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World line

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821: 2615:, oversimplify this concept to a one-dimensional timeline to fit a linear structure, which does not fit models of reality. Such time machines are often portrayed as being instantaneous, with its contents departing one time and arriving in another—but at the same literal geographic point in space. This is often carried out without note of a reference frame, or with the implicit assumption that the reference frame is local; as such, this would require either accurate teleportation, as a rotating planet, being under acceleration, is not an inertial frame, or for the time machine to remain in the same place, its contents 'frozen'. 2593:. It was advertised to be a "Mathematical Fantasy"—and it was! The substance of the exercise was as follows: He postulated that, commencing with his birth, every human being had some kind of spiritual aura with a long filament or thread attached, that traveled behind him throughout his life. He then proceeded in imagination to describe the complicated entanglement every individual became involved in his relationship to other individuals, comparing the simple entanglements of youth to those complicated knots that develop in later life. 151: 4191: 834: 2607:“Billy Pilgrim says that the Universe does not look like a lot of bright little dots to the creatures from Tralfamadore. The creatures can see where each star has been and where it is going, so that the heavens are filled with rarefied, luminous spaghetti. And Tralfamadorians don't see human beings as two-legged creatures, either. They see them as great millepedes - "with babies' legs at one end and old people's legs at the other," says Billy Pilgrim.” 43: 2007: 1108: 2648:
behind you more of this space-time event, reaching to perhaps nineteen-sixteen, of which we see a cross-section here at right angles to the time axis, and as thick as the present. At the far end is a baby, smelling of sour milk and drooling its breakfast on its bib. At the other end lies, perhaps, an old man someplace in the nineteen-eighties.
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He stepped up to one of the reporters. "Suppose we take you as an example. Your name is Rogers, is it not? Very well, Rogers, you are a space-time event having duration four ways. You are not quite six feet tall, you are about twenty inches wide and perhaps ten inches thick. In time, there stretches
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events corresponding to the history of the object. A world line is a special type of curve in spacetime. Below an equivalent definition will be explained: A world line is either a time-like or a null curve in spacetime. Each point of a world line is an event that can be labeled with the time and the
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Quantum field theory, the framework in which all of modern particle physics is described, is usually described as a theory of quantized fields. However, although not widely appreciated, it has been known since Feynman that many quantum field theories may equivalently be described in terms of world
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A line at constant space coordinate (a vertical line using the convention adopted above) may represent a particle at rest (or a stationary observer). A tilted line represents a particle with a constant coordinate speed (constant change in space coordinate with increasing time coordinate). The more
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are inaccessible to them; only points in the past can send signals to the observer. In ordinary laboratory experience, using common units and methods of measurement, it may seem that we look at the present, but in fact there is always a delay time for light to propagate. For example, we see the
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to their world line. It is really three-dimensional, though it would be a 2-plane in the diagram because we had to throw away one dimension to make an intelligible picture. Although the light cones are the same for all observers at a given spacetime event, different observers, with differing
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Often the time units are chosen such that the speed of light is represented by lines at a fixed angle, usually at 45 degrees, forming a cone with the vertical (time) axis. In general, useful curves in spacetime can be of three types (the other types would be partly one, partly another type):
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curves, having at each point the speed of light. They form a cone in spacetime, dividing it into two parts. The cone is three-dimensional in spacetime, appears as a line in drawings with two dimensions suppressed, and as a cone in drawings with one spatial dimension
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World lines of a particle and an observer may be interconnected with the world line of a photon (the path of light) and form a diagram depicting the emission of a photon by a particle that is subsequently observed by the observer (or absorbed by another particle).
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can be represented by the coordinates as a function of one parameter. Each value of the parameter corresponds to a point in spacetime and varying the parameter traces out a line. So in mathematical terms a curve is defined by four coordinate functions
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All curves through point p have a tangent vector, not only world lines. The sum of two vectors is again a tangent vector to some other curve and the same holds for multiplying by a scalar. Therefore, all tangent vectors for a point p span a
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is the analogous two-dimensional surface traced out by a one-dimensional line (like a string) traveling through spacetime. The world sheet of an open string (with loose ends) is a strip; that of a closed string (a loop) resembles a tube.
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then they share the same simultaneous hyperplane. This hyperplane exists mathematically, but physical relations in relativity involve the movement of information by light. For instance, the traditional electro-static force described by
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of the Earth in space is approximately a circle, a three-dimensional (closed) curve in space: the Earth returns every year to the same point in space relative to the sun. However, it arrives there at a different (later) time. The
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The momentarily co-moving inertial frames along the trajectory ("world line") of a rapidly accelerating observer (center). The vertical direction indicates time, while the horizontal indicates distance, the dashed line is the
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A curve that consists of a horizontal line segment (a line at constant coordinate time), may represent a rod in spacetime and would not be a world line in the proper sense. The parameter simply traces the length of the rod.
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or "encounter". Two world lines starting at the same event in spacetime, each following its own path afterwards, may represent e.g. the decay of a particle into two others or the emission of one particle by another.
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identifying the events. Each event can be labeled by four numbers: a time coordinate and three space coordinates; thus spacetime is a four-dimensional space. The mathematical term for spacetime is a four-dimensional
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whose "time axis" corresponds to that curve, and, since no observer is privileged, we can always find a local coordinate system in which lightcones are inclined at 45 degrees to the time axis. See also for example
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curves fall within the lightcone. However, a lightcone is not necessarily inclined at 45 degrees to the time axis. However, this is an artifact of the chosen coordinate system, and reflects the coordinate freedom
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velocities but coincident at the event (point) in the spacetime, have world lines that cross each other at an angle determined by their relative velocities, and thus they have different simultaneous hyperplanes.
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curves falling outside the light cone. Such curves may describe, for example, the length of a physical object. The circumference of a cylinder and the length of a rod are space-like curves.
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So far a world line (and the concept of tangent vectors) has been described without a means of quantifying the interval between events. The basic mathematics is as follows: The theory of
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at point p. For example, taking a 2-dimensional space, like the (curved) surface of the Earth, its tangent space at a specific point would be the flat approximation of the curved space.
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Why, then, should not the four-dimensional beings be ourselves, and our successive states the passing of them through the three-dimensional space to which our consciousness is confined.
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and can simply be differentiated by the usual calculus. Without the existence of a metric (this is important to realize) one can imagine the difference between a point
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at the given event is formed by all events that can be connected through light rays with the event. When we observe the sky at night, we basically see only the past
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A space armada trying to complete a (nearly) closed time-like path as a strategic maneuver forms the backdrop and a main plot device of "Singularity Sky" by
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of the observer. The small dots are specific events in spacetime. Note how the momentarily co-moving inertial frame changes when the observer accelerates.
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curves, with a speed less than the speed of light. These curves must fall within a cone defined by light-like curves. In our definition above:
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has proved particularly fruitful for various calculations in gauge theories and in describing nonlinear effects of electromagnetic fields.
