**弦論**是將結合量子力學和廣義相對論成萬有理論的理論物理學。

弦論已得到數十年的深入研究，在歷史上出現了兩次超弦革命。在眾多研究人員共同努力下，弦理論早已與量子引力、粒子物理和凝聚態物理、宇宙學和純數學融匯貫通，發展成了一個廣泛多樣的學科。

S矩陣理論
-----

維爾納·海森堡1943年一項研究計劃說弦理論是S-矩陣理論的產物。

約翰·惠勒于1937年引入S矩阵后，從1950年後期到60年代，許多著名的理論家都接受並提倡。但該領域在70年代中期被邊緣化並被丟棄 並在80年代被量子色動力學取代了。

1943年，维尔纳·海森堡提出了S矩阵理论作为粒子相互作用的原理。

已隱藏部分未翻譯内容，歡迎參與翻譯。
The theory presented a radical rethinking of the foundations of physical laws. By the 1940s it had become clear that the proton and the neutron were not pointlike particles like the electron. Their magnetic moment differed greatly from that of a pointlike spin-½ charged particle, too much to attribute the difference to a small perturbation. Their interactions were so strong that they scattered like a small sphere, not like a point. Heisenberg proposed that the strongly interacting particles were in fact extended objects, and because there are difficulties of principle with extended relativistic particles, he proposed that the notion of a space-time point broke down at nuclear scales.

Without space and time, it becomes difficult to formulate a physical theory. Heisenberg proposed a solution to this problem: focusing on the observable quantities—those things measurable by experiments. An experiment only sees a microscopic quantity if it can be transferred by a series of events to the classical devices that surround the experimental chamber. The objects that fly to infinity are stable particles, in quantum superpositions of different momentum states.

Heisenberg proposed that even when space and time are unreliable, the notion of momentum state, which is defined far away from the experimental chamber, still works. The physical quantity he proposed as fundamental is the quantum mechanical  amplitude for a group of incoming particles to turn into a group of outgoing particles, and he did not admit that there were any steps in between.

The S-matrix is the quantity that describes how a collection of incoming particles turn into outgoing ones. Heisenberg proposed to study the S-matrix directly, without any assumptions about space-time structure. But when transitions from the far-past to the far-future occur in one step with no intermediate steps, it becomes difficult to calculate anything. In quantum field theory, the intermediate steps are the fluctuations of fields or equivalently the fluctuations of virtual particles. In this proposed S-matrix theory, there are no local quantities at all.

Heisenberg proposed to use unitarity to determine the S-matrix. In all conceivable situations, the sum of the squares of the amplitudes must equal 1. This property can determine the amplitude in a quantum field theory order by order in a perturbation series once the basic interactions are given, and in many quantum field theories the amplitudes grow too fast at high energies to make a unitary S-matrix. But without extra assumptions on the high-energy behavior, unitarity is not enough to determine the scattering, and the proposal was ignored for many years.

Heisenberg's proposal was revived in 1956 when Murray Gell-Mann recognized that dispersion relations—like those discovered by Hendrik Kramers and Ralph Kronig in the 1920s (see Kramers–Kronig relations)—allow the formulation of a notion of causality, a notion that events in the future would not influence events in the past, even when the microscopic notion of past and future are not clearly defined. He also recognized that these relations might be useful in computing observables for the case of strong interaction physics. The dispersion relations were analytic properties of the S-matrix, and they imposed more stringent conditions than those that follow from unitarity alone. This development in S-matrix theory stemmed from Murray Gell-Mann and Marvin Leonard Goldberger's (1954) discovery of crossing symmetry, another condition that the S-matrix had to fulfil.

Prominent advocates of the new "dispersion relations" approach included Stanley Mandelstam and Geoffrey Chew, both at UC Berkeley at the time. Mandelstam discovered the double dispersion relations, a new and powerful analytic form, in 1958, and believed that it would provide the key to progress in the intractable strong interactions.

