The **Milne model** was a cosmological model proposed by Edward Arthur Milne. Milne was able to use Lorentz transformation formalisms to derive a model of an **empty universe** that has no curvature. Image File history File links example of a light cone created in Lightwave by stib File history Legend: (cur) = this is the current file, (del) = delete this old version, (rev) = revert to this old version. ...
Image File history File links example of a light cone created in Lightwave by stib File history Legend: (cur) = this is the current file, (del) = delete this old version, (rev) = revert to this old version. ...
The special theory of relativity was proposed in 1905 by Albert Einstein in his article On the Electrodynamics of Moving Bodies. ...
The observable Universe is a term used in cosmology to describe a ball-shaped region of space surrounding the Earth that is close enough that we might observe objects in it. ...
The Minkowski diagram is a graphical tool used in special relativity to visualize spacetime with regard to an inertial reference frame. ...
In special relativity, a light cone is the pattern describing the temporal evolution of a flash of light in Minkowski spacetime. ...
Cosmology, as a branch of astrophysics, is the study of the large-scale structure of the universe and is concerned with fundamental questions about its formation and evolution. ...
Image File history File links Download high resolution version (2198x1274, 1278 KB)WMAP map of CMB anisotropy, from NASA.gov File history Legend: (cur) = this is the current file, (del) = delete this old version, (rev) = revert to this old version. ...
Nothing is certain as to the extent of either the age or size of the universe, but the age of the Universe, according to the Big Bang theory, is defined as the largest possible value of proper time integrated along a timelike curve from the Earth at the present epoch...
According to the Big Bang theory, the universe emerged from an extremely dense and hot state (bottom). ...
The comoving distance or conformal distance of two objects in the universe is the distance divided by a time-varying scale factor representing the expansion of the universe. ...
In cosmology, the cosmic microwave background radiation (most often abbreviated CMB but occasionally CMBR, CBR or MBR) is a form of electromagnetic radiation discovered in 1965 that fills the entire universe. ...
In physical cosmology, dark energy is a hypothetical form of energy which permeates all of space and has strong negative pressure. ...
In astrophysics, dark matter refers to matter that does not emit or reflect enough electromagnetic radiation (such as light, x-rays and so on) to be detected directly, but whose presence may be inferred from its gravitational effects on visible matter. ...
The Friedmann-LemaÃ®tre-Robertson-Walker (FLRW) metric describes a homogeneous, isotropic expanding/contracting universe. ...
The Friedmann equations relate various cosmological parameters within the context of general relativity. ...
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Hubbles law is the statement in physical cosmology that the redshift in light coming from distant galaxies is proportional to their distance. ...
Astronomy and cosmology examine the universe to understand the large-scale structure of the cosmos. ...
A pie chart indicating the proportional composition of different energy-density components of the universe. ...
The metric expansion of space is a key part of sciences current understanding of the universe, whereby space itself is described by a metric which changes over time. ...
In cosmology, Big Bang nucleosynthesis (or primordial nucleosynthesis) refers to the production of nuclei other than H-1, the normal, light hydrogen, during the early phases of the universe, shortly after the Big Bang. ...
The observable Universe is a term used in cosmology to describe a ball-shaped region of space surrounding the Earth that is close enough that we might observe objects in it. ...
Redshift of spectral lines in the optical spectrum of a supercluster of distant galaxies (right), as compared to that of the Sun (left). ...
The shape of the Universe is a subject of investigation within cosmology. ...
A graphical timeline is available here: Graphical timeline of the Big Bang This timeline of the Big Bang describes the events that have occurred and will occur according to the scientific theory of the Big Bang. ...
The timeline of cosmology lists the sequence of cosmological theories and discoveries in chronological order. ...
The ultimate fate of our universe is a topic in physical cosmology. ...
The deepest visible-light image of the cosmos, the Hubble Ultra Deep Field. ...
Spiral Galaxy ESO 269-57 Astrophysics is the branch of astronomy that deals with the physics of the universe, including the physical properties (luminosity, density, temperature and chemical composition) of celestial objects such as stars, galaxies, and the interstellar medium, as well as their interactions. ...
General relativity (GR) is the geometrical theory of gravitation published by Albert Einstein in 1915. ...
