Superstring theory

Superstring theory is an attempt to explain all of the particles and fundamental forces of nature in one theory by modeling them as vibrations of tiny supersymmetric strings.

'Superstring theory' is a shorthand for supersymmetric string theory because unlike bosonic string theory, it is the version of string theory that accounts for both fermions and bosons and incorporates supersymmetry to model gravity.

Since the second superstring revolution, the five superstring theories (Type I, Type IIA, Type IIB, HO and HE) are regarded as different limits of a single theory tentatively called M-theory.

Background

One of the deepest open problems in theoretical physics is formulating a theory of quantum gravity. Such a theory incorporates both the theory of general relativity, which describes gravitation and applies to large-scale structures, and quantum mechanics or more specifically quantum field theory, which describes the other three fundamental forces that act on the atomic scale.

Quantum field theory, in particular the Standard model, is currently the most successful theory to describe fundamental forces, but while computing physical quantities of interest, naïvely one obtains infinite values. Physicists developed the technique of renormalization to 'eliminate these infinities' to obtain finite values which can be experimentally tested. This technique works for three of the four fundamental forces: Electromagnetism, the strong force and the weak force, but does not work for gravity, which is non-renormalizable. Development of a quantum theory of gravity therefore requires different means than those used for the other forces.[1]

According to superstring theory, or more generally string theory, the fundamental constituents of reality are strings with radius on the order of the Planck length (about 10−33 cm). An appealing feature of string theory is that fundamental particles can be viewed as excitations of the string. The tension in a string is on the order of the Planck force (1044 newtons). The graviton (the proposed messenger particle of the gravitational force) is predicted by the theory to be a string with wave amplitude zero.

History

Investigating how a string theory may include fermions in its spectrum led to the invention of supersymmetry (in the West[clarification needed])[2] in 1971,[3] a mathematical transformation between bosons and fermions. String theories that include fermionic vibrations are now known as "superstring theories".

Since its beginnings in the seventies and through the combined efforts of many different researchers, superstring theory has developed into a broad and varied subject with connections to quantum gravity, particle and condensed matter physics, cosmology, and pure mathematics.

Absence of physical evidence

Superstring theory is based on supersymmetry. No supersymmetric particles have been discovered and initial investigation, carried out in 2011 at the Large Hadron Collider (LHC)[4] and in 2006 at the Tevatron has excluded some of the ranges.[5][self-published source?][6][7][8] For instance, the mass constraint of the Minimal Supersymmetric Standard Model squarks has been up to 1.1 TeV, and gluinos up to 500 GeV.[9] No report on suggesting large extra dimensions has been delivered from LHC. There have been no principles so far to limit the number of vacua in the concept of a landscape of vacua.[10]

Some particle physicists became disappointed by the lack of experimental verification of supersymmetry, and some have already discarded it.[11] Jon Butterworth at University College London said that we had no sign of supersymmetry, even in higher energy region, excluding the superpartners of the top quark up to a few TeV. Ben Allanach at the University of Cambridge states that if we do not discover any new particles in the next trial at the LHC, then we can say it is unlikely to discover supersymmetry at CERN in the foreseeable future.[11]

Extra dimensions

Our physical space is observed to have three large spatial dimensions and, along with time, is a boundless 4-dimensional continuum known as spacetime. However, nothing prevents a theory from including more than 4 dimensions. In the case of string theory, consistency requires spacetime to have 10 dimensions (3D regular space + 1 time + 6D hyperspace).[12] The fact that we see only 3 dimensions of space can be explained by one of two mechanisms: either the extra dimensions are compactified on a very small scale, or else our world may live on a 3-dimensional submanifold corresponding to a brane, on which all known particles besides gravity would be restricted.

If the extra dimensions are compactified, then the extra 6 dimensions must be in the form of a Calabi–Yau manifold. Within the more complete framework of M-theory, they would have to take form of a G2 manifold. A particular exact symmetry of string/M-theory called T-duality (which exchanges momentum modes for winding number and sends compact dimensions of radius R to radius 1/R),[13] has led to the discovery of equivalences between different Calabi–Yau manifolds called mirror symmetry.