雷格理論
----

1950年代後期，不同人各自發現了存在許多自旋更高的強相互作用粒子，這很明顯非基本粒子。

已隱藏部分未翻譯内容，歡迎參與翻譯。
By the late 1950s, many strongly interacting particles of ever higher spins had been discovered, and it became clear that they were not all fundamental. While Japanese physicist Shoichi Sakata proposed that the particles could be understood as bound states of just three of them (the proton, the neutron and the Lambda; see Sakata model), Geoffrey Chew believed that none of these particles are fundamental (for details, see Bootstrap model). Sakata's approach was reworked in the 1960s into the quark model by Murray Gell-Mann and George Zweig by making the charges of the hypothetical constituents fractional and rejecting the idea that they were observed particles. At the time, Chew's approach was considered more mainstream because it did not introduce fractional charge values and because it focused on experimentally measurable S-matrix elements, not on hypothetical pointlike constituents.

In 1959, Tullio Regge, a young theorist in Italy, discovered that bound states in quantum mechanics can be organized into families known as Regge trajectories, each family having distinctive angular momenta. This idea was generalized to relativistic quantum mechanics by Stanley Mandelstam, Vladimir Gribov and Marcel Froissart​（法语）, using a mathematical method (the Sommerfeld–Watson representation) discovered decades earlier by Arnold Sommerfeld and Kenneth Marshall Watson​（德语）: the result was dubbed the Froissart–Gribov formula.

In 1961, Geoffrey Chew and Steven Frautschi recognized that mesons had straight line Regge trajectories (in their scheme, spin is plotted against mass squared on a so-called Chew–Frautschi plot), which implied that the scattering of these particles would have very strange behavior—it should fall off exponentially quickly at large angles. With this realization, theorists hoped to construct a theory of composite particles on Regge trajectories, whose scattering amplitudes had the asymptotic form demanded by Regge theory.

In 1967, a notable step forward in the bootstrap approach was the principle of DHS duality introduced by Richard Dolen, David Horn, and Christoph Schmid in 1967, at Caltech (the original term for it was "average duality" or "finite energy sum rule (FESR) duality"). The three researchers noticed that Regge pole exchange (at high energy) and resonance (at low energy) descriptions offer multiple representations/approximations of one and the same physically observable process.

雙共振模型
-----

由加布里埃萊·韋內齊亞諾意大利弦論先驅於1968年建構。

已隱藏部分未翻譯内容，歡迎參與翻譯。
The first model in which hadronic particles essentially follow the Regge trajectories was the dual resonance model that was constructed by Gabriele Veneziano in 1968, who noted that the Euler beta function could be used to describe 4-particle scattering amplitude data for such particles. The Veneziano scattering amplitude (or Veneziano model) was quickly generalized to an *N*-particle amplitude by Ziro Koba and Holger Bech Nielsen (their approach was dubbed the Koba–Nielsen formalism), and to what are now recognized as closed strings by Miguel Virasoro and Joel A. Shapiro (their approach was dubbed the Shapiro–Virasoro model).

In 1969, the Chan–Paton rules (proposed by Jack E. Paton and Hong-Mo Chan) enabled isospin factors to be added to the Veneziano model.

In 1969–70, Yoichiro Nambu, Holger Bech Nielsen, and Leonard Susskind presented a physical interpretation of the Veneziano amplitude by representing nuclear forces as vibrating, one-dimensional strings. However, this string-based description of the strong force made many predictions that directly contradicted experimental findings.

In 1971, Pierre Ramond and, independently, John H. Schwarz and André Neveu attempted to implement fermions into the dual model. This led to the concept of "spinning strings", and pointed the way to a method for removing the problematic tachyon (see RNS formalism).

Dual resonance models for strong interactions were a relatively popular subject of study between 1968 and 1973. The scientific community lost interest in string theory as a theory of strong interactions in 1973 when quantum chromodynamics became the main focus of theoretical research (mainly due to the theoretical appeal of its asymptotic freedom).

玻色弦理論和超弦理論
----------

### 玻色弦理論

1974年，約翰·席瓦茲和若埃爾·捨克、米谷民明先驅建構。

他們研究了玻色子弦振動，發現特性與引力子匹配。這導致了玻色子弦理論的發展。

弦理論是根據泊里雅科夫作用量描述弦如何在空間和時間中移動。像彈簧一樣，弦往往會收縮以最小化其勢能，但能量守恆會阻止它們消失而振盪。通過將量子力學應用於弦，可以推斷出弦不同振動模式，每個振動狀態又皆是不同粒子。每粒粒子的質量，以及相互作用的方式，都是由弦的振動方式決定。

已隱藏部分未翻譯内容，歡迎參與翻譯。
in essence, by the "note" the string "sounds." The scale of notes, each corresponding to a different kind of particle, is termed the "spectrum" of the theory.

