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- The electromagnetic field at a point ''p'' (i.e. an event) of a Lorentzian spacetime is represented by a [[Real number|real]] bivector {{nowrap|1=''F'' = ''F''< ...]. To simplify the notation, we will assume the spacetime ''is'' Minkowski spacetime. This tends to blur the distinction between the tangent space at ''p'' and ...8 KB (1,152 words) - 15:36, 16 February 2024
- ...or current''', it is used in the geometric context of ''four-dimensional [[spacetime]]'', rather than separating time from [[three-dimensional space|three-dimen Using the [[Minkowski metric]] <math>\eta_{\mu\nu}</math> of [[metric signature]] {{nowrap|(+ − − ...6 KB (849 words) - 16:44, 2 December 2023
- ...eld energy of an [[electromagnetic field]], which must satisfy the (curved-spacetime) ''source-free'' [[Maxwell equations]] appropriate to the given geometry. ...l phenomena is a [[Lorentzian manifold]], which is interpreted as a curved spacetime, and which is specified by defining a [[metric tensor]] <math>g_{ab}</math> ...12 KB (1,792 words) - 05:01, 14 June 2023
- ...escription|Mathematical object that describes the electromagnetic field in spacetime}} ...tensor]] formulation of [[special relativity]] was introduced by [[Hermann Minkowski]]. The tensor allows related physical laws to be written very concisely, an ...16 KB (2,376 words) - 10:20, 5 March 2024
- ...theory]], a branch of modern [[string theory]], describes a 12-dimensional spacetime having two dimensions of time, giving it the [[metric signature]] (10,2).<r ...into a complex plane.<ref name="dinov" /> Introducing it into [[Minkowski spacetime]] allows a generalization of [[Kaluza–Klein theory]].<ref>{{cite book |last ...8 KB (1,184 words) - 08:31, 19 January 2024
- ...]] as a model for (3+1)-dimensional [[spacetime]], representing a point in spacetime via a [[paravector]] (3-dimensional vector plus a 1-dimensional scalar). ...rd algebra]] Cl<sub>1,3</sub>('''R''') of the four-dimensional [[Minkowski spacetime]]. ...11 KB (1,521 words) - 15:56, 1 October 2023
- ...f> The stress–energy tensor describes the flow of energy and momentum in [[spacetime]]. The electromagnetic stress–energy tensor contains the negative of the cl ...{\mu\nu}</math> is the [[Metric tensor (general relativity)#Flat spacetime|Minkowski metric tensor]] of [[metric signature]] {{nowrap|(− + + +)}}. When using th ...8 KB (1,135 words) - 01:19, 26 February 2024
- ...Minkowski diagram (and a straight line is a [[geodesic]] in flat Minkowski spacetime), or the coordinate distance between the events in the inertial frame where ...cetime is "inertial", but in the local neighborhood of any point in curved spacetime we can define a "local inertial frame" in which the local speed of light is ...18 KB (2,863 words) - 22:48, 3 December 2023
- ...he most physical interest. We view <math>\mathbb R^n</math> as [[Minkowski spacetime]]. Since the [[gauge group]] of [[electromagnetism]] is <math>U(1)</math>, ...5 KB (790 words) - 10:02, 7 August 2023
- ...nother. However, this is not as general as [[Maxwell's equations in curved spacetime]] or non-rectilinear coordinate systems. ...nt of tensors]] and [[Einstein summation convention]] throughout and the [[Minkowski metric]] has the form {{math|diag(+1, −1, −1, −1)}}. Where the equations ar ...25 KB (3,600 words) - 17:34, 4 February 2024
- ...]]; the [[pseudo-Riemannian manifold]]s of [[general relativity]] describe spacetime with matter and gravity. 10 dimensions are used to describe [[superstring t ...sup>}} such small balls. This observation leads to the definition of the [[Minkowski dimension]] and its more sophisticated variant, the [[Hausdorff dimension]] ...34 KB (4,877 words) - 10:34, 13 February 2024
- ...t||the formulation in [[general relativity]]|Maxwell's equations in curved spacetime|the [[manifestly covariant]] formulation in [[special relativity]]|Classica ===Spacetime algebra=== ...42 KB (6,427 words) - 17:25, 15 February 2024
- ...undless [[four-dimensional]] [[Continuum (theory)|continuum]] known as ''[[spacetime]]''.<ref name="metafizika">{{cite journal|last1=Bunyadzade |first1=Konul |t ...ncept that space and time can be viewed as a single construct known as ''[[spacetime]]''. In this theory, the [[speed of light]] in [[vacuum]] is the same for a ...34 KB (5,050 words) - 01:42, 7 March 2024
- where <math>\mu=\{0,1,2,3\}</math> denotes four indices of the [[spacetime]] and [[Einstein notation|Einstein's summation convention]] has been applie ...th>g^{\mu\nu}=\rm{diag}\{1,-1,-1,-1\}</math> is the metric tensor of the [[Minkowski space]]. ...10 KB (1,489 words) - 18:56, 14 January 2024
- ...Lectures on Physics }}</ref> and its [[motion (physics)|motion]] through [[spacetime]], along with related concepts such as [[energy]] and [[force]].<ref>{{cite ...ton|Sands|1963|p=I-2}}</ref> and its [[Motion (physics)|motion]] through [[Spacetime|space and time]], along with related concepts such as [[energy]] and [[forc ...33 KB (4,348 words) - 13:11, 24 February 2024
- ...stress–energy tensor]], into [[Einstein field equations]] that include the spacetime curvature.</ref> In fact, [[Albert Einstein]] developed special and general {{For|the equations in [[general relativity]]|Maxwell's equations in curved spacetime}} ...81 KB (11,800 words) - 00:24, 4 March 2024
- ...of [[special relativity]], and it turns out that the [[conformal group of spacetime]] includes the [[Lorentz group]] and the [[Poincaré group]] as subgroups. H ...esponds to the above Cayley metric (based on a real conic section), if the spacetime coordinates are identified with the above homogeneous coordinates ...55 KB (7,904 words) - 15:30, 2 September 2023
- ...tly depending on relative motion, and [[space]] and time are merged into [[spacetime]], where we live on a [[world line]] rather than a timeline. In this view t ===Einstein's physics: spacetime=== ...44 KB (6,747 words) - 20:40, 12 January 2024
- ...reference frame]]. Also conserved is the vector length ([[Minkowski space|Minkowski norm]]), which is the [[rest mass]] for single particles, and the [[invaria ...e with time) or asymptotically flat (that is, at an infinite distance away spacetime looks empty), then energy conservation holds without major pitfalls. In pra ...45 KB (6,756 words) - 14:54, 28 February 2024
- {{Spacetime|cTopic=Types}} ...nto a single [[four-dimensional]] [[continuum (measurement)|continuum]]. [[Spacetime diagram]]s are useful in visualizing and understanding [[Special relativity ...197 KB (29,900 words) - 06:15, 7 March 2024