Superstring theory is not the first theory to propose extra spatial dimensions. It can be seen as building upon the Kaluza–Klein theory, which proposed a 4+1 dimensional (5D) theory of gravity. When compactified on a circle, the gravity in the extra dimension precisely describes electromagnetism from the perspective of the 3 remaining large space dimensions. Thus the original Kaluza–Klein theory is a prototype for the unification of gauge and gravity interactions, at least at the classical level, however it is known to be insufficient to describe nature for a variety of reasons (missing weak and strong forces, lack of parity violation, etc.) A more complex compact geometry is needed to reproduce the known gauge forces. Also, to obtain a consistent, fundamental, quantum theory requires the upgrade to string theory, not just the extra dimensions.

Number of superstring theories

Theoretical physicists were troubled by the existence of five separate superstring theories. A possible solution for this dilemma was suggested at the beginning of what is called the second superstring revolution in the 1990s, which suggests that the five string theories might be different limits of a single underlying theory, called M-theory. This remains a conjecture.[14]

String theories
Type Spacetime dimensions SUSY generators chiral open strings heterotic compactification gauge group tachyon
Bosonic (closed) 26 N = 0 no no no none yes
Bosonic (open) 26 N = 0 no yes no U(1) yes
I 10 N = (1,0) yes yes no SO(32) no
IIA 10 N = (1,1) no no no U(1) no
IIB 10 N = (2,0) yes no no none no
HO 10 N = (1,0) yes no yes SO(32) no
HE 10 N = (1,0) yes no yes E8 × E8 no
M-theory 11 N = 1 no no no none no

The five consistent superstring theories are:

  • The type I string has one supersymmetry in the ten-dimensional sense (16 supercharges). This theory is special in the sense that it is based on unoriented open and closed strings, while the rest are based on oriented closed strings.
  • The type II string theories have two supersymmetries in the ten-dimensional sense (32 supercharges). There are actually two kinds of type II strings called type IIA and type IIB. They differ mainly in the fact that the IIA theory is non-chiral (parity conserving) while the IIB theory is chiral (parity violating).
  • The heterotic string theories are based on a peculiar hybrid of a type I superstring and a bosonic string. There are two kinds of heterotic strings differing in their ten-dimensional gauge groups: the heterotic E8×E8 string and the heterotic SO(32) string. (The name heterotic SO(32) is slightly inaccurate since among the SO(32) Lie groups, string theory singles out a quotient Spin(32)/Z2 that is not equivalent to SO(32).)

Chiral gauge theories can be inconsistent due to anomalies. This happens when certain one-loop Feynman diagrams cause a quantum mechanical breakdown of the gauge symmetry. The anomalies were canceled out via the Green–Schwarz mechanism.

Even though there are only five superstring theories, making detailed predictions for real experiments requires information about exactly what physical configuration the theory is in. This considerably complicates efforts to test string theory because there is an astronomically high number—10500 or more—of configurations that meet some of the basic requirements to be consistent with our world. Along with the extreme remoteness of the Planck scale, this is the other major reason it is hard to test superstring theory.

Another approach to the number of superstring theories refers to the mathematical structure called composition algebra. In the findings of abstract algebra there are just seven composition algebras over the field of real numbers. In 1990 physicists R. Foot and G.C. Joshi in Australia stated that "the seven classical superstring theories are in one-to-one correspondence to the seven composition algebras".[15]

Integrating general relativity and quantum mechanics

General relativity typically deals with situations involving large mass objects in fairly large regions of spacetime whereas quantum mechanics is generally reserved for scenarios at the atomic scale (small spacetime regions). The two are very rarely used together, and the most common case that combines them is in the study of black holes. Having peak density, or the maximum amount of matter possible in a space, and very small area, the two must be used in synchrony to predict conditions in such places. Yet, when used together, the equations fall apart, spitting out impossible answers, such as imaginary distances and less than one dimension.

The major problem with their incongruence is that, at Planck scale (a fundamental small unit of length) lengths, general relativity predicts a smooth, flowing surface, while quantum mechanics predicts a random, warped surface, which are nowhere near compatible. Superstring theory resolves this issue, replacing the classical idea of point particles with strings. These strings have an average diameter of the Planck length, with extremely small variances, which completely ignores the quantum mechanical predictions of Planck-scale length dimensional warping. Also, these surfaces can be mapped as branes. These branes can be viewed as objects with a morphism between them. In this case, the morphism will be the state of a string that stretches between brane A and brane B.

Singularities are avoided because the observed consequences of "Big Crunches" never reach zero size. In fact, should the universe begin a "big crunch" sort of process, string theory dictates that the universe could never be smaller than the size of one string, at which point it would actually begin expanding.

