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#31
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Beyond IDCS J1426.5+3508
In article , "Richard D. Saam"
writes: On 9/10/12 7:18 PM, Phillip Helbig---undress to reply wrote: Right. However, what does it mean that it is 2.5 percent of the present universe? What is the luminosity distance to z=infinity? (Hint: much larger than the speed of light times the age of the universe.) Yes, one can express it as a percentage, but the question is whether this is useful. Yes in the conventional view, luminosity distance to z=infinity is much larger than speed of light times the age of the universe. This points to an error in concept. What is the error? What is a non linear distance function of redshift such that distance approaches speed of light times the age of the universe as redshift approaches infinity? If that is what you want, then you can just define your distance as the speed of light multiplied by the light-travel time. |
#32
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Beyond IDCS J1426.5+3508
In article , "Richard D. Saam"
writes: It is understood that universe radius is subject to the particular model used and can be expressed as a function of z A model can be used wherein the Hubble sphere expands at c This is not relevant to the main thread, but perhaps interesting nonetheless: The Hubble sphere is, by definition, at the distance at which the current velocity (proper distance per proper time) of recession due to cosmological expansion is the speed of light. If the Hubble constant is constant in time (which is true in the case of exponential expansion, e.g. in the de Sitter model), then the Hubble sphere has a fixed size. If the Hubble constant decreases, the Hubble sphere expands. At a given time, one could have a model in which the Hubble sphere expands with c. I don't think there is a conventional cosmological model (i.e. one described by the Friedmann-Lemaître equation) in which the Hubble sphere expands with c at all times. The radius of the universe is generally understood to be the radius of curvature of the universe. It could be equal to the Hubble radius, but not in general. (If the radius of curvature is infinite, i.e. in a flat universe, then the scale factor is often DEFINED as the radius of the Hubble sphere, rather than the curvature radius.) The scale factor changes with time. Since the ratio of the scale factor now to that at a previous time is just 1+z, then the relationship between the scale factor and redshift is trivial (though the relationship between the scale factor and time, or the redshift and time, is not). The particle horizon expands (locally) at the speed of light in all cosmological models, always increases with time (at least in comoving coordinates) and corresponds to what is generally thought of as the observable universe. It doesn't have much connection with the Hubble sphere. |
#33
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Beyond IDCS J1426.5+3508
On 9/11/12 10:03 AM, Phillip Helbig---undress to reply wrote:
In article , "Richard D. Saam" writes: It is understood that universe radius is subject to the particular model used and can be expressed as a function of z A model can be used wherein the Hubble sphere expands at c This is not relevant to the main thread, but perhaps interesting nonetheless: The Hubble sphere is, by definition, at the distance at which the current velocity (proper distance per proper time) of recession due to cosmological expansion is the speed of light. If the Hubble constant is constant in time (which is true in the case of exponential expansion, e.g. in the de Sitter model), then the Hubble sphere has a fixed size. If the Hubble constant decreases, the Hubble sphere expands. At a given time, one could have a model in which the Hubble sphere expands with c. I don't think there is a conventional cosmological model (i.e. one described by the Friedmann-Lemaître equation) in which the Hubble sphere expands with c at all times. referencing Harrison equation 16.4 for universal expanding sphe (dR/dt)^2 = (8/3)*pi*G*rho*R^2 dR/dt could equal constant c at all times if G*(1+z)^n gravitational parameter rho*(1+z)^n universe density parameter R*(1+z)^-n universe radius parameter perhaps n=1 for Hubble sphere and n=3 for particle horizon which would not negate the Friedmann-Lemaître equation. |
#34
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Beyond IDCS J1426.5+3508
In article , "Richard D. Saam"
writes: The Hubble sphere is, by definition, at the distance at which the current velocity (proper distance per proper time) of recession due to cosmological expansion is the speed of light. referencing Harrison equation 16.4 A good reference. Harrison wrote a couple of papers distinguishing concepts which are often confused, including horizons and Hubble spheres. for universal expanding sphe (dR/dt)^2 = (8/3)*pi*G*rho*R^2 Right, but that is not necessarily Hubble sphere. dR/dt could equal constant c at all times if G*(1+z)^n gravitational parameter rho*(1+z)^n universe density parameter R*(1+z)^-n universe radius parameter Presumably you mean replacing G with G*(1+z)^n etc? |
#35
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Beyond IDCS J1426.5+3508
On 9/14/12 4:52 AM, Phillip Helbig---undress to reply wrote:
Right, but that is not necessarily Hubble sphere. not necessarily but let R be constrained to Hubble length c/H Presumably you mean replacing G with G*(1+z)^n etc? Yes and for present values G = G rho = (3*H^2/(8*pi*G) R = c*H (dR/dt)^2 = (8/3)*pi*G*(1+z)^n*rho*(1+z)^n*(R*(1+z)^-n)^2 = c^2 The expression collapses to c^2 for all z but is there any meaning in the uncollapsed form? It is interesting to note that the expression with n=3 G*(1+z)^3 rho*(1+z)^3 R*(1+z)^-3 is dimensionally and numerically consistent with CMBR temperature scaling with (1+z)^1 as observed. The Hubble sphere may contain another coordinate system (represented by CMBR temperature scaling) that expands differently but in a well defined manner relative to the Hubble sphere R^3. A big question results: Does Newtonian G scale with z G*(1+z)^3 ? [Mod. note: quoted text trimmed. In the local universe (z1), we can write lookback time t = z/H_0, thus G = G_0(1+z)^3 = (binomial expansion) G = G_0(1+3z) = G = G_0(1+3H_0t) = dG/dt = 3G_0 H_0 = (dG/dt)/G_0 = 3H_0 where 3H_0 = 2.1e-10 yr^-1. Current experimental evidence puts an upper limit on (dG/dt)/G of a few times 10^-12 yr^-1 (http://arxiv.org/abs/gr-qc/0411113). So this strong a scaling is inconsistent with experiment -- mjh] |
