File:Monopole_SU(2)_vortices.jpg The simplest neutral quadruplet of chiral vortices.[1] Electromagnetism with SU(2) symmetry allows for complex nonlinear phenomena such as topological vortices, known as monopoles.

Magnetic monopoles are emergent quasiparticles that exist if and only if the electromagnetic field has non-trivial topology.[2] Magnetic monopoles conserve magnetism, in an analogous way that electrons and protons conserve electric charge. They can be thought of as a kind of domain wall or topological soliton that occurs when the symmetry of electric-magnetic duality is spontaneously broken. Condensation of magnetic monopoles induces the quantization of electric charge, in an exactly analogous way in the Higgs mechanism will quantize the mass of the electron. They can exhibit rich behaviour not encountered in conventional electromagnetism, and are far less constrained then the symmetry considerations required of a relativistically invariant electromagnetic field.[3]

Electromagnetic particles (e.g. electons, protons etc) described in the standard Maxwell equations, or quantum electrodynamics (QED) form a symmetry group. When a particle is translated into any other position, orientation, speed etc. the value of the particle's charge does not vary and is conserved under what is called a gauge transformation, the magnetisation of the particle is not conserved. By definition, a particle that would conserve magnetic and electric charge, a monopole or dyon, would have to have higher symmetry, monopoles are not allowed to exist in in order for divergence-less solenoidal magnetic fields to exist (i.e. it is a requirement of Gauss's law which states that ∇⋅B = 0). Only electric charge is conserved in symmetry. In order for magnetism to be conserved in particles we must use or higher symmetry groups.[4]

Electromagnetism as a gauge theory edit

Aharonov–Bohm effect edit

 

It is tempting to believe that if the electromagnetic field has no net force there here should be no electromagnetic action. The outcome of the Aharonov–Bohm experiment[a] is widely regarded as the strongest single piece of evidence that supports the view that electromagnetism is a gauge theory, and that the notion of local forces fails to describe all electromagnetic phenomena.[6]





Berry phase edit

History of searches for the monopole edit

Pierre Curie suggested in 1894 that monopoles might exist.[7] Henri Poincaré one of the founders of topology and who laid the groundwork for chaos theory, was aware that the lack symmetry in Maxwell's reformulated equations prevented monopoles, and in 1896[8] he investigated the motion of an electron in the presence of a monopole, spurred on by Kristian Birkeland's earlier report of anomalous motion of cathode rays in the presence of a magnetized needle.[9][10] Joseph John Thomson in 1900[11][12] investigated the case of a single magnetic pole[13] Paul Ulrich Villard known as the discover of gamma radiation believed he had discovered magnetic monopoles or has he called them magnetons, but the turned out to be the effect of cathode rays.[14][15]

https://books.google.co.uk/books?id=e9wEntQmA0IC&pg=PA96&lpg=PA96&dq=heaviside+monopole&source=bl&ots=f2oWrxzTRu&sig=15j2R-6DfsjsmMUk7CSK19XGR1o&hl=en&sa=X&ved=0ahUKEwjwnJ6C5JrSAhXhAMAKHd5uCawQ6AEIIzAB#v=onepage&q=no%20magnetic%20charge&f=false

https://books.google.co.uk/books?id=zXm1Bso1VREC&printsec=frontcover#v=onepage&q=villard%201905&f=false

History of monopole mathematics edit

Quaternionic electromagnetism edit

 
Broom Bridge

19th century mathematicians were inspired by the mathematical beauty of complex numbers and complex analysis[b] to seek new "generalized complex numbers" which would apply in a natural way to higher dimensions, and in particular, 3-dimensional space.[17] In 1843 William Rowan Hamilton famously discovered quaternions while walking across Broom Bridge.[c] Since complex numbers describe rotations in two dimensions and have two components, it might be thought that to describe three dimensions you need numbers which have three components, counterintuitively you need four dimensions to describe rotations in three dimension. A quaternion consists of an ordinary number, or scalar, combined with a vector, which has both magnitude and direction.[20] The vector can be broken down into three components i, j and k that are perpendicular, or orthogonal, to each other such that there is no linear relationship between these components. A quaternion is generally represented in the form a + bi + cj + dk and the vector identities can be related via:

Quaternion identities
 

where:

 

These quantities satisfy all the usual laws of algebra we are familiar with from real and complex numbers bar one rule: the commutative law of multiplication ab = ba is violated by quaternions.[21] The quaternions were the first time in history that a non-commutative product appeared in mathematics.[22] This non-commutativity can be visualised by considering rotation of an object in 3D, if we rotate about the object 900 about the X axis and then 900 about the Z axis it does not end up in the same configuaration as rotation about Z axis then X axis. Order of the operation matters, just like solving a rubix cube.