Particles explode from the collision point of two relativistic (100 GeV per nucleon) gold ions in the STAR detector of the Relativistic Heavy Ion Collider. ...
Quantum gravity is the field of theoretical physics attempting to unify the theory of quantum mechanics, which describes three of the fundamental forces of nature, with general relativity, the theory of the fourth fundamental force: gravity. ...
Cosmology, as a branch of astrophysics, is the study of the large-scale structure of the universe and is concerned with fundamental questions about its formation and evolution. ...
Look up model in Wiktionary, the free dictionary. ...
Edward Arthur Milne (February 14, 1896 – September 21, 1950) was a British mathematician and astrophysicist. ...
A Lorentz transformation (LT) is a linear transformation that preserves the spacetime interval between any two events in Minkowski space, while leaving the origin fixed (=rotation of Minkowski space). ...
Curvature refers to a number of loosely related concepts in different areas of geometry. ...
## Milne metric
The Milne Metric is flat space. It is not similar to Einstein's static universe, however, because in Milne's model, the particles are moving apart. In Einstein's static universe, the particles were all standing still. Friedmann's solution to the Einstein Field Equations requires that a constant uniform density somehow affects the curvature of three dimensional space in a higher dimensional space. Milne argues against this idea, repudiating the assumptions that led to the Friedmann solution. Even so, cosmologists like to see what Milne's model says as viewed through the FLRW model, and it says the following: The more general Friedmann, Lemaitre, Robertson, Walker Metric (FLRW metric) reduces to the Milne universe for a spacetime that is a pure vacuum without matter, radiation, or a cosmological constant. Milne cosmology therefore corresponds to a cosmological solution to the Einstein equations for In physics, spacetime is a model that combines three-dimensional space and one-dimensional time into a single construct called the space-time continuum, in which time plays the role of the 4th dimension. ...
Matter is commonly defined as the substance of which physical objects are composed. ...
Electromagnetic radiation can be conceptualized as a self propagating transverse oscillating wave of electric and magnetic fields. ...
The cosmological constant (usually denoted by the Greek capital letter lambda: Î›) occurs in Einsteins theory of general relativity. ...
*T*_{ab} = 0. The Milne metric follows when the scale factor of the FRLW metric is a constant over time, yielding: The scale factor, parameter of Friedmann-LemaÃ®tre-Robertson-Walker model, is a function of time which represents the relative expansion of the universe. ...
*d**s*^{2} = *c*^{2}*d**t*^{2} − *d**r*^{2} − *r*^{2}*d*Ω^{2} where: *d*Ω^{2} = *d*θ^{2} + sin^{2}θ*d*φ^{2} *r* gives the proper motion distance between points in the universe. and appropriate constants are subsumed into relevant coordinates. The Milne metric is therefore simply a restatement of the Minkowski metric. In physics, proper length is the length of an object or a contour as measured in the reference frame of the object itself in the context of special relativity. ...
In physics and mathematics, Minkowski space (or Minkowski spacetime) is the mathematical setting in which Einsteins theory of special relativity is most conveniently formulated. ...
There are two types of motion in the galaxy. That which goes along with Hubble flow and Peculiar velocity which is motion of a freely projected particle or galaxy relative to the Hubble flow. In cosmology, the Hubble expansion is the motion of galaxies away from each other, due to the expansion of the universe. ...
The term peculiar velocity refers to the components of a receding galaxys velocity that cannot be explained by Hubbles law. ...
Whereas the FLRW metric explains all of the redshift associated with the Hubble flow by the metric expansion of space, Milne's model has no expansion of space, thus all of the Hubble flow redshift is explained by the recessional velocity associated with the hypothetical explosion. The metric expansion of space is a key part of sciences current understanding of the universe, whereby space itself is described by a metric which changes over time. ...
Recessional Velocity is a term used to describe the rate at which an object is moving away, typically from Earth. ...
## Milne's density function Milne proposed that the universe's density changes in time because of an initial outward explosion of matter. Milne's model assumes an inhomogeneous density function which is Lorentz Invariant (around the event t=x=y=z=0). When rendered graphically Milne's density distribution shows a three-dimensional spherical Lobachevskian pattern with outer edges moving outward at the speed of light. Every inertial body perceives itself to be at the center of the explosion of matter (see observable universe). From such a perspective, the universe appears isotropic though not homogeneous. The observable Universe is a term used in cosmology to describe a ball-shaped region of space surrounding the Earth that is close enough that we might observe objects in it. ...
