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Schwinger limit

In quantum electrodynamics (QED), the Schwinger limit is a scale above which the electromagnetic field is expected to become nonlinear. The limit was first derived in one of QED's earliest theoretical successes by Fritz Sauter in 1931[1] and discussed further by Werner Heisenberg and his student Hans Heinrich Euler.[2] The limit, however, is commonly named in the literature[3] for Julian Schwinger, who derived the leading nonlinear corrections to the fields and calculated the rate of electron–positron pair production in a strong electric field.[4] The limit is typically reported as a maximum electric field or magnetic field before nonlinearity for the vacuum of

A Feynman diagram (box diagram) for photon–photon scattering; one photon scatters from the transient vacuum charge fluctuations of the other.

where me is the mass of the electron, c is the speed of light in vacuum, qe is the elementary charge, and ħ is the reduced Planck constant. These are enormous field strengths. Such an electric field is capable of accelerating a proton from rest to the maximum energy attained by protons at the Large Hadron Collider in only approximately 5 micrometers. The magnetic field is associated with birefringence of the vacuum and is exceeded on magnetars.

In vacuum, the classical Maxwell's equations are perfectly linear differential equations. This implies – by the superposition principle – that the sum of any two solutions to Maxwell's equations is another solution to Maxwell's equations. For example, two intersecting beams of light should simply add together their electric fields and pass right through each other. Thus Maxwell's equations predict the impossibility of any but trivial elastic photon–photon scattering. In QED, however, non-elastic photon–photon scattering becomes possible when the combined energy is large enough to create virtual electron–positron pairs spontaneously, illustrated by the Feynman diagram in the adjacent figure. This creates nonlinear effects that are approximately described by Euler and Heisenberg's nonlinear variant of Maxwell's equations.

A single plane wave is insufficient to cause nonlinear effects, even in QED.[4] The basic reason for this is that a single plane wave of a given energy may always be viewed in a different reference frame, where it has less energy (the same is the case for a single photon). A single wave or photon does not have a center-of-momentum frame where its energy must be at minimal value. However, two waves or two photons not traveling in the same direction always have a minimum combined energy in their center-of-momentum frame, and it is this energy and the electric field strengths associated with it, which determine particle–antiparticle creation, and associated scattering phenomena.

Photon–photon scattering and other effects of nonlinear optics in vacuum is an active area of experimental research, with current or planned technology beginning to approach the Schwinger limit.[5] It has already been observed through inelastic channels in SLAC Experiment 144.[6][7] However, the direct effects in elastic scattering have not been observed. As of 2012, the best constraint on the elastic photon–photon scattering cross section belonged to PVLAS, which reported an upper limit far above the level predicted by the Standard Model.[8]

Proposals were made to measure elastic light-by-light scattering using the strong electromagnetic fields of the hadrons collided at the LHC.[9] In 2019, the ATLAS experiment at the LHC announced the first definitive observation of photon–photon scattering, observed in lead ion collisions that produced fields as large as 1025 V/m, well in excess of the Schwinger limit.[10] Observation of a cross section larger or smaller than that predicted by the Standard Model could signify new physics such as axions, the search of which is the primary goal of PVLAS and several similar experiments. ATLAS observed more events than expected, potentially evidence that the cross section is larger than predicted by the Standard Model, but the excess is not yet statistically significant.[11]

The planned, funded ELI–Ultra High Field Facility, which will study light at the intensity frontier, is likely to remain well below the Schwinger limit[12] although it may still be possible to observe some nonlinear optical effects.[13] The Station of Extreme Light (SEL) is another laser facility under construction which should be powerful enough to observe the effect.[14] Such an experiment, in which ultra-intense light causes pair production, has been described in the popular media as creating a "hernia" in spacetime.[15]