Hamilton's quaternions were the first step towards what is now called a Clifford algebra, developed in 1876 by William Kingdon Clifford.[d][24] In modern group theory, a group that preserves commutativity, like for example the complex numbers  , is said to form an abelian group named after Niels Henrik Abel; the quaternion group,  , is said to be a non-abelian.[e] The complex numbers,  , can be written by Euler's formula in the form   and form a   symmetry group. Geometrically,   is the unit circle  . We can identify the plane   with the complex plane  , letting   represent  . Multiplication of any complex number   can be thought of as a rotation by an angle   and is the same kind of symmetry as rotating a unit circle about the origin. For the quaternions,  , it is often helpful two write them in the form of a 2 × 2 complex matrix. The quaternion a + bi + cj + dk can be represented as:

 
 

Instead of the unit circle   in  , we need to consider the 3-sphere   embedded in four dimentional  .The 3-sphere   is the set of points   such that  . It can be shown that the   symmetry group is replaced by  .

 
Peter Guthrie Tait

In 1858 Hamilton begun corresponding with Peter Guthrie Tait.[26] Tait showed that quaternions had relevance to many problems in physics,[20] and he used them to describe the theoretical properties of "magnetic particles".[f] Tait's friend James Clerk Maxwell enigmatically called him the "Chief Musician upon Nabla"[28] and wrote favourably about the benefits of using quaternion notation for science:


What are called Maxwell's equations today are usually presented in a very different form to what was originally published in the first edition. Maxwell gave the main results in his Treatise on Electricity and Magnetism as twenty quaternion equations[29] as well as cartesian equations.[20] Maxwell later remarked to Tait that "The like of you may write everything and prove everything in pure 4nions, but in the transition period the bilingual method may help to introduce and explain the more perfect."[30] Though Maxwell expressed a strong liking of the ideas behind quaternions, he was somewhat dismayed by their lack of linear symmetry and hence complex practicality. He was also troubled by the fact that they led to results which were not homogenous, and the fact that the square of the velocity vector made the kinetic energy negative.[31]

 
Oliver Heaviside

Oliver Heaviside read Maxwell's Treatise in the 1870's where he came across the quaternion notation for the first time. He turned to the work of Tait to get a better understanding of the strange algebra, however he found that it was "without exception the hardest book to read I ever saw". Even after mastering the subject Heaviside was no fan of the algebra and was particularly troubled by the square of the vector being negative. He wrote


The work of William Thomson and Tait focused on potentials based on the principle of least action and Lagrangians;[g] Heaviside by contrast focused on what he coined the "principle of activity" through the use of local forces. He regarded the notion of force rather then potential as the best guide to understand local transformations of energy and give the best insight into the real workings of dynamical systems.[33] He saw the potentials as unphysical mathematical constructs that could have no observable effect in the context of electromagnetism. Heaviside developed the tools of vector analysis to help achieve this, and had great success in simplifying Maxwell's equations. Heaviside along with Josiah Willard Gibbs, John Henry Poynting, George Francis FitzGerald and Oliver Lodge significantly reformulated Maxwell's equations to make them more practical. They did this by ensuring that the potentials where symmetrical and scalar (and thus unobservable)[h] to ensure the E and B fields were topologically homogenous.