Early models included both *open* strings, which have two distinct endpoints, and *closed* strings, where the endpoints are joined to make a complete loop. The two types of string behave in slightly different ways, yielding two spectra. Not all modern string theories use both types; some incorporate only the closed variety.

The earliest string model has several problems: it has a critical dimension *D* = 26, a feature that was originally discovered by Claud Lovelace in 1971; the theory has a fundamental instability, the presence of tachyons (see tachyon condensation); additionally, the spectrum of particles contains only bosons, particles like the photon that obey particular rules of behavior. While bosons are a critical ingredient of the Universe, they are not its only constituents. Investigating how a string theory may include fermions in its spectrum led to the invention of supersymmetry (in the West) in 1971, a mathematical transformation between bosons and fermions. String theories that include fermionic vibrations are now known as superstring theories.

In 1977, the GSO projection (named after Ferdinando Gliozzi, Joël Scherk, and David I. Olive) led to a family of tachyon-free unitary free string theories, the first consistent superstring theories (see below).

第一次超弦革命
-------

已隱藏部分未翻譯内容，歡迎參與翻譯。
The **first superstring revolution** is a period of important discoveries that began in 1984. It was realized that string theory was capable of describing all elementary particles as well as the interactions between them. Hundreds of physicists started to work on string theory as the most promising idea to unify physical theories. The revolution was started by a discovery of anomaly cancellation in type I string theory via the Green–Schwarz mechanism (named after Michael Green and John H. Schwarz) in 1984. The ground-breaking discovery of the heterotic string was made by David Gross, Jeffrey Harvey, Emil Martinec, and Ryan Rohm in 1985. It was also realized by Philip Candelas, Gary Horowitz, Andrew Strominger, and Edward Witten in 1985 that to obtain {\displaystyle N=1} supersymmetry, the six small extra dimensions (the *D* = 10 critical dimension of superstring theory had been originally discovered by John H. Schwarz in 1972) need to be compactified on a Calabi–Yau manifold. (In string theory, compactification is a generalization of Kaluza–Klein theory, which was first proposed in the 1920s.)

By 1985, five separate superstring theories had been described: type I, type II (IIA and IIB), and heterotic (SO(32) and *E*8×*E*8).

*Discover* magazine in the November 1986 issue (vol. 7, #11) featured a cover story written by Gary Taubes, "Everything's Now Tied to Strings", which explained string theory for a popular audience.

In 1987, Eric Bergshoeff​（德语）, Ergin Sezgin​（德语） and Paul Townsend showed that there are no superstrings in eleven dimensions (the largest number of dimensions consistent with a single graviton in supergravity theories), but supermembranes.

第二次超弦革命
-------

1990年代，受對偶性的啓發，愛德華·維頓造了個11維的M理論，把5種版本的10維超弦理論與11維超重力論推演成M理論的6個形。這些發現帶動了第二次超弦革命有數百篇論文出現。

已隱藏部分未翻譯内容，歡迎參與翻譯。
In the early 1990s, Edward Witten and others found strong evidence that the different superstring theories were different limits of an 11-dimensional theory that became known as M-theory (for details, see Introduction to M-theory). These discoveries sparked the **second superstring revolution** that took place approximately between 1994 and 1995.

The different versions of superstring theory were unified, as long hoped, by new equivalences. These are known as S-duality, T-duality, U-duality, mirror symmetry, and conifold transitions. The different theories of strings were also related to M-theory.

In 1995, Joseph Polchinski discovered that the theory requires the inclusion of higher-dimensional objects, called D-branes: these are the sources of electric and magnetic Ramond–Ramond fields that are required by string duality. D-branes added additional rich mathematical structure to the theory, and opened possibilities for constructing realistic cosmological models in the theory (for details, see Brane cosmology).