#36
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Beyond IDCS J1426.5+3508
In article , "Richard D. Saam"
writes: On 9/14/12 4:52 AM, Phillip Helbig---undress to reply wrote: Right, but that is not necessarily Hubble sphere. not necessarily but let R be constrained to Hubble length c/H Presumably you mean replacing G with G*(1+z)^n etc? Yes and for present values G = G rho = (3*H^2/(8*pi*G) R = c*H (dR/dt)^2 = (8/3)*pi*G*(1+z)^n*rho*(1+z)^n*(R*(1+z)^-n)^2 = c^2 You need to specify a) what you are postulating and what you are deriving and b) the physics (e.g. general relativity or something else) which is used in your derivation. What is R? Is it some scale factor, is it the radius of curvature or is it both? (Convention is to choose the scale factor to be equal to the radius of curvature except when the latter is infinite in which the scale factor is set to 1---all in units of c/H_0.) |
#37
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Beyond IDCS J1426.5+3508
On 9/17/12 9:34 AM, Richard D. Saam wrote:
A big question results: Does Newtonian G scale with z G*(1+z)^3 ? [Mod. note: quoted text trimmed. In the local universe (z1), we can write lookback time t = z/H_0, thus G = G_0(1+z)^3 = (binomial expansion) G = G_0(1+3z) = G = G_0(1+3H_0t) = dG/dt = 3G_0 H_0 = (dG/dt)/G_0 = 3H_0 where 3H_0 = 2.1e-10 yr^-1. Current experimental evidence puts an upper limit on (dG/dt)/G of a few times 10^-12 yr^-1 (http://arxiv.org/abs/gr-qc/0411113). So this strong a scaling is inconsistent with experiment -- mjh] but is the observed dG/dt)/G of a few times 10^-12 yr^-1 (essentially constant) a consequence of G*(1+z)^3*R*(1+z)^-3 = constant and also rho*(1+z)^3*R*(1+z)^-3 = constant because speed of GR gravity is the same as Newtonian gravity that is infinite http://math.ucr.edu/home/baez/physic...rav_speed.html ? |
#38
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Beyond IDCS J1426.5+3508
In article , "Richard D. Saam"
writes: but is the observed dG/dt)/G of a few times 10^-12 yr^-1 (essentially constant) a consequence of G*(1+z)^3*R*(1+z)^-3 = constant This reduces to G*R = constant. and also rho*(1+z)^3*R*(1+z)^-3 = constant This reduces to rho*R = constant Due to conservation of matter, rho should be proportional to (1+z)^3. Again, since these equations imply a very different universe than the one we live in, and even a very different one than the possible ones which exist given the known laws of physics, such a discussion makes sense only if it is clear what is postulated (and why) and what is derived (and how). because speed of GR gravity is the same as Newtonian gravity that is infinite http://math.ucr.edu/home/baez/physic...rav_speed.html ? No. In GR gravity propagates at the speed of light. What you might be thinking of is that people often assume it propagates at the speed of light. This is wrong, but something else is wrong as well: it should propagate from where the object was then, not where it is now. It turns out that the two effects cancel. |
#39
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Beyond IDCS J1426.5+3508
Richard D. Saam wrote:
but is the observed dG/dt)/G of a few times 10^-12 yr^-1 (essentially constant) Actually the limits are considerably tighter than that. Quoting section 3 of Stephen M. Merkowitz "Tests of Gravity Using Lunar Laser Ranging", Living Reviews in Relativity 13 (2010), 7 http://www.livingreviews.org/lrr-2010-7 (n.b. this is online open-access!), | Recent analysis of LLR data by the JPL group sets a limit on | (dG/dt)/G = (6 +/- 7) * 10^{-13}/year [69]. Similarly, Mueller | et al find (dG/dt)/G = (2 +/- 7) * 10^{-13}/year and | and (d^2G/dt^2)/G = (4 +/- 5) * 10^{-15}/year^2 [35]. | These limits translate to less than a 1% variation of G over | the 13.7 billion year age of the universe. ciao, -- -- "Jonathan Thornburg [remove -animal to reply]" Dept of Astronomy & IUCSS, Indiana University, Bloomington, Indiana, USA currently on sabbatical in Canada "Washing one's hands of the conflict between the powerful and the powerless means to side with the powerful, not to be neutral." -- quote by Freire / poster by Oxfam |
#40
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Beyond IDCS J1426.5+3508
On 9/18/12 4:35 AM, Phillip Helbig---undress to reply wrote:
because speed of GR gravity is the same as Newtonian gravity that is infinite http://math.ucr.edu/home/baez/physic...rav_speed.html ? No. In GR gravity propagates at the speed of light. What you might be thinking of is that people often assume it propagates at the speed of light. This is wrong, but something else is wrong as well: it should propagate from where the object was then, not where it is now. It turns out that the two effects cancel. What Baez is saying is different: "In that case, one finds that the "force" in GR is not quite central—it does not point directly towards the source of the gravitational field—and that it depends on velocity as well as position. The net result is that the effect of propagation delay is almost exactly cancelled, and general relativity very nearly reproduces the newtonian result." Such an explanation could explain in part the world we live in wherein the observed dG/dt)/G of a few times 10^-12 yr^-1 (essentially constant) no matter where you look. Such an explanation appears to outside of current universe expansion models. |
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