Talk:Hubble's law
Talk:Hubble's law Question -- Avramov 08:36, 4 ... times. How is this possible! H(t) Hubble's constant does indeed decrease over time ... zero cosmological constant. The cosmological constant causes Hubble's constant to decrease slower (resulting in ... expansion), but a constant or even increasing Hubble's constant is not contained in any ... would have extremely strange consequences. --AxelBoldt The Hubble parameter can remain constant, for $...$
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Anyone who's bored can remove the links on here to existing article (not just redirect pages). I only want the reds and redirects.
... arpent area]] #[[arpent length]] #[[ascending node]] #[[asymmetry parameter]] #[[athermalization]] #[[atmospheric diffusion]] #[[atmospheric layers]] #[[atomic decay ... buckling length]] #[[bulk modulus]] #[[bulk viscosity]] #[[bullen parameter]] #[[buoyancy force]] #[[buoyancy oscillation]] #[[buoyancy pressure]] #[[Buys ... copenhagen problem]] #[[coriolis acceleration]] #[[coriolis frequency]] #[[coriolis parameter]] #[[correlation interferometer]] #[[cosmic background radiati...]] #[[cosmic censorship ... Debye-Falkenhagen effect]] | [[debye-falkenhagen effect]] #[[deceleration parameter]] #[[decibel scale]] | [[decibel]] #[[deflection angle]] #[[deformable body ... reflection]] #[[diffusion coefficient]] #[[diffusion equation]] #[[dimensional analysis]] #[[dimensionless logarithmic...]] #[[dipole antenna]] #[[dipole approximation]] #[[dipole ...
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User talk:Salsb/Missing physics
... arpent area arpent length ascending node asymmetry parameter athermalization atmospheric diffusion atmospheric layers atomic decay ... buckling length bulk modulus bulk viscosity bullen parameter buoyancy force buoyancy oscillation buoyancy pressure Buys ... copenhagen problem coriolis acceleration coriolis frequency coriolis parameter correlation interferometer cosmic background radiati... cosmic censorship ... Debye-Falkenhagen effect | debye-falkenhagen effect deceleration parameter decibel scale | decibel deflection angle deformable body ... reflection diffusion coefficient diffusion equation dimensional analysis dimensionless logarithmic... dipole antenna dipole approximation dipole ...
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Variable speed of light
... meaningful as investigating a change in the dimensionless fundamental physical constants such as the fine ... only human constructs. They assert ultimately only dimensionless quantities are measured or perceived by our ... c, G, h, ε 0 remain, only dimensionless quantities. Shorn of their anthropometric unit dependence ... of worlds are the values of the dimensionless constants of Nature. If all masses were ... may be viewed as unitless (but not dimensionless) because the theory of relativity indicates ...
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Talk:Universe
... Gpc (where h=0.7 is the Hubble constant) OK :), this is approximately correct for ... to say that the next second the Hubble telescope will not see a 'boundary' somewhere ... of the universe (other methods typically involve Hubble law and maximum age of stars, etc ... how different methods for determining the same parameter (in this case – the age of ... factor” a=R/Ro, which would be dimensionless regardless of how you represented R. ...
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Ultimate fate of the universe
... matter FLRW metric Friedmann equations Galaxy formation Hubble's law Inflation Large-scale structure Lambda ... is, essentially, the Big Bang. An important parameter in fate of the universe theory is the density parameter, Omega (Ω), defined as the average matter ... not long in coming. In 1929, Edwin Hubble published his conclusion, based on his observations ... that the universe would remain static. After Hubble announced his conclusion that the universe ...
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Scale factor (Universe)
Scale factor (Universe) The scale factor, parameter of Friedmann-Lemaître-Robertson-Walker model, is ... principle, have units of length or be dimensionless. Most commonly in modern usage, it is chosen to be dimensionless, with the current value equal to one ... homogeneous universe by the Friedmann equations. The Hubble parameter is defined: $H\; =\; \{\backslash dot\{a\}(\; ...$
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Self creation cosmology
... matter FLRW metric Friedmann equations Galaxy formation Hubble's law Inflation Large-scale structure Lambda ... In the new SCC, the Brans Dicke parameter $\backslash lambda$ has been determined to ... left( x^\mu \right) is the dimensionless Newtonian gravitational potential, defined by a measurement ... the total matter (visible and Dark) density parameter $\backslash Omega\_m\; =\; 0.22$, and the false vacuum energy density parameter $\backslash Omega\_\{\backslash Lambda\}\; =\; 0.11$. ...
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User:Patrick/wt
... observable Talk:Universe, with a matter density parameter of approximately 30% of the Talk:critical ... Talk:Gravity Research Foundation Talk:Standard gravitational parameter Talk:Weight Talk:N-body problem Gravity ... 4 kg 10 t 11 t Talk:Hubble Space Telescope 12 t largest Talk:elephant ... area, volume, mass, energy, power, temperature and dimensionless numbers. Time Length Area Volume Mass Energy ...
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Equation of state (cosmology)
... a perfect fluid is characterized by a dimensionless number w, equal to the ratio of ... math>, where the constant H is the Hubble parameter. More generally, the universe is accelerating for ...
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