Mathematics

D-branes

D-branes are membrane-like objects in 10D string theory. They can be thought of as occurring as a result of a Kaluza–Klein compactification of 11D M-theory that contains membranes. Because compactification of a geometric theory produces extra vector fields the D-branes can be included in the action by adding an extra U(1) vector field to the string action.

In type I open string theory, the ends of open strings are always attached to D-brane surfaces. A string theory with more gauge fields such as SU(2) gauge fields would then correspond to the compactification of some higher-dimensional theory above 11 dimensions, which is not thought to be possible to date. Furthermore, the tachyons attached to the D-branes show the instability of those D-branes with respect to the annihilation. The tachyon total energy is (or reflects) the total energy of the D-branes.

Why five superstring theories?

For a 10 dimensional supersymmetric theory we are allowed a 32-component Majorana spinor. This can be decomposed into a pair of 16-component Majorana-Weyl (chiral) spinors. There are then various ways to construct an invariant depending on whether these two spinors have the same or opposite chiralities:

Superstring model Invariant
Heterotic
IIA
IIB

The heterotic superstrings come in two types SO(32) and E8×E8 as indicated above and the type I superstrings include open strings.

Beyond superstring theory

It is conceivable that the five superstring theories are approximated to a theory in higher dimensions possibly involving membranes. Because the action for this involves quartic terms and higher so is not Gaussian, the functional integrals are very difficult to solve and so this has confounded the top theoretical physicists. Edward Witten has popularised the concept of a theory in 11 dimensions, called M-theory, involving membranes interpolating from the known symmetries of superstring theory. It may turn out that there exist membrane models or other non-membrane models in higher dimensions—which may become acceptable when we find new unknown symmetries of nature, such as noncommutative geometry. It is thought, however, that 16 is probably the maximum since SO(16) is a maximal subgroup of E8, the largest exceptional Lie group, and also is more than large enough to contain the Standard Model. Quartic integrals of the non-functional kind are easier to solve so there is hope for the future. This is the series solution, which is always convergent when a is non-zero and negative:

In the case of membranes the series would correspond to sums of various membrane interactions that are not seen in string theory.

Compactification

Investigating theories of higher dimensions often involves looking at the 10 dimensional superstring theory and interpreting some of the more obscure results in terms of compactified dimensions. For example, D-branes are seen as compactified membranes from 11D M-theory. Theories of higher dimensions such as 12D F-theory and beyond produce other effects, such as gauge terms higher than U(1). The components of the extra vector fields (A) in the D-brane actions can be thought of as extra coordinates (X) in disguise. However, the known symmetries including supersymmetry currently restrict the spinors to 32-components—which limits the number of dimensions to 11 (or 12 if you include two time dimensions.) Some physicists (e.g., John Baez et al.) have speculated that the exceptional Lie groups E6, E7 and E8 having maximum orthogonal subgroups SO(10), SO(12) and SO(16) may be related to theories in 10, 12 and 16 dimensions; 10 dimensions corresponding to string theory and the 12 and 16 dimensional theories being yet undiscovered but would be theories based on 3-branes and 7-branes respectively. However, this is a minority view within the string community. Since E7 is in some sense F4 quaternified and E8 is F4 octonified, the 12 and 16 dimensional theories, if they did exist, may involve the noncommutative geometry based on the quaternions and octonions respectively. From the above discussion, it can be seen that physicists have many ideas for extending superstring theory beyond the current 10 dimensional theory, but so far all have been unsuccessful.

Kac–Moody algebras

Since strings can have an infinite number of modes, the symmetry used to describe string theory is based on infinite dimensional Lie algebras. Some Kac–Moody algebras that have been considered as symmetries for M-theory have been E10 and E11 and their supersymmetric extensions.