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of the given event is formed by all events that can influence the event (that is, that can be connected by world lines within the past
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of the given event is formed by all events that can be reached through time-like curves lying within the future light cone.
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A world line of an object (generally approximated as a point in space, e.g., a particle or observer) is the sequence of
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World lines of free-falling particles or objects (such as planets around the Sun or an astronaut in space) are called
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may be pictured in a simultaneous hyperplane, but relativistic relations of charge and force involve
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involves a long discussion of worldlines over dinner in the midst of a philosophical debate between
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Schubert, Christian (2001). "Perturbative quantum field theory in the string-inspired formalism".
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lines. This preceded much of his work on the formulation which later became more standard. The
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Once the object is not approximated as a mere point but has extended volume, it traces not a
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is thick; it is not a 3-dimensional volume but is instead a 4-dimensional spacetime region.
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of the particle. If the worldline M is a line segment, then the particle is said to be in
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in spacetime (a curve in a four-dimensional space) and does not return to the same point.
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and are dependent on the mass-energy distribution in spacetime. Again the metric defines
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puts some constraints on possible world lines. In special relativity the description of
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Three different world lines representing travel at different constant four-velocities.
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Almost all science-fiction stories which use this concept actively, such as to enable
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if its tangent is future timelike at each point. The arclength parameter is called
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in the early days of relativity. As described by Toronto lawyer Norman Robertson:
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Absolute Choice depicts different world lines as a sub-plot and setting device.
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coordinate systems that do not accelerate (and so do not rotate either), termed
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wrote an essay "What is the fourth dimension ?", which he published as a
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in which he related a simplified explanation of the hypothesis for laymen.
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curve in spacetime. This terminology causes confusions. More properly, a
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The concept of a "world line" is distinguished from concepts such as an "
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Two world lines that start out separately and then intersect, signify a
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I remember lecturing at one of the Saturday evening lectures at the
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as it was about 8 minutes ago, not as it is "right now". Unlike the
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defining a world line, are real number functions of a real variable
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is the region between the two light cones. Points in an observer's
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World line, worldsheet, and world volume, as they are derived from
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A world line traces out the path of a single point in spacetime. A
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The Mathematics Department in the University of Toronto, 1827–1978
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for each pair of events. The bilinear form is sometimes termed a
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usually denotes the time coordinate) depending on one parameter
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of a particle, observer or small object. One usually uses the
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is a constant. The structure of spacetime is determined by a
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the line is tilted from the vertical, the larger the speed.
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World lines of freely falling particles/objects are called
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curves. Also, in general relativity, world lines include