In 1997–98, Juan Maldacena conjectured a relationship between type IIB string theory and *N* = 4 supersymmetric Yang–Mills theory, a gauge theory. This conjecture, called the AdS/CFT correspondence, has generated a great deal of interest in high energy physics. It is a realization of the holographic principle, which has far-reaching implications: the AdS/CFT correspondence has helped elucidate the mysteries of black holes suggested by Stephen Hawking's work and is believed to provide a resolution of the black hole information paradox.

千禧年
---

已隱藏部分未翻譯内容，歡迎參與翻譯。
In 2003, Michael R. Douglas's discovery of the string theory landscape, which suggests that string theory has a large number of inequivalent false vacua, led to much discussion of what string theory might eventually be expected to predict, and how cosmology can be incorporated into the theory.

A possible mechanism of string theory vacuum stabilization (the KKLT mechanism) was proposed in 2003 by Shamit Kachru, Renata Kallosh, Andrei Linde, and Sandip Trivedi.

參考
--

* Rickles, Dean.. Springer. 2014. ISBN 978-3-642-45128-7.

1. ↑  Heisenberg, W.. Zeitschrift für Physik. 1943, **120** (7): 513–538. Bibcode:1943ZPhy..120..513H. S2CID 120706757. doi:10.1007/bf01329800.
2. ↑  Rickles 2014, p. 28 n. 17: "S-matrix theory had enough time to spawn string theory".
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4. ↑  John Archibald Wheeler, "On the Mathematical Description of Light Nuclei by the Method of Resonating Group Structure", *Phys. Rev.* **52**, 1107–1122 (1937).
5. ↑  Rickles 2014, p. 113："An unfortunate (for string theory) series of events terminated the growing popularity that string theory was enjoying in the early 1970s."
6. ↑  Rickles 2014, p. 4.
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16. ↑  Regge, Tullio, "Introduction to complex angular momentum," *Il Nuovo Cimento Series* 10, Vol. 14, 1959, p. 951.
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51. ↑  Candelas, P.; Horowitz, G.; Strominger, A.; Witten, E.. Nuclear Physics B. 1985, **258**: 46–74. Bibcode:1985NuPhB.258...46C. doi:10.1016/0550-3213(85)90602-9.
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53. 1 2  Green, M. B. Schwarz, J. H. (1982). "Supersymmetrical string theories." *Physics Letters B*, **109**, 444–448 (this paper classified the consistent ten-dimensional superstring theories and gave them the names Type I, Type IIA, and Type IIB).
54. ↑  This was demonstrated in Nahm, Werner, "Supersymmetries and their representations". *Nuclear Physics B* **135** no 1 (1978) pp 149-166, doi:10.1016/0550-3213(78)90218-3 （页面存档备份，存于）
55. ↑  E. Bergshoeff, E. Sezgin, P. K. Townsend, "Supermembranes and Eleven-Dimensional Supergravity," *Phys. Lett. B* **189**: 75 (1987).
56. ↑  It was Edward Witten who observed that the theory must be an 11-dimensional one in Witten, Edward.. Nuclear Physics B. 1995, **443** (1): 85–126. Bibcode:1995NuPhB.443...85W. S2CID 16790997. arXiv:hep-th/9503124 可免费查阅. doi:10.1016/0550-3213(95)00158-O.
57. ↑  Duff, Michael.. Scientific American. 1998, **278** (2): 64–9. Bibcode:1998SciAm.278b..64D. doi:10.1038/scientificamerican0298-64.
58. ↑  When Witten named it M-theory, he did not specify what the "M" stood for, presumably because he did not feel he had the right to name a theory he had not been able to fully describe. The "M" sometimes is said to stand for Mystery, or Magic, or Mother. More serious suggestions include Matrix or Membrane. Sheldon Glashow has noted that the "M" might be an upside down "W", standing for Witten. Others have suggested that the "M" in M-theory should stand for Missing, Monstrous or even Murky. According to Witten himself, as quoted in the PBS documentary （页面存档备份，存于） based on Brian Greene's *The Elegant Universe*, the "M" in M-theory stands for "magic, mystery, or matrix according to taste."
59. ↑  Rickles 2014, p. 208 n. 2.
60. ↑  Polchinski, J.. Physical Review D. 1995, **50** (10): R6041–R6045. Bibcode:1995PhRvL..75.4724P. PMID 10059981. S2CID 4671529. arXiv:hep-th/9510017 可免费查阅. doi:10.1103/PhysRevLett.75.4724.
61. ↑  Rickles 2014, p. 212.
62. ↑  Maldacena, Juan.. Advances in Theoretical and Mathematical Physics. 1998, **2** (4): 231–252. Bibcode:1998AdTMP...2..231M. arXiv:hep-th/9711200 可免费查阅. doi:10.4310/ATMP.1998.V2.N2.A1.
63. ↑  Rickles 2014, p. 207.
64. ↑  Rickles 2014, p. 222.
65. ↑  Maldacena, Juan.  (PDF). Scientific American. 2005, **293** (5): 56–63. Bibcode:2005SciAm.293e..56M. PMID 16318027. doi:10.1038/scientificamerican1105-56. （原始内容 (PDF)存档于2013-11-10）.  (p. 63.)
66. ↑  Douglas, Michael R. "The statistics of string / M theory vacua", *JHEP* **0305**, 46 (2003). arXiv:hep-th/0303194
67. ↑  The most commonly quoted number is of the order 10500. See: Ashok S. Douglas, M. "Counting flux vacua", *JHEP* **0401**, 060 (2004).
68. ↑  Rickles 2014, pp. 230–5 and 236 n. 63.
69. ↑  Kachru, Shamit; Kallosh, Renata; Linde, Andrei; Trivedi, Sandip P.. Physical Review D. 2003, **68** (4): 046005. Bibcode:2003PhRvD..68d6005K. S2CID 119482182. arXiv:hep-th/0301240 可免费查阅. doi:10.1103/PhysRevD.68.046005.