See also

References

  1. ^ Polchinski 1998a, p. 4
  2. ^ Rickles, Dean (2014). A Brief History of String Theory: From Dual Models to M-Theory. Springer, p. 104. ISBN 978-3-642-45128-7
  3. ^ J. L. Gervais and B. Sakita worked on the two-dimensional case in which they use the concept of "supergauge," taken from Ramond, Neveu, and Schwarz's work on dual models: Gervais, J.-L.; Sakita, B. (1971). "Field theory interpretation of supergauges in dual models". Nuclear Physics B. 34 (2): 632–639. Bibcode:1971NuPhB..34..632G. doi:10.1016/0550-3213(71)90351-8.
  4. ^ Buchmueller, O.; Cavanaugh, R.; Colling, D.; De Roeck, A.; Dolan, M. J.; Ellis, J. R.; Flächer, H.; Heinemeyer, S.; Isidori, G.; Olive, K.; Rogerson, S.; Ronga, F.; Weiglein, G. (May 2011). "Implications of initial LHC searches for supersymmetry". The European Physical Journal C. 71 (5): 1634. arXiv:1102.4585. Bibcode:2011EPJC...71.1634B. doi:10.1140/epjc/s10052-011-1634-1. S2CID 52026092.
  5. ^ Woit, Peter (February 22, 2011). "Implications of Initial LHC Searches for Supersymmetry".
  6. ^ Cassel, S.; Ghilencea, D. M.; Kraml, S.; Lessa, A.; Ross, G. G. (2011). "Fine-tuning implications for complementary dark matter and LHC SUSY searches". Journal of High Energy Physics. 2011 (5): 120. arXiv:1101.4664. Bibcode:2011JHEP...05..120C. doi:10.1007/JHEP05(2011)120. S2CID 53467362.
  7. ^ Falkowski, Adam (Jester) (February 16, 2011). "What LHC tells about SUSY". resonaances.blogspot.com. Archived from the original on March 22, 2014. Retrieved March 22, 2014.
  8. ^ Tapper, Alex (24 March 2010). "Early SUSY searches at the LHC" (PDF). Imperial College London.
  9. ^ Chatrchyan, S.; et al. (2011-11-21). "Search for Supersymmetry at the LHC in Events with Jets and Missing Transverse Energy". Physical Review Letters. 107 (22). CMS Collaboration: 221804. arXiv:1109.2352. Bibcode:2011PhRvL.107v1804C. doi:10.1103/PhysRevLett.107.221804. ISSN 0031-9007. PMID 22182023. S2CID 22498269.
  10. ^ Shifman, M. (2012). "Frontiers Beyond the Standard Model: Reflections and Impressionistic Portrait of the Conference". Modern Physics Letters A. 27 (40): 1230043. Bibcode:2012MPLA...2730043S. doi:10.1142/S0217732312300431.
  11. ^ a b Jha, Alok (August 6, 2013). "One year on from the Higgs boson find, has physics hit the buffers?". The Guardian. photograph: Harold Cunningham/Getty Images. London: GMG. ISSN 0261-3077. OCLC 60623878. Archived from the original on March 22, 2014. Retrieved March 22, 2014.
  12. ^ The D = 10 critical dimension was originally discovered by John H. Schwarz in Schwarz, J. H. (1972). "Physical states and pomeron poles in the dual pion model". Nuclear Physics, B46(1), 61–74.
  13. ^ Polchinski 1998a, p. 247
  14. ^ Polchinski 1998b, p. 198
  15. ^ Foot, R.; Joshi, G. C. (1990). "Nonstandard signature of spacetime, superstrings, and the split composition algebras". Letters in Mathematical Physics. 19 (1): 65–71. Bibcode:1990LMaPh..19...65F. doi:10.1007/BF00402262. S2CID 120143992.

Cited sources

Read other articles:

Species of plant Lemon grass Scientific classification Kingdom: Plantae Clade: Tracheophytes Clade: Angiosperms Clade: Monocots Clade: Commelinids Order: Poales Family: Poaceae Subfamily: Panicoideae Genus: Cymbopogon Species: C. citratus Binomial name Cymbopogon citratus(DC.) Stapf,[1] 1906 Synonyms[2] List Andropogon cerifer Hack. Andropogon ceriferus Hack. Andropogon citratus DC. Andropogon citriodorus Desf. nom. inval. Andropogon fragrans C.Cordem. Andropogon roxburgh...

This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by adding missing items with reliable sources. Marion Cotillard awards and nominations Cotillard at the 2017 Cabourg Film Festival Award Wins Nominations Academy Awards 1 2 BAFTA Awards 1 2 César Awards 2 7 European Film Awards 1 2 Golden Globe Awards 1 4 SAG Awards 0 4 Wins 30 Runner-up 4 Nominations 66 This is a list of awards and nominations received by French actress Marion Cotilla...

American law enforcement official (born 1959) Keith SchillerDirector of Oval Office OperationsIn officeJanuary 20, 2017 – September 20, 2017PresidentDonald TrumpPreceded byBrian MostellerSucceeded byJordan Karem Personal detailsBorn1959 (age 63–64)New York City, New York, U.S.Political partyRepublicanSpouseLena SchillerChildren2Military serviceBranch/serviceUnited States NavyYears of service1978–1982RankRadioman Keith Schiller (born c. 1959)[1] is an...