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and usually denoted τ. The length of M is called the
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A popular description of human world lines was given by
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often means the single spacetime event being considered.
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Unique path of an object as it travels through spacetime
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in depth text on world lines and special relativity
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are rendered as curves in spacetime to show their (
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When two world lines 3363: 3109: 2965:Annual Review of Nuclear and Particle Science 2115:, which is defined for a given observer by a 2049:At a given event on a world line, spacetime ( 2037:world lines are time-like curves in spacetime 1476:and a point on the curve a little (parameter 1338:Tangent vector to a world line: four-velocity 980:spatial position of the object at that time. 859: 3297:Various English translations on Wikisource: 2556: 1265:is a curve in spacetime that traces out the 1103:World lines as a method of describing events 1063:, horizontally. As expressed by F.R. Harvey 1043:, vertically, and the space coordinate, say 2899: 2511:curves and null curves in spacetime, where 3370: 3356: 2137: 1818: 1787: 1756: 1371: 1165: 951:The idea of world lines was originated by 866: 852: 3132: 3026: 2995: 2977: 127:Learn how and when to remove this message 3223: 3197: 3010: 2017: 2005: 1402:{\displaystyle x^{a}(\tau ),\;a=0,1,2,3} 1300: 1196:{\displaystyle x^{a}(\tau ),\;a=0,1,2,3} 1106: 2957:"Progress in one-loop QCD computations" 2852: 2816: 897:. It is an important concept of modern 14: 4206: 3171: 2783: 2643:describes the world line of a person: 2227:that is time-like, the Minkowski form 2220:{\displaystyle v={\frac {dw}{d\tau }}} 1505:{\displaystyle \tau _{0}+\Delta \tau } 3351: 2696:are also used throughout the series. 1975:of mathematics, the bilinear form is 2332:{\displaystyle x\mapsto \eta (v,x).} 1979:a mathematical metric on spacetime. 1449:on the curve at the parameter value 1297:Trivial examples of spacetime curves 65:adding citations to reliable sources 36: 3942:Tolman–Oppenheimer–Volkoff equation 3895:Friedmann–LemaĂźtre–Robertson–Walker 2544:World lines in quantum field theory 970: 24: 2288:{\displaystyle R^{4}\rightarrow R} 2104:in Galilean/Newtonian theory, the 1955:. In such coordinate systems, the 1548: 1519: 1496: 177: 25: 4235: 3712:Hamilton–Jacobi–Einstein equation 3322: 3181:Scientific Romances: First Series 2531:Eddington-Finkelstein coordinates 2467:World lines in general relativity 2177:{\displaystyle w(\tau )\in R^{4}} 1935:World lines in special relativity 1534:{\displaystyle \Delta \tau \to 0} 4190: 4189: 2347:of this linear functional. Then 833: 832: 819: 149: 41: 3248: 3199:Robinson, Gilbert de Beauregard 3191: 3177:"What is the fourth dimension?" 2184:determines a velocity 4-vector 2111:Included in "elsewhere" is the 2053:) is divided into three parts. 1912:{\displaystyle \tau =\tau _{0}} 1568:of the world line at the point 999:Spacetime is the collection of 52:needs additional citations for 3519:Mass–energy equivalence (E=mc) 3377: 3256:"Technovelgy: Chronovitameter" 3165: 3103: 3059: 3004: 2941: 2893: 2846: 2810: 2777: 2733:Specific types of world lines 2323: 2311: 2305: 2279: 2249: 2237: 2158: 2152: 1653: 1624: 1525: 1365: 1359: 1342:The four coordinate functions 1159: 1153: 13: 1: 3045:10.1016/S0370-1573(01)00013-8 2997:10.1146/annurev.nucl.46.1.109 2770: 2520:) of general relativity. Any 2262:determines a linear function 1541:, this difference divided by 1512:) farther away. In the limit 3097:10.1016/0550-3213(82)90455-2 2955:; Kosower, David A. (1996). 2597:Kurt Vonnegut, in his novel 2475:is basically the same as in 2083:within the entire spacetime. 1557:{\displaystyle \Delta \tau } 7: 3534:Relativistic Doppler effect 3275:Minkowski, Hermann (1909), 3207:University of Toronto Press 2927:10.1103/PhysRevLett.66.1669 2727: 2479:, with the difference that 1953:inertial coordinate systems 890:that an object traces in 4- 330:Gravitational time dilation 10: 4240: 4005:In computational physics: 3529:Relativity of simultaneity 3151:10.1103/PhysRevD.72.105004 2471:The use of world lines in 2361:relativity of simultaneity 2255:{\displaystyle \eta (v,x)} 1633:{\displaystyle {\vec {v}}} 1067:A curve M in is called a 992:of the Earth is therefore 450:Mathisson–Papapetrou–Dixon 291:Pseudo-Riemannian manifold 29: 4187: 4019: 3884: 3856: 3842:Lense–Thirring precession 3725: 3674: 3636: 3615: 3604: 3562: 3506: 3490: 3432: 3424:Doubly special relativity 3396: 3385: 3283:Physikalische Zeitschrift 2784:Harvey, F. Reese (1990). 2557:World lines in literature 2518:diffeomorphism invariance 1469:{\displaystyle \tau _{0}} 1099:but rather a world tube. 940:—to reveal the nature of 3702:Post-Newtonian formalism 3692:Einstein field equations 3628:Mathematical formulation 3452:Hyperbolic orthogonality 3230:Oliver Franklin (2008). 2790:Spinors and Calibrations 2673:(expanded from "Beep"). 