It is interesting to note that Nikola Tesla made use of quaternion notation. It is broadly accepted that he used a very different means of electrical engineering then that present in today's conventional circuits. It has been argued convincingly that due to the reactive (capacitive, etc.) coupling in his oscillating-shuttle-circuits (OSC), they cannot be analysed using standard distributed circuit frameworks. The OSC is more compatible with the physics of nonlinear optics and as it takes advantage of the nonlinear features of the quaternion   symmetry.[34][4]

It has sometimes been argued that quaternions present difficult issues of compatibility when describing space-time,[35] though models have been proposed.[i]

Dirac edit

 
Paul Dirac 1933

The discovery of the spin of the electron by to two Dutch scientists, George Uhlenbeck and Samuel Goudsmit, forced physicists to search for mathematical tools to describe, within the framework of quantum mechanics, this new degree of freedom.[37] In 1928 Paul Dirac argued that in order to do this he needed to find an equation for the electron in which the time-derivative appears in a first-order form   (rather then second order form  ). His reason for this was to ensure that the probability of finding an electron in any given time would be always positive, and thus the probability can never be negative. In order to do this he was forced to add non-commuting quantities to the equations; it was these non-commutative quantities that turned out to describe the physical spin of a particle. In finding non-commuting spin quantities, Dirac had inadvertently rediscovered an instance of Clifford algebra. Dirac appears to have been completely unaware of the work of Clifford and Hamilton before him. Clifford and Hamilton had noticed that non-commutative algebras can be used to "take the square root" of Laplacians, where the dimension is 4 and the signature  . Hamilton had shown that a square root of the ordinary 3-dimensional Laplacian can be obtained by using quaternions:[j][38]

 

Clifford generalised this idea for higher dimensions[k]

The Dirac equation with no external field is:

Dirac equation

 

Consider a global gauge transformation where   is a hermitian matrix and   a constant phase:

 

A necessary condition of the gauge invariance of the Dirac equation is that the factor does not depend on  , this is possible with two and only two matrices

Schwinger edit

Dirac, P. A. M. (1948). "The Theory of Magnetic Poles". Physical Review. 74 (7): 817–830. Bibcode:1948PhRv...74..817D. doi:10.1103/PhysRev.74.817. ISSN 0031-899X.
Schwinger, Julian (1966). "Magnetic Charge and Quantum Field Theory". Physical Review. 144 (4): 1087–1093. Bibcode:1966PhRv..144.1087S. doi:10.1103/PhysRev.144.1087. ISSN 0031-899X.
Schwinger, Julian (1966). "Electric- and Magnetic-Charge Renormalization. I". Physical Review. 151 (4): 1048–1054. Bibcode:1966PhRv..151.1048S. doi:10.1103/PhysRev.151.1048. ISSN 0031-899X.
Schwinger, Julian (1966). "Electric- and Magnetic-Charge Renormalization. II". Physical Review. 151 (4): 1055–1057. Bibcode:1966PhRv..151.1055S. doi:10.1103/PhysRev.151.1055. ISSN 0031-899X.
Schwinger, Julian (1966). "Magnetic Charge and Quantum Field Theory". Physical Review. 144 (4): 1087–1093. Bibcode:1966PhRv..144.1087S. doi:10.1103/PhysRev.144.1087. ISSN 0031-899X.
Schwinger, Julian (1968). "Sources and Magnetic Charge". Physical Review. 173 (5): 1536–1544. Bibcode:1968PhRv..173.1536S. doi:10.1103/PhysRev.173.1536. ISSN 0031-899X.
Schwinger, J. (1969). "A Magnetic Model of Matter". Science. 165 (3895): 757–761. Bibcode:1969Sci...165..757S. doi:10.1126/science.165.3895.757. ISSN 0036-8075. PMID 17742261.
Schwinger, Julian (1975). "Magnetic charge and the charge quantization condition". Physical Review D. 12 (10): 3105–3111. Bibcode:1975PhRvD..12.3105S. doi:10.1103/PhysRevD.12.3105. ISSN 0556-2821.

Magnetic photon edit

A. Salam (1966). "Magnetic monopole and two photon theories of C-violation". Physics Letters. 22 (5): 683–684. Bibcode:1966PhL....22..683S. doi:10.1016/0031-9163(66)90704-9.</ref>

Wu & Yang edit

Wu, T. T.; Yang, C. N. (1969). Mark, H.; Fernbach, S. (eds.). Properties of Matter under Unusual Conditions. New York: Interscience. pp. 349–354.
Wu, Tai Tsun; Yang, Chen Ning (1976). "Dirac monopole without strings: Monopole harmonics". Nuclear Physics B. 107 (3): 365–380. Bibcode:1976NuPhB.107..365W. doi:10.1016/0550-3213(76)90143-7. ISSN 0550-3213.
Wu, Tai Tsun; Yang, Chen Ning (1977). "Some properties of monopole harmonics". Physical Review D. 16 (4): 1018–1021. Bibcode:1977PhRvD..16.1018W. doi:10.1103/PhysRevD.16.1018. ISSN 0556-2821.