Unless the universe modeled has zero density, Milne's proposal does not follow the predictions of general relativity for the curvature of space caused by global matter distribution, as seen in, for example statistics associated with large-scale structure. General relativity (GR) is the geometrical theory of gravitation published by Albert Einstein in 1915. ...
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## Differences between Milne model and other models In order to explain the existence of matter in the universe, Milne proposed a physical explosion of matter which would not affect the universe's geometry. This is in contrast to the metric expansion of space that is the hallmark feature of many of the more famous cosmological models including the Big Bang and Steady State models. Milne's universe shares a superficial similarity to Einstein's static universe in that the metric of space is not time-dependent They are superficially similar in the sense that an explosion in a room is superficially similar to a bunch of cobwebs in a room. i.e. the room is the same.) The metric expansion of space is a key part of sciences current understanding of the universe, whereby space itself is described by a metric which changes over time. ...
According to the Big Bang theory, the universe emerged from an extremely dense and hot state (bottom). ...
For alternative meanings see steady state (disambiguation). ...
Basic description The theory of a static universe is the rival theory to an expanding universe and all of its subvarieties. ...
See: International System of Units, colloquially called the Metric System, and also metrication. ...
Space has been an interest for philosophers and scientists for much of human history, and hence it is difficult to provide an uncontroversial and clear definition outside of specific defined contexts. ...
Unlike Einstein's initial cosmology, Milne's proposal directly contradicts the Einstein equations for cosmological scales. Special relativity becomes a global property of Milne's universe while general relativity is confined to a local property. The reverse is true for standard cosmological models, and most scientists and mathematicians agree that the latter is self-consistent while the former is mathematically impossible. The special theory of relativity was proposed in 1905 by Albert Einstein in his article On the Electrodynamics of Moving Bodies. ...
General relativity (GR) is the geometrical theory of gravitation published by Albert Einstein in 1915. ...
Milne held up his model as an existence proof that these mathematicions were incorrect. Edward Arthur Milne predicted a kind of event horizon through the use of this model, as can be seen clearly in the last sentence of the plate. "The particles near the boundary tend towards invisibility as seen by the central observer, and fade into a continuous background of finite intensity." Edward Arthur Milne (February 14, 1896 – September 21, 1950) was a British mathematician and astrophysicist. ...
This article or section is in need of attention from an expert on the subject. ...
At the time Milne proposed his model, observations of the universe did not appear to be in a homogeneous form. This, to Milne, was completely compatible with both his own model, and the competing cosmological models which relied on the cosmological principle that demanded a homogeneous universe. What he disliked about the competing models was that they assumed that this homogeneity extended for eternity in all directions, whereas he felt that there was definitely not enough data to support such an assumption. “This conventional homogeneity is only definite when the motion of the particles is first prescribed.” With present observations of the homogeneity of the universe on the largest scales seen in the cosmic microwave background and in the so-called "End of Greatness", questions about the homogeneity of the universe have been settled in the minds of most observational cosmologists. However our observations only extend out to about 10 or 15 billion light years. At these distances, it is unclear whether the density is the same as it is here, or if it is affected by the effects of high recession velocity which would be predicted by Special Relativity. Milne's model says that the universe at these distances is younger and denser than it is locally. Look up Homogeneous in Wiktionary, the free dictionary. ...
The Cosmological Principle is a principle invoked in cosmology that severely restricts the large variety of possible cosmological theories: On large scales, the Universe is homogeneous and isotropic. ...
WMAP image of the CMB anisotropy,Cosmic microwave background radiation(June 2003) The cosmic microwave background radiation (CMB) is a form of electromagnetic radiation that fills the whole of the universe. ...
Observational cosmology is the study of the structure, the evolution and the origin of the universe through observation, using instruments such as telescopes and cosmic ray detectors. ...
## References Milne, "Relativity, Gravitation and World Structure" http://world.std.com/~mmcirvin/milne.html ("Milne Cosmology, and Why I Keep Talking About It," by Matt McMirvin.") http://www.phys-astro.sonoma.edu/BruceMedalists/Milne/MilneRefs.html Here is a list of further reading on Milne's life and work. |