2591:Royal Canadian Institute 2493:Einstein field equations 455:Hamilton–Jacobi–Einstein 435:Einstein field equations 258:Mathematical formulation 3413:Galilean transformation 3404:Principle of relativity 2906:Physical Review Letters 2663:uses the term, as does 2353:simultaneous hyperplane 2138:Simultaneous hyperplane 2113:simultaneous hyperplane 1257:is used informally for 1069:worldline of a particle 3498:Lorentz transformation 2887:10.1103/PhysRev.84.108 2840:10.1103/PhysRev.80.440 2742:Closed timelike curves 2626:work in 2008 entitled 2448: 2333: 2289: 2256: 2221: 2178: 2028: 2015: 1963:η, which gives a 1913: 1880: 1858: 1634: 1602: 1582: 1564:defines a vector, the 1558: 1535: 1506: 1470: 1443: 1423: 1403: 1314: 1293:along the world line. 1287: 1244: 1224: 1197: 1124: 1057: 1037: 886:) of an object is the 325:Gravitational redshift 218: 3966:Weyl−Lewis−Papapetrou 3707:Raychaudhuri equation 3646:Equivalence principle 3316:Macmillan and Company 3278:"Raum und Zeit"  2660:Methuselah's Children 2583:University of Toronto 2449: 2377:orthogonal complement 2334: 2290: 2257: 2222: 2179: 2121:hyperbolic-orthogonal 2072:to the given event). 2021: 2009: 1914: 1881: 1859: 1635: 1603: 1583: 1559: 1536: 1507: 1471: 1444: 1424: 1422:{\displaystyle \tau } 1404: 1304: 1288: 1286:{\displaystyle \tau } 1245: 1243:{\displaystyle \tau } 1225: 1223:{\displaystyle x^{0}} 1198: 1110: 1058: 1038: 955:and was pioneered by 613:Weyl−Lewis−Papapetrou 568:Kerr–Newman–de Sitter 388:Einstein–Rosen bridge 320:Gravitational lensing 276:Equivalence principle 219: 4214:Theory of relativity 4007:Numerical relativity 3848:pulsar timing arrays 3312:Theory of Relativity 3069:; Alvarez, Orlando; 2670:The Quincunx of Time 2395: 2363:is a statement that 2299: 2266: 2231: 2188: 2146: 1890: 1870: 1644: 1640:, or in components: 1615: 1592: 1572: 1545: 1516: 1480: 1453: 1433: 1413: 1346: 1277: 1253:Sometimes, the term 1234: 1207: 1140: 1047: 1027: 916:" (e.g., a planet's 543:Einstein–Rosen waves 269:Fundamental concepts 158: 61:improve this article 4219:Minkowski spacetime 3899:Friedmann equations 3793:Hulse–Taylor binary 3755:Gravitational waves 3651:Riemannian geometry 3477:Proper acceleration 3462:Maxwell's equations 3408:Galilean relativity 3143:2005PhRvD..72j5004D 3089:1982NuPhB.197..509A 3071:Manton, Nicholas S. 3037:2001PhR...355...73S 2988:1996ARNPS..46..109B 2919:1991PhRvL..66.1669B 2879:1951PhRv...84..108F 2854:Feynman, Richard P. 2818:Feynman, Richard P. 2633:In the short story 2600:Slaughterhouse-Five 2461:retarded potentials 2142:Since a world line 903:theoretical physics 901:, and particularly 497:Kaluza–Klein theory 383:Minkowski spacetime 335:Gravitational waves 3948:Reissner–Nordström 3866:Brans–Dicke theory 3697:Linearized gravity 3524:Length contraction 3442:Frame of reference 3419:Special relativity 3308:Ludwik Silberstein 2796:. pp. 62–67. 2641:Robert A. Heinlein 2567:scientific romance 2477:special relativity 2473:general relativity 2444: 2329: 2285: 2252: 2217: 2174: 2029: 2016: 1941:special relativity 1909: 1876: 1854: 1630: 1598: 1578: 1554: 1531: 1502: 1466: 1439: 1419: 1399: 1315: 1283: 1240: 1220: 1193: 1127:A one-dimensional 1125: 1053: 1033: 1003:, together with a 965:general relativity 961:special relativity 942:special relativity 826:Physics portal 598:Oppenheimer–Snyder 538:Reissner–Nordström 430:Linearized gravity 378:Spacetime diagrams 281:Special relativity 214: 143:General relativity 4201: 4200: 4015: 4014: 3994:OzsvĂĄth–SchĂŒcking 3600: 3599: 3582:Minkowski diagram 3539:Thomas precession 3482:Relativistic mass 3241:978-1-906557-00-3 3120:Physical Review D 3076:Nuclear Physics B 2913:(13): 1669–1672. 2690:Science Adventure 2526:comoving observer 2439: 2416: 2215: 1879:{\displaystyle p} 1847: 1816: 1785: 1754: 1656: 1627: 1601:{\displaystyle p} 1581:{\displaystyle p} 1442:{\displaystyle p} 1056:{\displaystyle x} 1036:{\displaystyle t} 1021:Minkowski diagram 1012:coordinate system 983:For example, the 957:Hermann Minkowski 876: 875: 509: 508: 395: 394: 137: 136: 129: 111: 16:(Redirected from 4231: 4193: 4192: 3976:van Stockum dust 3748:Two-body problem 3666:Mach's principle 3613: 3612: 3554:Terrell rotation 3394: 3393: 3372: 3365: 3358: 3349: 3348: 3290: 3280: 3267: 3266: 3264: 3262: 3252: 3246: 3245: 3227: 3221: 3220: 3195: 3189: 3188: 3187:. pp. 1–32. 3169: 3163: 3162: 3136: 3116: 3107: 3101: 3100: 3063: 3057: 3056: 3030: 3008: 3002: 3001: 2999: 2981: 2961: 2945: 2939: 2938: 2897: 2891: 2890: 2862: 2850: 2844: 2843: 2814: 2808: 2807: 2781: 2747:Causal structure 2708:Platonic realism 2453: 2451: 2450: 2445: 2440: 2438: 2430: 2422: 2417: 2415: 2407: 2399: 2355:with respect to 2338: 2336: 2335: 2330: 2294: 2292: 2291: 2286: 2278: 2277: 2261: 2259: 2258: 2253: 2226: 2224: 2223: 2218: 2216: 2214: 2206: 2198: 2183: 2181: 2180: 2175: 2173: 2172: 2010:An example of a 1969:spacetime metric 1918: 1916: 1915: 1910: 1908: 1907: 1885: 1883: 1882: 1877: 1863: 1861: 1860: 1855: 1853: 1849: 1848: 1846: 1838: 1837: 1836: 1823: 1817: 1815: 1807: 1806: 1805: 1792: 1786: 1784: 1776: 1775: 1774: 1761: 1755: 1753: 1745: 1744: 1743: 1730: 1720: 1716: 1715: 1714: 1702: 1701: 1689: 1688: 1676: 1675: 1658: 1657: 1649: 1639: 1637: 1636: 1631: 1629: 1628: 1620: 1607: 1605: 1604: 1599: 1587: 1585: 1584: 1579: 1563: 1561: 1560: 1555: 1540: 1538: 1537: 1532: 1511: 1509: 1508: 1503: 1492: 1491: 1475: 