Tora! Tora! Tora! (Filmposter op en.wikipedia.org) Regie Richard FleischerKinji FukasakuToshio Masuda Scenario Ladislas FaragoGordon W. PrangeLarry ForresterRyuzo KikushimaHideo OguniAkira Kurosawa Muziek Jerry Goldsmith Distributie Twentieth Century Fox Première 23 september 1970 Genre Oorlogsfilm Speelduur ca 138 minuten (dvd) Taal Engels/Japans Land Verenigde Staten / Japan (en) IMDb-profiel MovieMeter-profiel Portaal    Film Tora! Tora! Tora! (Japans: トラ・トラ・トラ) ...

Денис Миколайович Меньшов Персональні дані Дата  народження 25 січня 1978(1978-01-25) (45 років) Країна  Росія Зріст 180 см Вага 65 кг Командна інформація Дисципліна Шосейні велоперегони Тип гонщика універсал Професійні команди 2000–20042005–201020112012–2013 BanestoRabobankGeox–TMCKatusha[1] Г�...

Railway station in Bridgend, Wales WildmillWelsh: Melin WylltGeneral informationLocationBridgend, BridgendWalesCoordinates51°31′12″N 3°34′49″W / 51.5199°N 3.5803°W / 51.5199; -3.5803Grid referenceSS904812Managed byTransport for Wales RailPlatforms1Other informationStation codeWMIClassificationDfT category F2HistoryOriginal companyBritish RailKey dates16 November 1992 (1992-11-16)Opened16 November 1992Closed12 December 1992ReopenedPassengers20...

Production history British TV sci-fi series (1963–) This page is about the production history of the TV series Doctor Who. For a more general overview, see the main Doctor Who page. For more about the main character of the Doctor, see the The Doctor (Doctor Who). Pages regarding individual Doctors and the various series and serials are linked in the List of Doctor Who serials. For information about the Dalek films of the 1960s, see Dr. Who (Dalek films). This article has multiple issues. Pl...

American college football season 2023 Northwestern Wildcats footballLas Vegas Bowl, vs. UtahConferenceBig Ten ConferenceDivisionWest DivisionRecord7–5 (5–4 Big Ten)Head coachDavid Braun (1st season)Offensive coordinatorMike Bajakian (4th season)Offensive schemeSpreadBase defenseMultiple 4–3Home stadiumRyan Field(capacity: 47,130)Seasons← 20222024 → 2023 Big Ten Conference football standings vte Conf Overall Team   W   L   ...

Province of the Byzantine Empire Theme of ThessalonicaΘεσσαλονίκη, θέμα ΘεσσαλονίκηςTheme of the Byzantine Empire800s (decade)–12041242–1392Map of Byzantine Greece ca. 900 AD, with the themes and major settlementsCapitalThessalonicaHistoryHistorical eraMiddle Ages• Established 809• Fourth Crusade 1204• Recovery by Nicaean Empire 1242• Captured by Ottomans 1392 Today part ofGreece The Theme of Thessalonica (Greek: Θέμα Θεσσαλ...

2023 Marathi action drama film SuryaTheatrical release posterDirected byHasnain HyderabadwalaScreenplay byVijay KadamMangesh ThangeMangesh KedarHemant EdalabadkarStory byMangesh ThangeProduced byReshma Mangesh ThangeRajendra ThakareAakash GoelStarring Prakash Mangesh Ruchita Jadhav Akhilendra Mishra Hemant Birje Uday Tikekar Pradeep Patwardhan Arun Nalawade CinematographyMadhu S RaoEdited byRahul BhatankaMusic byDev ChouhanProductioncompanySP Motion PicturesRelease date January 6, 2...

Clase I-400 I-400, con su gran hangar y catapulta delanteraPaís productorPaís productor Países en servicio Armada Imperial JaponesaTipo submarino portaavionesEstadísticasPrimera unidad Japanese submarine I-400Clase posterior Submarinos Clase I-201Periodo construcción 1944-45Unidades planteadas 18Unidades concluidas 3Unidades hundidas 3 (echadas a pique)Características de la claseDesplazamiento 5.223 tDesplazamiento en inmersión 6.560 tEslora 122 mManga 12 mCalado 7 mArmamento 8 tubos l...