進一步閱讀
-----

* Paul Frampton.. Frontiers in Physics, W. A. Benjamin. 1974. ISBN 978-0-8053-2581-2.
* Joel A. Shapiro.. 2007. arXiv:0711.3448 可免费查阅 [hep-th].
* John H. Schwarz.. 2012. arXiv:1201.0981 可免费查阅 [physics.hist-ph].
* Andrea Cappelli; Elena Castellani; Filippo Colomo; Paolo Di Vecchia.. Cambridge University Press. 2012. ISBN 978-0-521-19790-8.

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| * 
* 论
* 编
弦理論 |
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|  |
| 基本对象 | 
* 弦
* 膜
* D膜
* S膜（英语：）
* NS5膜
* M2膜
* M5膜
* 黑膜（英语：）

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| 背景理論 | 
* 南部-后藤作用量
* 泊里雅科夫作用量
* 陳-西蒙斯理論
* 共形场论
* 量子引力
* 卡鲁扎-克莱因理论
* 全像原理
* 万有理论
* 杨-米尔斯理论

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|  |
| 微扰弦理论 | 
* 玻色弦理論
* 超弦理論
* 第一型弦理論
* 第二型弦理論（第二A型 · 第二B型）
* 混合弦理論（SO(32)雜弦 · *E*8x*E*8雜弦）
* 弦拓扑
* 扭量弦理論（英语：）

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| 非微扰结果 | 
* 弦場論
* 弦論對偶性
* S對偶
* T對偶
* U對偶
* 镜像对称性
* M理论（入門）
* AdS/CFT对偶

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| 现象学 | 
* 弦唯象学
* 弦宇宙學
* 弦論地景
* 膜宇宙學

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| 数学方法 | 
* 陈–怕吞因素
* 摄动理论
* 巴塔林-維爾可維斯基代數
* 格爾斯滕哈伯代數
* 顶点算子代数
* 維拉宿代數
* 卡茨-穆迪代數
* 1/N展开

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|  |
| 几何 | 
* RNS体系（英语：）
* GS体系（英语：）
* GSO映射（英语：）
* 卡拉比-丘流形
* K3曲面
* G2流形（英语：）
* 紧化
* 軌形（英语：）
* 定向形（英语：）
* 錐形(弦论)（英语：）
* 塞伯格-維騰理論
* 塞伯格-維騰不變量
* 塞伯格-維騰映射
* 快子凝聚
* 微扰反常
* O(N)模型
* 非线性σ模型