1473: 1472: 1467: 1465: 1464: 1448: 1446: 1445: 1440: 1428: 1426: 1425: 1420: 1408: 1406: 1405: 1400: 1358: 1357: 1292: 1290: 1289: 1284: 1249: 1247: 1246: 1241: 1229: 1227: 1226: 1221: 1219: 1218: 1202: 1200: 1199: 1194: 1152: 1151: 1062: 1060: 1059: 1054: 1042: 1040: 1039: 1034: 971:Usage in physics 936:) more absolute 868: 861: 854: 841: 836: 835: 828: 824: 823: 608:van Stockum dust 593:Robertson–Walker 419: 418: 309: 308: 223: 221: 220: 215: 213: 212: 200: 192: 191: 173: 172: 153: 139: 138: 132: 125: 121: 118: 112: 110: 69: 45: 37: 21: 4239: 4238: 4234: 4233: 4232: 4230: 4229: 4228: 4224:Time in science 4204: 4203: 4202: 4197: 4183: 4011: 3915:BKL singularity 3905:LemaĂźtre–Tolman 3880: 3876:Quantum gravity 3858: 3852: 3838:geodetic effect 3812:(together with 3782:LISA Pathfinder 3721: 3670: 3656:Penrose diagram 3638: 3632: 3607: 3596: 3592:Minkowski space 3558: 3502: 3486: 3434: 3428: 3388: 3381: 3376: 3325: 3271: 3270: 3260: 3258: 3254: 3253: 3249: 3242: 3228: 3224: 3217: 3196: 3192: 3185:S. Sonnenschein 3170: 3166: 3114: 3108: 3104: 3067:Affleck, Ian K. 3064: 3060: 3021:(2–3): 73–234. 3014:Physics Reports 3009: 3005: 2959: 2946: 2942: 2898: 2894: 2866:Physical Review 2860: 2851: 2847: 2827:Physical Review 2815: 2811: 2804: 2782: 2778: 2773: 2760:Feynman diagram 2730: 2700:Neal Stephenson 2624:science fiction 2620:Oliver Franklin 2559: 2546: 2524:curve admits a 2469: 2431: 2423: 2421: 2408: 2400: 2398: 2396: 2393: 2392: 2391:are related by 2300: 2297: 2296: 2273: 2269: 2267: 2264: 2263: 2232: 2229: 2228: 2207: 2199: 2197: 2189: 2186: 2185: 2168: 2164: 2147: 2144: 2143: 2140: 2051:Minkowski space 1988:Minkowski space 1937: 1903: 1899: 1891: 1888: 1887: 1871: 1868: 1867: 1839: 1832: 1828: 1824: 1822: 1808: 1801: 1797: 1793: 1791: 1777: 1770: 1766: 1762: 1760: 1746: 1739: 1735: 1731: 1729: 1728: 1724: 1710: 1706: 1697: 1693: 1684: 1680: 1671: 1667: 1666: 1662: 1648: 1647: 1645: 1642: 1641: 1619: 1618: 1616: 1613: 1612: 1593: 1590: 1589: 1573: 1570: 1569: 1546: 1543: 1542: 1517: 1514: 1513: 1487: 1483: 1481: 1478: 1477: 1460: 1456: 1454: 1451: 1450: 1434: 1431: 1430: 1414: 1411: 1410: 1353: 1349: 1347: 1344: 1343: 1340: 1299: 1278: 1275: 1274: 1235: 1232: 1231: 1214: 1210: 1208: 1205: 1204: 1147: 1143: 1141: 1138: 1137: 1105: 1048: 1045: 1044: 1028: 1025: 1024: 973: 938:position states 872: 831: 818: 817: 810: 809: 633: 632: 623: 622: 578:LemaĂźtre–Tolman 523: 522: 511: 510: 502:Quantum gravity 489:Advanced theory 416: 415: 414: 397: 396: 345:Geodetic effect 306: 305: 296: 295: 271: 270: 254: 224: 205: 201: 196: 184: 180: 165: 161: 159: 156: 155: 133: 122: 116: 113: 70: 68: 58: 46: 35: 28: 23: 22: 15: 12: 11: 5: 4237: 4227: 4226: 4221: 4216: 4199: 4198: 4188: 4185: 4184: 4182: 4181: 4174: 4169: 4164: 4159: 4154: 4149: 4144: 4139: 4134: 4129: 4124: 4119: 4114: 4109: 4104: 4102:Choquet-Bruhat 4099: 4094: 4089: 4084: 4079: 4074: 4069: 4064: 4059: 4054: 4049: 4044: 4039: 4034: 4029: 4023: 4021: 4017: 4016: 4013: 4012: 4010: 4009: 4002: 4001: 3996: 3991: 3984: 3983: 3978: 3973: 3968: 3963: 3954:Axisymmetric: 3951: 3950: 3945: 3939: 3928: 3927: 3922: 3917: 3912: 3907: 3902: 3893:Cosmological: 3890: 3888: 3882: 3881: 3879: 3878: 3873: 3868: 3862: 3860: 3854: 3853: 3851: 3850: 3845: 3834:frame-dragging 3831: 3826: 3821: 3818:Einstein rings 3814:Einstein cross 3807: 3796: 3795: 3790: 3784: 3779: 3774: 3761: 3751: 3750: 3745: 3740: 3735: 3729: 3727: 3723: 3722: 3720: 3719: 3717:Ernst equation 3714: 3709: 3704: 3699: 3694: 3689: 3687:BSSN formalism 3684: 3678: 3676: 3672: 3671: 3669: 3668: 3663: 3658: 3653: 3648: 3642: 3640: 3634: 3633: 3631: 3630: 3625: 3619: 3617: 3610: 3602: 3601: 3598: 3597: 3595: 3594: 3589: 3584: 3579: 3574: 3568: 3566: 3560: 3559: 3557: 3556: 3551: 3546: 3544:Ladder paradox 3541: 3536: 3531: 3526: 3521: 3516: 3510: 3508: 3504: 3503: 3501: 3500: 3494: 3492: 3488: 3487: 3485: 3484: 3479: 3474: 3469: 3464: 3459: 3454: 3449: 3447:Speed of light 3444: 3438: 3436: 3430: 3429: 3427: 3426: 3421: 3416: 3410: 3400: 3398: 3391: 3383: 3382: 3375: 3374: 3367: 3360: 3352: 3346: 3345: 3337: 3336: 3324: 3323:External links 3321: 3320: 3319: 3304: 3303: 3302: 3301: 3299:Space and Time 3292: 3291: 3269: 3268: 3247: 3240: 3234:. Epic Press. 3222: 3215: 3209:. p. 19. 3190: 3164: 3134:hep-th/0507174 3127:(10): 105004. 3102: 3083:(3): 509–519. 3058: 3028:hep-th/0101036 3003: 2979:hep-ph/9602280 2940: 2892: 2873:(3): 440–457. 2845: 2834:(1): 108–128. 2809: 2802: 2794:Academic Press 2775: 2774: 2772: 2769: 2768: 2767: 2765:Time geography 2762: 2757: 2756: 2755: 2753:Isotropic line 2750: 2744: 2739: 2729: 2726: 2722:Charles Stross 2684:, produced by 2655: 2654: 2650: 2649: 2609: 2608: 2595: 2594: 2575: 2574: 2558: 2555: 2545: 2542: 2468: 2465: 2443: 2437: 2434: 2429: 2426: 2420: 2414: 2411: 2406: 2403: 2351:is called the 2328: 2325: 2322: 2319: 2316: 2313: 2310: 2307: 2304: 2284: 2281: 2276: 2272: 2251: 2248: 2245: 2242: 2239: 2236: 2213: 2210: 2205: 2202: 2196: 2193: 2171: 2167: 2163: 2160: 2157: 2154: 2151: 2139: 2136: 2135: 2134: 2133: 2132: 2125: 2086: 2085: 2084: 2062: 2047: 2046: 2040: 2004: 2003: 1957:speed of light 1947:is limited to 1936: 1933: 1906: 1902: 1898: 1895: 1875: 1852: 1845: 1842: 1835: 1831: 1827: 1821: 1814: 1811: 1804: 1800: 1796: 1790: 1783: 1780: 1773: 1769: 1765: 1759: 1752: 1749: 1742: 1738: 1734: 1727: 1723: 1719: 1713: 1709: 1705: 1700: 1696: 1692: 1687: 1683: 1679: 1674: 1670: 1665: 1661: 1655: 1652: 1626: 1623: 1597: 1577: 1566:tangent vector 1553: 1550: 1530: 1527: 1524: 1521: 1501: 1498: 1495: 1490: 1486: 1463: 1459: 1438: 1418: 1398: 1395: 1392: 1389: 1386: 1383: 1380: 1377: 1374: 1370: 1367: 1364: 1361: 1356: 1352: 1339: 1336: 1298: 1295: 1282: 1267:(time) history 1239: 1217: 1213: 1192: 1189: 1186: 1183: 1180: 1177: 1174: 1171: 1168: 1164: 1161: 1158: 1155: 1150: 1146: 1104: 1101: 1085: 1084: 1052: 1032: 972: 969: 948:interactions. 