Weinberg-Salam model edit

't Hooft–Polyakov monopole edit

Montonen–Olive conjecture edit

Montonen, C.; Olive, D. (1977). "Magnetic monopoles as gauge particles?" (PDF). Physics Letters B. 72 (1): 117–120. Bibcode:1977PhLB...72..117M. doi:10.1016/0370-2693(77)90076-4. ISSN 0370-2693.
Goddard, P; Olive, D I (1978). "Magnetic monopoles in gauge field theories" (PDF). Reports on Progress in Physics. 41 (9): 1357–1437. Bibcode:1978RPPh...41.1357G. doi:10.1088/0034-4885/41/9/001. ISSN 0034-4885.

Nambu edit

Nambu, Y. (1977). "String-like configurations in the Weinberg-Salam theory". Nuclear Physics B. 130 (3): 505–515. Bibcode:1977NuPhB.130..505N. doi:10.1016/0550-3213(77)90252-8. ISSN 0550-3213.

Supersymmetry edit

Since the gauge field is Abelian, ∇⋅B = 0, and isolated magnetic monopoles are necessarily singular in semilocal models. The only way to make the singularity disappear is by embedding the theory in a larger non-Abelian theory which provides a regular core, or by putting the singularity behind an event horizon.

Gibbons, G.W.; Ortiz, M.E.; Ruiz Ruiz, F.; Samols, T.M. (1992). "Semi-local strings and monopoles". Nuclear Physics B. 385 (1–2): 127–144. arXiv:hep-th/9203023. Bibcode:1992NuPhB.385..127G. doi:10.1016/0550-3213(92)90097-U. ISSN 0550-3213.
Cho, Y.M.; Maison, D. (1997). "Monopole configuration in Weinberg-Salam model" (PDF). Physics Letters B. 391 (3–4): 360–365. arXiv:hep-th/9601028. Bibcode:1997PhLB..391..360C. doi:10.1016/S0370-2693(96)01492-X. ISSN 0370-2693.

For longer then a century it was believed that all physical theory could be derived from some unknown Theory of Everything. The Seiberg-Witten theory in 1994 changed that ideology profoundly. It is now believed that there is no unique fundamental theory, from which all the properties of the universe can be described based on reductive properties , but dualities that offer equivalent perspectives, each useful in different contexts.[39] Donaldson theory

Experiments edit

Stanford edit

Spin ice edit

 
FIGURE 3. The orientation of the magnetic moments (light blue arrows) considering a single tetrahedron within the spin ice state, as in Figure 2. Here, the magnetic moments obey the two-in, two-out rule: there is as much "magnetization field" going in the tetrahedron (bottom two arrows) as there is going out (top two arrows). The corresponding magnetization field has zero divergence. There is therefore no sink or source of the magnetization inside the tetrahedron, or no monopole. If a thermal fluctuation caused one of the bottom two magnetic moments to flip from "in" to "out", one would then have a 1-in, 3-out configuration; hence an "outflow' of magnetization, hence a positive divergence, that one could assign to a positively charged monopole of charge +Q. Flipping the two bottom magnetic moments would give a 0-in, 4-out configuration, the maximum possible "outflow" (i.e. divergence) of magnetization and, therefore, an associated monopole of charge +2Q.

Magnetricity edit

https://www.newscientist.com/article/dn17983-magnetricity-observed-for-first-time/

Mathematics edit

Electromagnetism can be placed in the broader context of Yang-Mills theory.[40]

A particle that conserves both magnetic and electric charge is known as a dyon and requires a greater symmetry group SU(2) to describe the preservation of magnetic symmetry. https://arxiv.org/abs/hep-th/9603086

Einstein insisted that all fundamental laws of nature could be understood in terms of geometry and symmetry.[41] Before 1980 all states of matter could be classified by the principle of symmetry breaking. The quantum Hall state provided the first example of a quantum state that had no spontaneously broken symmetry. Its behaviour depends only on its topology and not its specific geometry. The quantum Hall effect earned Klaus von Klitzing the Nobel Prize in Physics for 1985.[l] Though it was not understood at the time, the quantum Hall effect is an example of topological order, the subject of the 2016 Nobel Prize in Physics. Topological order violates the long-held belief that order in nature requires symmetry breaking. Fundamental aspects of nature can now also be understood in the context of topology, and physicists such as Edward Witten have developed topological field theory to develop this paradigm.[43]

when   is constant in eq. (13.2) and (13.4) it has been shown[m] that the presence of a monopole may be considered as a local torsion of an affine twisted space[n], the total curvature of which is ...[44]