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|  |
| 规范场论 | 
* 陈-西蒙斯形式
* 楊-米爾斯理論
* Wess-Zumino-Witten模型
* 纽结理论
* 瞬子
* BRST量子化
* BPS態
* 磁单极子

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| 超对称 | 
* 超引力
* 超空間
* 李超群（英语：）
* 超對稱楊-米爾斯理論

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|  |
| 理论家 | 
* 阿尔卡尼-哈米德
* 迈克尔·阿蒂亚
* 湯姆·班克斯
* 陈省身
* 戴克赫拉夫
* 朵夫（英语：）
* 費斯勒（英语：）
* 丹尼爾·弗里丹
* 蓋茲（英语：）
* Gliozzi（英语：）
* 迈克尔·格林 (物理学家)
* 布莱恩·葛林
* 戴维·格娄斯
* 葛布澤（英语：）
* 哈維（英语：）
* 霍扎瓦（英语：）
* 加来道雄
* Klebanov（英语：）
* 南部阳一郎
* 孔采维奇
* 胡安·马尔达西那
* 曼德尔施塔姆
* Martinec（英语：）
* 格雷·穆爾
* 莫特爾
* Nekrasov（英语：）
* Neveu（英语：）
* 奧利佛（英语：）
* 波尔钦斯基
* 泊里雅科夫
* 加來道雄
* 麗莎·藍道爾
* 皮埃尔·拉蒙
* Rohm（英语：）
* Scherk（英语：）
* 约翰·施瓦茨
* 内森·塞伯格
* Sen（英语：）
* Sơn（英语：）
* 安德鲁·施特罗明格
* 桑壯（英语：）
* 萨斯坎德
* 特·胡夫特
* Townsend（英语：）
* 瓦法
* 韦内齐亚诺
* 埃·弗尔林德
* 赫·弗尔林德（英语：）
* 爱德华·威滕
* 杨振宁
* 丘成桐
* Zaslow（英语：）
* 弗朗克·韦尔切克
* 文小刚
* 徐一鴻

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* 历史
* 词汇

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| 

| * 
* 论
* 编
重力理論 |
| --- |
|  |
| 標準引力理論 | 

|  |  |
| --- | --- |
| 牛頓重力 | 
* 万有引力定律（古典力學）
* 重力理論史

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|  |
| 廣義相對論 | 
* 入門
* 歷史
* 數學
* 验证
* 後牛頓形式論
* 線性化重力
* ADM質量

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|  |
| 廣義相對論的替代理論 | 

|  |  |
| --- | --- |
| 範型 | 
* 古典重力理論
* 量子重力
* 万有理论

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|  |
| 古典重力理論 | 
* 愛因斯坦-嘉當理論（ECT理論）
* 雙度規理論（英语：）
* 共形重力（英语：）
* 調整牛頓動力學（英语：）
* 幾何動力學（英语：）
* Teleparallelism（英语：）
* 複合重力（英语：）
* 具質量重力（英语：）
* 純量重力理論（英语：）（諾德斯特洛姆重力理論（英语：））
* 純量-張量理論（英语：）（布蘭斯-狄克理論（英语：））
* 懷海德重力理論（英语：）
* 非對稱重力理論（英语：）
* 純量-張量-向量重力（英语：）
* 張量-向量-純量重力（英语：）

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|  |
| 量子重力理論 | 
* 歐幾里得量子重力（英语：）
* 正則量子重力（英语：）（惠勒-德威特方程式 · 迴圈量子重力 · 自旋泡沫）
* 因果動力學三角剖分（英语：）
* 引生重力（英语：）
* 因果集（英语：）
* DGP模型

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|  |
| 经典统一场论 | 
* 卡魯扎-克萊因理論
* 超引力

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|  |
| 量子统一场论 | 
* 非交換幾何（自我創造宇宙學（英语：））
* 半古典重力
* 弦論（M理论 · 超弦理論）

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|  |
| 廣義相對論推廣 | 
* 劉維爾重力（英语：）
* 高斯-博內重力（英语：）

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|  |
| 前牛頓理論與玩具模型 | 亚里士多德物理学（重力理論） · 重力的力學解釋（英语：）（勒薩吉重力理論 · 引力的熵力假说） · 反物質的重力交互作用（英语：） |

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