918:orbit in space 874: 873: 871: 870: 863: 856: 848: 845: 844: 843: 842: 829: 812: 811: 808: 807: 800: 795: 790: 785: 780: 775: 770: 765: 760: 755: 750: 745: 740: 735: 730: 725: 720: 715: 710: 705: 700: 695: 690: 685: 680: 675: 670: 665: 660: 655: 650: 645: 640: 634: 630: 629: 628: 625: 624: 621: 620: 615: 610: 605: 600: 595: 590: 585: 580: 575: 570: 565: 560: 555: 550: 545: 540: 535: 524: 518: 517: 516: 513: 512: 507: 506: 505: 504: 499: 491: 490: 486: 485: 484: 483: 481:Post-Newtonian 478: 473: 465: 464: 460: 459: 458: 457: 452: 447: 442: 437: 432: 424: 423: 417: 413: 412: 409: 405: 404: 403: 402: 399: 398: 393: 392: 391: 390: 385: 380: 372: 371: 365: 364: 363: 362: 357: 352: 347: 342: 340:Frame-dragging 337: 332: 327: 322: 317: 315:Kepler problem 307: 303: 302: 301: 298: 297: 294: 293: 288: 283: 278: 272: 268: 267: 266: 263: 262: 261: 260: 255: 253: 252: 247: 242: 236: 234: 226: 225: 211: 208: 204: 199: 195: 190: 187: 183: 179: 176: 171: 168: 164: 154: 146: 145: 135: 134: 49: 47: 40: 26: 9: 6: 4: 3: 2: 4236: 4225: 4222: 4220: 4217: 4215: 4212: 4211: 4209: 4196: 4186: 4180: 4179: 4175: 4173: 4170: 4168: 4165: 4163: 4160: 4158: 4155: 4153: 4150: 4148: 4145: 4143: 4140: 4138: 4135: 4133: 4130: 4128: 4125: 4123: 4120: 4118: 4115: 4113: 4110: 4108: 4105: 4103: 4100: 4098: 4095: 4093: 4090: 4088: 4087:Chandrasekhar 4085: 4083: 4080: 4078: 4075: 4073: 4070: 4068: 4065: 4063: 4060: 4058: 4055: 4053: 4050: 4048: 4047:Schwarzschild 4045: 4043: 4040: 4038: 4035: 4033: 4030: 4028: 4025: 4024: 4022: 4018: 4008: 4004: 4003: 4000: 3997: 3995: 3992: 3990: 3986: 3985: 3982: 3979: 3977: 3974: 3972: 3969: 3967: 3964: 3961: 3957: 3953: 3952: 3949: 3946: 3943: 3940: 3938: 3934: 3933:Schwarzschild 3930: 3929: 3926: 3923: 3921: 3918: 3916: 3913: 3911: 3908: 3906: 3903: 3900: 3896: 3892: 3891: 3889: 3887: 3883: 3877: 3874: 3872: 3869: 3867: 3864: 3863: 3861: 3855: 3849: 3846: 3843: 3839: 3835: 3832: 3830: 3829:Shapiro delay 3827: 3825: 3822: 3819: 3815: 3811: 3808: 3805: 3801: 3798: 3797: 3794: 3791: 3788: 3785: 3783: 3780: 3778: 3775: 3773: 3772:collaboration 3769: 3765: 3762: 3760: 3756: 3753: 3752: 3749: 3746: 3744: 3741: 3739: 3738:Event horizon 3736: 3734: 3731: 3730: 3728: 3724: 3718: 3715: 3713: 3710: 3708: 3705: 3703: 3700: 3698: 3695: 3693: 3690: 3688: 3685: 3683: 3682:ADM formalism 3680: 3679: 3677: 3673: 3667: 3664: 3662: 3659: 3657: 3654: 3652: 3649: 3647: 3644: 3643: 3641: 3635: 3629: 3626: 3624: 3621: 3620: 3618: 3614: 3611: 3609: 3603: 3593: 3590: 3588: 3587:Biquaternions 3585: 3583: 3580: 3578: 3575: 3573: 3570: 3569: 3567: 3565: 3561: 3555: 3552: 3550: 3547: 3545: 3542: 3540: 3537: 3535: 3532: 3530: 3527: 3525: 3522: 3520: 3517: 3515: 3514:Time dilation 3512: 3511: 3509: 3505: 3499: 3496: 3495: 3493: 3489: 3483: 3480: 3478: 3475: 3473: 3470: 3468: 3467:Proper length 3465: 3463: 3460: 3458: 3455: 3453: 3450: 3448: 3445: 3443: 3440: 3439: 3437: 3431: 3425: 3422: 3420: 3417: 3414: 3411: 3409: 3405: 3402: 3401: 3399: 3395: 3392: 3390: 3384: 3380: 3373: 3368: 3366: 3361: 3359: 3354: 3353: 3350: 3344: 3341: 3340: 3339: 3334: 3330: 3327: 3326: 3317: 3313: 3309: 3306: 3305: 3300: 3296: 3295: 3294: 3293: 3288: 3284: 3279: 3273: 3272: 3257: 3251: 3243: 3237: 3233: 3226: 3218: 3216:0-7727-1600-5 3212: 3208: 3204: 3200: 3194: 3186: 3182: 3178: 3174: 3173:Hinton, C. H. 3168: 3160: 3156: 3152: 3148: 3144: 3140: 3135: 3130: 3126: 3122: 3121: 3113: 3106: 3098: 3094: 3090: 3086: 3082: 3078: 3077: 3072: 3068: 3062: 3054: 3050: 3046: 3042: 3038: 3034: 3029: 3024: 3020: 3016: 3015: 3007: 2998: 2993: 2989: 2985: 2980: 2975: 2971: 2967: 2966: 2958: 2954: 2950: 2944: 2936: 2932: 2928: 2924: 2920: 2916: 2912: 2908: 2907: 2902: 2896: 2888: 2884: 2880: 2876: 2872: 2868: 2867: 2859: 2855: 2849: 2841: 2837: 2833: 2829: 2828: 2823: 2819: 2813: 2805: 2803:9780080918631 2799: 2795: 2791: 2787: 2780: 2776: 2766: 2763: 2761: 2758: 2754: 2751: 2748: 2745: 2743: 2740: 2738: 2735: 2734: 2732: 2731: 2725: 2723: 2718: 2715: 2713: 2709: 2705: 2701: 2697: 2695: 2691: 2687: 2683: 2679: 2674: 2672: 2671: 2666: 2662: 2661: 2652: 2651: 2646: 2645: 2644: 2642: 2638: 2637: 2631: 2629: 2625: 2621: 2616: 2614: 2606: 2605: 2604: 2602: 2601: 2592: 2588: 2587: 2586: 2584: 2580: 2572: 2571: 2570: 2568: 2564: 2554: 2552: 2541: 2539: 2534: 2532: 2527: 2523: 2519: 2514: 2510: 2506: 2502: 2498: 2494: 2490: 2486: 2482: 2478: 2474: 2464: 2462: 2458: 2457:Coulomb's law 2441: 2435: 2432: 2427: 2424: 2418: 2412: 2409: 2404: 2401: 2390: 2386: 2382: 2378: 2374: 2370: 2366: 2362: 2358: 2354: 2350: 2346: 2342: 2326: 2320: 2317: 2314: 2308: 2302: 2282: 2274: 2270: 2246: 2243: 2240: 2234: 2211: 2208: 2203: 2200: 2194: 2191: 2169: 2165: 2161: 2155: 2149: 