Women's national basketball team representing the United States This article is about the women's team. For the men's team, see United States men's national basketball team. United StatesFIBA ranking1 (August 21, 2023)[1]FIBA zoneFIBA AmericasNational federationUSA BasketballCoachCheryl ReeveNickname(s)Team USAUSBWNTOlympic GamesAppearances11Medals Gold: (1984, 1988,1996, 2000, 2004, 2008, 2012, 2016, 2020) Silver: (1976) Bronze: (1992)World CupAppearances17Medals Gold: (1953, 1957, 1...

Instituto Japonés de la Imagen en Movimiento 日本映画大学 Nihon Eiga Daigaku LocalizaciónPaís  JapónLocalidad Kawasaki JapónCoordenadas 35°35′30″N 139°30′45″E / 35.591654, 139.512402InformaciónApertura 1975[editar datos en Wikidata] El Instituto Japonés de la Imagen en Movimiento[1]​ (en japonés: 日本映画大学 Nihon Eiga Daigaku) antes conocida como la Escuela Técnica de Radiodifusión de Yokohama, es una escuela de cine ...

Artikel ini memberikan informasi dasar tentang topik kesehatan. Informasi dalam artikel ini hanya boleh digunakan hanya untuk penjelasan ilmiah, bukan untuk diagnosis diri dan tidak dapat menggantikan diagnosis medis. Perhatian: Informasi dalam artikel ini bukanlah resep atau nasihat medis. Wikipedia tidak memberikan konsultasi medis. Jika Anda perlu bantuan atau hendak berobat, berkonsultasilah dengan tenaga kesehatan profesional. Artikel ini perlu dikembangkan agar dapat memenuhi kriteria s...

1927 film by Alan Crosland Not to be confused with The Delightful Rogue. The Beloved RogueOriginal theatrical posterDirected byAlan CroslandWritten byPaul Bern (adaptation & scenario)Walter Anthony (intertitles)Based onIf I Were Kingby Justin Huntley McCarthyProduced byJoseph M. SchenckStarringJohn BarrymoreCinematographyJoseph H. AugustEdited byHal C. KernProductioncompaniesArt Cinema Corporation /Feature ProductionsDistributed byUnited ArtistsRelease date March 12, 1927 (...

Japanese media franchise This article needs additional citations for verification. Please help improve this article by adding citations to reliable sources. Unsourced material may be challenged and removed.Find sources: Subete ga F ni Naru – news · newspapers · books · scholar · JSTOR (December 2014) (Learn how and when to remove this template message) Subete ga F ni NaruCover of Subete ga F ni Naru novelすべてがFになる NovelWritten byHiros...

Series of fiction anthologies collecting original stories Books of Blood Books of Blood Omnibus, volumes 1–3AuthorClive BarkerCover artistClive BarkerCountryUnited KingdomLanguageEnglishSeriesBooks of BloodGenreHorrorPublisherSphere Books (UK)Publication date1984–1985Media typePrint (Hardcover and Paperback) Books of Blood is a series of six horror fiction anthologies collecting original stories written by British author, playwright, and filmmaker Clive Barker in 1984 and 1985. ...

1955 Indian filmJayasimhaTheatrical release posterDirected byD. YoganandWritten bySamudrala JrProduced byN. Trivikrama RaoStarringN. T. Rama RaoAnjali DeviS. V. Ranga RaoWaheeda RehmanCinematographyM. A. RehmanEdited byG. D. JoshiMusic byT. V. RajuProductioncompanyNational Art TheaterRelease date 21 October 1955 (1955-10-21) Running time165 minsCountryIndiaLanguageTelugu Jayasimha is a 1955 Indian Telugu-language swashbuckler film, written by Samudrala Jr. and produced by N. T....

この記事は検証可能な参考文献や出典が全く示されていないか、不十分です。出典を追加して記事の信頼性向上にご協力ください。(このテンプレートの使い方)出典検索?: コメット連続墜落事故 – ニュース · 書籍 · スカラー · CiNii · J-STAGE · NDL · dlib.jp · ジャパンサーチ · TWL(2018年6月) 英国海外航空のコメットMk.I コメッ...

This article includes a list of general references, but it lacks sufficient corresponding inline citations. Please help to improve this article by introducing more precise citations. (September 2015) (Learn how and when to remove this template message) 56th (King's Own) Anti-Tank RegimentBush hat badge and PA patch worn in BurmaActive1938–1961Country United KingdomBranch Territorial ArmyRoleAnti-Tank artillerySizeRegimentGarrison/HQUlverstonMotto(s)RA mottoes:Quo Fas Et Gloria Ducunt (...