Indirect empirical evidence of monopoles has been suggested in the form of particles that move in a helical motion in ferromagnetic aerosols.[o]

Instantons are topologically nontrivial solutions of Yang–Mills equations that absolutely minimize the energy functional within their topological type. The first such solutions were discovered in the case of four-dimensional Euclidean space compactified to the four-dimensional sphere, and turned out to be localized in space-time, prompting the names pseudoparticle and instanton.

Many methods developed in studying instantons have also been applied to monopoles. This is because magnetic monopoles arise as solutions of a dimensional reduction of the Yang–Mills equations.[45]

In the context of (classical) field theory, the partial differential equations are the field equations of the theory and the trivial solutions are the vacuum solutions, i.e. the solutions that minimise the energy[46]


an ordinary homotopy between two smooth functions is equivalent to the existence of a smooth homotopy.[47]


A dipole such as an electron above the surface of a topological insulator induces an emergent quasi-particle image magnetic monopole, known as a dyon, which is a composite of electric and magnetic charges.[p] This new particle obeys neither Bose nor Fermi statistics but behave like a so called anyon named as such because it is governed by with "any possible" statistics.[42]

An electromagnetic field which contains a magnetic monopole is not Lorentz invariant.[50]



Since the gauge field is Abelian, divB = 0, and isolated magnetic monopoles are necessarily singular in semilocal models. The only way to make the singularity disappear is by embedding the theory in a larger non-Abelian theory which provides a regular core, or by putting the singularity behind an event horizon.

Gibbons, G.W.; Ortiz, M.E.; Ruiz Ruiz, F.; Samols, T.M. (1992). "Semi-local strings and monopoles". Nuclear Physics B. 385 (1–2): 127–144. arXiv:hep-th/9203023. Bibcode:1992NuPhB.385..127G. doi:10.1016/0550-3213(92)90097-U. ISSN 0550-3213.
Cho, Y.M.; Maison, D. (1997). "Monopole configuration in Weinberg-Salam model" (PDF). Physics Letters B. 391 (3–4): 360–365. arXiv:hep-th/9601028. Bibcode:1997PhLB..391..360C. doi:10.1016/S0370-2693(96)01492-X. ISSN 0370-2693.

B-field edit

Anne-Christine Davis; Robert Brandenberger (6 December 2012). Formation and Interactions of Topological Defects: Proceedings of a NATO Advanced Study Institute on Formation and Interactions of Topological Defects, held August 22–September 2, 1994, in Cambridge, England. Springer Science & Business Media. ISBN 978-1-4615-1883-9.

Philosophy edit

Monopoles are everywhere - https://www.youtube.com/watch?v=seBwiL9InII&feature=youtu.be&t=48m14s