2130: 2126: 2122: 2118: 2114: 2110: 2109: 2107: 2103: 2099: 2094: 2090: 2087: 2082: 2078: 2074: 2073: 2071: 2067: 2063: 2060: 2056: 2055: 2054: 2052: 2044: 2041: 2038: 2034: 2031: 2030: 2026: 2020: 2013: 2008: 2000: 1997: 1996: 1995: 1991: 1989: 1985: 1980: 1978: 1974: 1973:metric spaces 1970: 1966: 1962: 1961:bilinear form 1958: 1954: 1950: 1946: 1942: 1932: 1930: 1929:tangent space 1927:, termed the 1926: 1920: 1904: 1900: 1896: 1893: 1873: 1864: 1850: 1843: 1840: 1833: 1829: 1825: 1819: 1812: 1809: 1802: 1798: 1794: 1788: 1781: 1778: 1771: 1767: 1763: 1757: 1750: 1747: 1740: 1736: 1732: 1725: 1721: 1717: 1711: 1707: 1703: 1698: 1694: 1690: 1685: 1681: 1677: 1672: 1668: 1663: 1659: 1650: 1621: 1611: 1610:four-velocity 1595: 1575: 1567: 1551: 1528: 1522: 1499: 1493: 1488: 1484: 1461: 1457: 1436: 1416: 1396: 1393: 1390: 1387: 1384: 1381: 1378: 1375: 1372: 1368: 1362: 1354: 1350: 1335: 1331: 1328: 1323: 1319: 1312: 1308: 1303: 1294: 1280: 1272: 1268: 1264: 1260: 1256: 1251: 1237: 1215: 1211: 1190: 1187: 1184: 1181: 1178: 1175: 1172: 1169: 1166: 1162: 1156: 1148: 1144: 1134: 1130: 1122: 1118: 1114: 1109: 1100: 1098: 1093: 1090: 1082: 1078: 1074: 1070: 1066: 1065: 1064: 1050: 1030: 1022: 1018: 1013: 1010: 1006: 1002: 997: 995: 991: 986: 981: 978: 968: 966: 962: 958: 954: 949: 947: 946:gravitational 943: 939: 935: 931: 927: 923: 919: 915: 911: 906: 904: 900: 896: 893: 889: 885: 881: 869: 864: 862: 857: 855: 850: 849: 847: 846: 840: 830: 827: 822: 816: 815: 814: 813: 806: 805: 801: 799: 796: 794: 791: 789: 786: 784: 781: 779: 776: 774: 771: 769: 766: 764: 761: 759: 756: 754: 751: 749: 746: 744: 743:Chandrasekhar 741: 739: 736: 734: 731: 729: 726: 724: 721: 719: 716: 714: 711: 709: 706: 704: 701: 699: 696: 694: 691: 689: 686: 684: 681: 679: 676: 674: 671: 669: 666: 664: 661: 659: 658:Schwarzschild 656: 654: 651: 649: 646: 644: 641: 639: 636: 635: 627: 626: 619: 618:Hartle–Thorne 616: 614: 611: 609: 606: 604: 601: 599: 596: 594: 591: 589: 586: 584: 581: 579: 576: 574: 571: 569: 566: 564: 561: 559: 556: 554: 551: 549: 546: 544: 541: 539: 536: 533: 529: 528:Schwarzschild 526: 525: 521: 515: 514: 503: 500: 498: 495: 494: 493: 492: 488: 487: 482: 479: 477: 474: 472: 469: 468: 467: 466: 462: 461: 456: 453: 451: 448: 446: 443: 441: 438: 436: 433: 431: 428: 427: 426: 425: 421: 420: 410: 407: 406: 401: 400: 389: 386: 384: 381: 379: 376: 375: 374: 373: 370: 367: 366: 361: 358: 356: 353: 351: 350:Event horizon 348: 346: 343: 341: 338: 336: 333: 331: 328: 326: 323: 321: 318: 316: 313: 312: 311: 310: 300: 299: 292: 289: 287: 284: 282: 279: 277: 274: 273: 265: 264: 259: 256: 251: 248: 246: 243: 241: 238: 237: 235: 233: 230: 229: 228: 227: 209: 206: 202: 197: 193: 188: 185: 181: 174: 169: 166: 162: 152: 148: 147: 144: 141: 140: 131: 128: 120: 117:November 2023 109: 106: 102: 99: 95: 92: 88: 85: 81: 78: â€“  77: 73: 72:Find sources: 66: 62: 56: 55: 50:This article 48: 44: 39: 38: 33: 19: 4177: 3871:Kaluza–Klein 3623:Introduction 3576: 3549:Twin paradox 3338: 3311: 3286: 3282: 3259:. Retrieved 3250: 3231: 3225: 3202: 3193: 3180: 3167: 3124: 3118: 3105: 3080: 3074: 3061: 3018: 3012: 3006: 2969: 2963: 2953:Dixon, Lance 2943: 2910: 2904: 2895: 2870: 2864: 2848: 2831: 2825: 2812: 2789: 2779: 2719: 2716: 2698: 2678:visual novel 2675: 2668: 2658: 2656: 2634: 2632: 2627: 2622:published a 2617: 2610: 2598: 2596: 2579:J. C. Fields 2576: 2563:C. H. Hinton 2560: 2547: 2535: 2470: 2388: 2384: 2380: 2372: 2368: 2364: 2356: 2352: 2348: 2340: 2141: 2128: 2112: 2105: 2101: 2092: 2088: 2076: 2065: 2058: 2048: 2042: 2036: 2032: 1998: 1992: 1981: 1976: 1968: 1948: 1938: 1925:linear space 1921: 1865: 1565: 1341: 1332: 1326: 1324: 1320: 1316: 1310: 1309:is time and 1306: 1266: 1262: 1258: 1254: 1252: 1132: 1128: 1126: 1096: 1094: 1086: 1076: 1068: 998: 989: 984: 982: 974: 950: 930:perceptually 925: 921: 917: 907: 883: 879: 877: 803: 763:Raychaudhuri 285: 232:Introduction 123: 114: 104: 97: 90: 83: 76:"World line" 71: 59:Please help 54:verification 51: 32:Worldline SA 3960:Kerr–Newman 3931:Spherical: 3800:Other tests 3743:Singularity 3675:Formulation 3637:Fundamental 3491:Formulation 3472:Proper time 3433:Fundamental 3331:article on 3329:World lines 3261:8 September 3232:World Lines 2972:: 109–148. 2682:Steins;Gate 2665:James Blish 2657:Heinlein's 2628:World Lines 2613:time travel 2569:. He wrote 2367:depends on 2002:suppressed. 1965:real number 1271:proper time 1089:world sheet 1077:proper time 1073:proper time 892:dimensional 778:van Stockum 708:Oppenheimer 563:Kerr–Newman 355:Singularity 4208:Categories 4112:Zel'dovich 4020:Scientists 3999:Alcubierre 3806:of Mercury 3804:precession 3733:Black hole 3616:Background 3608:relativity 3577:World line 3572:Light cone 3397:Background 3389:relativity 3379:Relativity 2771:References 2712:nominalism 2371:. Indeed, 2345:null space 2081:light cone 2070:light cone 2043:space-like 2012:light cone 1999:light-like 1263:world line 1255:world line 1097:world line 1005:continuous 990:world line 953:physicists 934:relatively 922:trajectory 914:trajectory 880:world line 631:Scientists 463:Formalisms 411:Formalisms 360:Black hole 286:World line 87:newspapers 4082:Robertson 4067:Friedmann 4062:Eddington 4052:de Sitter 3886:Solutions 3764:detectors 3759:astronomy 3726:Phenomena 3661:Geodesics 3564:Spacetime 3507:Phenomena 3314:, p 130, 3159:119357180 3053:118891361 2949:Bern, Zvi 2901:Bern, Zvi 2737:Geodesics 2702:'s novel 2694:Dirac Sea 2639:, author 2636:Life-Line 2538:geodesics 2501:spacelike 2497:lightlike 2481:spacetime 2436:τ 2413:τ 2309:η 2306:↦ 2280:→ 2235:η 2212:τ 2162:∈ 2156:τ 2106:elsewhere 2093:elsewhere 2089:Elsewhere 2077:lightcone 2033:time-like 2025:spacetime 1984:geodesics 1945:spacetime 1901:τ 1894:τ 1844:τ 1813:τ 1782:τ 1751:τ 1654:→ 1625:→ 1552:τ 1549:Δ 1526:→ 1523:τ 1520:Δ 1500:τ 1497:Δ 1485:τ 1458:τ 1417:τ 1363:τ 1327:collision 1313:distance. 