop rape. | http://patriot.net/%7Ejlazio/ sci.astro FAQ at http://sciastro.astronomy.net/sci.astro.html |
#29
|
|||
|
|||
Doppler Tests on Local Stars
Oh No wrote:
The thing I find is a different amount of red shift than standard general relativity. Did you mean what you wrote? Red shift is a _measurement_, of displacement of spectral lines of well known absorbing or emitting atoms and molecules; within measurement error, it isn't susceptable to you finding a "different amount" of it. xanthian. |
#30
|
|||
|
|||
Doppler Tests on Local Stars
Thus spake Kent Paul Dolan
Oh No wrote: The thing I find is a different amount of red shift than standard general relativity. Did you mean what you wrote? Red shift is a _measurement_, of displacement of spectral lines of well known absorbing or emitting atoms and molecules; within measurement error, it isn't susceptable to you finding a "different amount" of it. Clearly I need to be more precise. I find a different amount of red shift than standard general relativity for a given age/distance/velocity of the source. Since the measured redshift is clearly fixed, the measurement yields a different value for the age/distance/velocity. Regards -- Charles Francis moderator sci.physics.foundations. substitute charles for NotI to email |
Thread Tools | |
Display Modes | |
|
|
Similar Threads | ||||
Thread | Thread Starter | Forum | Replies | Last Post |
Gravitational Doppler | [email protected] | Astronomy Misc | 138 | March 28th 07 07:44 PM |
Gravitational Doppler | [email protected] | Astronomy Misc | 0 | July 31st 06 08:44 AM |
Gravitational Doppler | [email protected] | Astronomy Misc | 12 | July 28th 06 08:41 AM |
redshift Vs doppler shift | Maximus | Misc | 0 | July 1st 05 10:19 AM |