Ontology edit

References edit

Notes edit

  1. ^ See Aharonov & Bohm (1959). In fact, this idea had already been noted 10 years earlier by Ehrenberg & Siday (1949). It was experimentally verified by Chambers (1960) and then more convincingly by Tonomura et al. (1982, 1986)[5]
  2. ^ In particular, the usefulness of the Cauchy–Riemann equations which allow the Laplace equation to define holomorphic functions[16]
  3. ^ Carl Friedrich Gauss was actually first to discover quaternions in 1819 but the results were not published until after his death (Gauss 1900, pp. 357–362). Olinde Rodrigues also came across the results, published them in 1840, though this was largely ignored (Rodrigues 1840).[18] Hamilton wrote a letter to his friend John Graves on 16 October 1843, first published by McConnell (1943) and included in Hamilton (1967). Next day a final letter was written and sent, later published in the Philosophical Magazine (Hamilton 1844a). The November report to the Irish Academy was published almost at the same time (Hamilton 1844b)[19]
  4. ^ Clifford also combined ideas from the exterior algebra of Hermann Grassmann. The first announcement of the result was issued in a talk in 1876, which was published in 1882 after Clifford's death (Clifford 1882, pp. 397–401). The first publication of the invention came out in another paper in 1878 (Clifford 1878).[23]
  5. ^ Abel was born in 1802 and died of tuberculosis in 1829, aged 28. The more general non-abelian group theory (abba) was introduced by the even more tragically short-lived French mathematician Évariste Galois (1811-1832), who was killed in a dual at the age of 20 having been up the previous night writing down his revolutionary ideas that involve the use of groups to investigate the solubility of algebraic equations, now called Galois theory[25]
  6. ^ See Tait (1867), p. 310. Tait wrote on December 1867 to Maxwell "If you read the last 20 or 30 pages of my book [Treatise on Quaternions] I think you will see that 4ions are worth getting up, for there it is shown that they go into that ∇ business like greased lightning. Unfortunately I cannot find time to work steadily at them..."[27]
  7. ^ For a historical review of Thomson & Tait (1867) see Smith & Wise (1989), pp. 348–398
  8. ^ See Noether theorem for more information on the relation between symmetry and observables
  9. ^ See for example Rocher (1972), Imaeda (1976) and Kauffmann & Sun (1993)[36]
  10. ^ See Trautman (1997) for a reference on these square root ideas
  11. ^ See Clifford (1882), pp. 778–815; see also Lounesto (2001) for general treatment
  12. ^ See von Klitzing et al. (1980)[42]
  13. ^ See Lochak (1985, 1987) who builds on an older work of Rodichev (1961)
  14. ^ See Einstein–Cartan theory
  15. ^ See Mikhailov (1985)[4] and Mikhailov (1991)[4]
  16. ^ See Ray et al. (2014)[48] and Ray et al. (2015)[49]

Citations edit

  1. ^ Nikolić 2014, p. 8.
  2. ^ Baarsma 2009, p. 13.
  3. ^ Rehn & Moessne 2016, p. 1.
  4. ^ a b c d Reed 1995, p. 242.
  5. ^ Penrose, p. 453-454, 469.
  6. ^ Chan & Tsou 1993, p. 5.
  7. ^ Curie 1894.
  8. ^ Poincaré 1896.
  9. ^ Birkeland 1986.
  10. ^ Milton 2006, p. 2.
  11. ^ Thomson 1909, p. 532.
  12. ^ Thomson 1937, pp. 370–371.
  13. ^ Adawi 1976.
  14. ^ Villard 1905.
  15. ^ Kragh 1990, p. 206.
  16. ^ Penrose 2005, pp. 193–196.
  17. ^ Penrose 2005, p. 198.
  18. ^ Altmann 1989, p. 306.
  19. ^ Altmann 1989, p. 297.
  20. ^ a b c Hunt 2005, p. 105.
  21. ^ Penrose 2005, p. 199.
  22. ^ Altmann 1989, p. 296.
  23. ^ Lounesto 2001, p. 9.
  24. ^ Lounesto 2001, p. 321.
  25. ^ Penrose 2005, pp. 248, 289.
  26. ^ Crowe 1967, p. 118.
  27. ^ Crowe 1967, p. 132.
  28. ^ Crowe 1967, p. 250.
  29. ^ Barrett 2008, p. 8.
  30. ^ Crowe 1967, p. 137.
  31. ^ Crowe, p. 139.
  32. ^ Hunt 2006, pp. 105–106.
  33. ^ Hunt 2005, pp. 122–123.
  34. ^ Barrett 1991.
  35. ^ Penrose 2005, p. 201.
  36. ^ Reed 1995, p. 241.
  37. ^ Trautman 1997, p. 3.
  38. ^ Penrose 2005, pp. 618–619.
  39. ^ Shnir 2006, pp. 465=466.
  40. ^ Roussel-Dupré & Barrett 1994, p. 366.
  41. ^ Qi & Zhang 2010, p. 38.
  42. ^ a b Qi & Zhang 2010, p. 33.
  43. ^ Witten 1988.
  44. ^ Lochak 1995, p. 143.
  45. ^ Hitchin 1987, p. 1.
  46. ^ Baarsma 2009, p. 9.
  47. ^ Hirsch 1976, sec 8.2.
  48. ^ Amherst College 2014; Morgan 2014.
  49. ^ Aalto University 2015.
  50. ^ Hagen 1965.

Bibliography edit