1281:τ 1238:τ 1157:τ 1113:particles 1081:free fall 977:spacetime 895:spacetime 884:worldline 723:Robertson 688:Friedmann 683:Eddington 673:Nordström 663:de Sitter 520:Solutions 445:Geodesics 440:Friedmann 422:Equations 408:Equations 369:Spacetime 304:Phenomena 210:ν 207:μ 198:κ 189:ν 186:μ 178:Λ 170:ν 167:μ 18:Worldline 4195:Category 4072:LemaĂźtre 4037:Einstein 4027:PoincarĂ© 3987:Others: 3971:Taub–NUT 3937:interior 3859:theories 3857:Advanced 3824:redshift 3639:concepts 3457:Rapidity 3435:concepts 3201:(1979). 3175:(1884). 2935:10043277 2856:(1951). 2820:(1950). 2728:See also 2561:In 1884 2522:timelike 2513:timelike 2509:timelike 2505:timelike 2499:(null), 2119:that is 1886:, so at 1017:manifold 912:" or a " 839:Category 703:LemaĂźtre 668:Reissner 653:PoincarĂ© 638:Einstein 583:Taub–NUT 548:Wormhole 532:interior 245:Timeline 4137:Hawking 4132:Penrose 4117:Novikov 4097:Wheeler 4042:Hilbert 4032:Lorentz 3989:pp-wave 3810:lensing 3606:General 3387:Special 3310:(1914) 3289:: 75–88 3139:Bibcode 3085:Bibcode 3033:Bibcode 2984:Bibcode 2915:Bibcode 2875:Bibcode 2704:Anathem 2618:Author 2581:at the 2483:can be 2375:is the 2343:be the 2129:present 2102:present 1949:special 1203:(where 1117:strings 994:helical 920:or the 899:physics 758:Hawking 753:Penrose 728:Bardeen 718:Wheeler 648:Hilbert 643:Lorentz 603:pp-wave 240:History 101:scholar 4178:others 4167:Thorne 4157:Misner 4142:Taylor 4127:Geroch 4122:Ehlers 4092:Zwicky 3910:Kasner 3238:  3213:  3157:  3051:  2933:  2800:  2680:named 2503:, and 2489:metric 2485:curved 2359:. The 2059:future 1121:branes 1119:, and 1009:smooth 1001:events 837:  804:others 798:Thorne 788:Newman 768:Taylor 748:Ehlers 733:Walker 698:Zwicky 573:Kasner 103:  96:  89:  82:  74:  4172:Weiss 4152:Bondi 4147:Hulse 4077:Milne 3981:discs 3925:Milne 3920:Gödel 3777:Virgo 3155:S2CID 3129:arXiv 3115:(PDF) 3049:S2CID 3023:arXiv 2974:arXiv 2960:(PDF) 2861:(PDF) 2339:Let 2117:space 1133:curve 985:orbit 910:orbit 773:Hulse 713:Gödel 693:Milne 588:Milne 553:Gödel 250:Tests 108:JSTOR 94:books 4107:Kerr 4057:Weyl 3956:Kerr 3816:and 3770:and 3768:LIGO 3333:h2g2 3263:2010 3236:ISBN 3211:ISBN 2931:PMID 2798:ISBN 2710:and 2686:5pb. 2487:. A 2387:and 2127:The 2075:The 2066:past 2064:The 2057:The 1129:line 1007:and 963:and 926:time 888:path 882:(or 878:The 783:Taub 738:Kerr 678:Weyl 558:Kerr 476:BSSN 80:news 4162:Yau 3787:GEO 3147:doi 3093:doi 3081:197 3041:doi 3019:355 2992:doi 2923:doi 2883:doi 2836:doi 2667:'s 2379:of 2295:by 2098:Sun 1977:not 1259:any 1131:or 967:). 944:or 793:Yau 471:ADM 63:by 4210:: 3836:/ 3802:: 3757:: 3287:10 3285:, 3281:, 3205:. 3183:. 3179:. 3153:. 3145:. 3137:. 3125:72 3123:. 3117:. 3091:. 3079:. 3047:. 3039:. 3031:. 3017:. 2990:. 2982:. 2970:46 2968:. 2962:. 2951:; 2929:. 2921:. 2911:66 2909:. 2881:. 2871:84 2869:. 2863:. 2832:80 2830:. 2824:. 2792:. 2788:. 2724:. 2714:. 2676:A 2540:. 2533:. 2463:. 1990:. 1919:. 1115:, 905:. 3962:) 3958:( 3944:) 3935:( 3901:) 3897:( 3844:) 3840:( 3820:) 3789:) 3766:( 3415:) 3406:( 3371:e 3364:t 3357:v 3335:. 3318:. 3265:. 3244:. 3219:. 3161:. 3149:: 3141:: 3131:: 3099:. 3095:: 3087:: 3055:. 3043:: 3035:: 3025:: 3000:. 2994:: 2986:: 2976:: 2937:. 2925:: 2917:: 2889:. 2885:: 2877:: 2842:. 2838:: 2806:. 2516:( 2442:, 2433:d 2428:w 2425:d 2419:= 2410:d 2405:u 2402:d 2389:w 2385:u 2381:v 2373:N 2369:v 2365:N 2357:v 2349:N 2341:N 2327:. 2324:) 2321:x 2318:, 2315:v 2312:( 2303:x 2283:R 2275:4 2271:R 2250:) 2247:x 2244:, 2241:v 2238:( 2209:d 2204:w 2201:d 2195:= 2192:v 2170:4 2166:R 2159:) 2153:( 2150:w 2039:. 1905:0 1897:= 1874:p 1851:) 1841:d 1834:3 1830:x 1826:d 1820:, 1810:d 1803:2 1799:x 1795:d 1789:, 1779:d 1772:1 1768:x 1764:d 1758:, 1748:d 1741:0 1737:x 1733:d 1726:( 1722:= 1718:) 1712:3 1708:v 1704:, 1699:2 1695:v 1691:, 1686:1 1682:v 1678:, 1673:0 1669:v 1664:( 1660:= 1651:v 1622:v 1596:p 1576:p 1529:0 1494:+ 1489:0 1462:0 1437:p 1397:3 1394:, 1391:2 1388:, 1385:1 1382:, 1379:0 1376:= 1373:a 1369:, 1366:) 1360:( 1355:a 1351:x 1311:x 1307:t 1216:0 1212:x 1191:3 1188:, 1185:2 1182:, 1179:1 1176:, 1173:0 1170:= 1167:a 1163:, 1160:) 1154:( 1149:a 1145:x 1123:. 1083:. 1051:x 1031:t 867:e 860:t 853:v 534:) 530:( 203:T 194:= 182:g 175:+ 163:G 130:) 124:( 119:) 115:( 105:· 98:· 91:· 84:· 57:. 34:. 20:)

Index

Worldline
Worldline SA

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General relativity
Spacetime curvature schematic
Introduction
History
Timeline
Tests
Mathematical formulation
Equivalence principle
Special relativity
World line
Pseudo-Riemannian manifold
Kepler problem
Gravitational lensing
Gravitational redshift
Gravitational time dilation
Gravitational waves
Frame-dragging

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