See also edit

References edit

  1. ^ F. Sauter (1931). "Über das Verhalten eines Elektrons im homogenen elektrischen Feld nach der relativistischen Theorie Diracs". Zeitschrift für Physik (82nd ed.) (published November 1931). 69 (11–12): 742–764. Bibcode:1931ZPhy...69..742S. doi:10.1007/BF01339461. ISSN 1434-6001. S2CID 122120733. Wikidata Q60698281.
  2. ^ Werner Heisenberg; Hans Heinrich Euler (1936). "Folgerungen aus der Diracschen Theorie des Positrons". Zeitschrift für Physik (in German) (98th ed.) (published November 1936). 98 (11–12): 714–732. Bibcode:1936ZPhy...98..714H. doi:10.1007/BF01343663. ISSN 1434-6001. S2CID 120354480. Wikidata Q28794438. English translation
  3. ^ Mark Buchanan (2006). "Thesis: Past the Schwinger limit". Nature Physics (2nd ed.) (published November 2006). 2 (11): 721. Bibcode:2006NatPh...2..721B. doi:10.1038/nphys448. ISSN 1745-2473. S2CID 119831515. Wikidata Q63918589.
  4. ^ a b J. Schwinger (1951). "On Gauge Invariance and Vacuum Polarization". Phys. Rev. (82nd ed.) (published June 1951). 82 (5): 664–679. Bibcode:1951PhRv...82..664S. doi:10.1103/PhysRev.82.664. ISSN 0031-899X. Wikidata Q21709192.
  5. ^ Stepan S Bulanov; Timur Esirkepov; Alexander G. Thomas; James K Koga; Sergei V Bulanov (2010). "On the Schwinger limit attainability with extreme power lasers". Phys. Rev. Lett. (105th ed.) (published 24 November 2010). 105 (22): 220407. arXiv:1007.4306. doi:10.1103/PhysRevLett.105.220407. ISSN 0031-9007. PMID 21231373. S2CID 36857911. Wikidata Q27447776.
  6. ^ C. Bula; K. T. McDonald; E. J. Prebys; et al. (1996). "Observation of Nonlinear Effects in Compton Scattering". Phys. Rev. Lett. (76th ed.) (published 22 April 1996). 76 (17): 3116–3119. Bibcode:1996PhRvL..76.3116B. doi:10.1103/PhysRevLett.76.3116. ISSN 0031-9007. PMID 10060879. Wikidata Q27450530.
  7. ^ C. Bamber; S. J. Boege; T. Koffas; et al. (1999). "Studies of nonlinear QED in collisions of 46.6 GeV electrons with intense laser pulses". Phys. Rev. D (60th ed.) (published 8 October 1999). 60 (9): 092004. Bibcode:1999PhRvD..60i2004B. doi:10.1103/PhysRevD.60.092004. ISSN 1550-7998. Wikidata Q27441586.
  8. ^ G. ZAVATTINI; U. GASTALDI; R. PENGO; G. RUOSO; F. DELLA VALLE; E. MILOTTI (20 June 2012). "Measuring the magnetic birefringence of vacuum: the PVLAS experiment". International Journal of Modern Physics A. 27 (15): 1260017. arXiv:1201.2309. doi:10.1142/S0217751X12600172. ISSN 0217-751X. Wikidata Q62555414.
  9. ^ David d'Enterria; Gustavo G da Silveira (2013). "Observing Light-by-Light Scattering at the Large Hadron Collider". Phys. Rev. Lett. (111th ed.) (published 22 August 2013). 111 (8): 080405. arXiv:1305.7142. Bibcode:2013PhRvL.111h0405D. doi:10.1103/PhysRevLett.111.080405. ISSN 0031-9007. PMID 24010419. S2CID 43797550. Wikidata Q85643997.
  10. ^ ATLAS Collaboration (17 March 2019). "ATLAS observes light scattering off light".
  11. ^ G. Aad; et al. (31 July 2019). "Observation of Light-by-Light Scattering in Ultraperipheral Pb+Pb Collisions with the ATLAS Detector". Physical Review Letters. 123 (5): 052001. arXiv:1904.03536. Bibcode:2019PhRvL.123e2001A. doi:10.1103/PhysRevLett.123.052001. PMID 31491300. S2CID 260811101.
  12. ^ Heinzl, T. (2012). "Strong-Field QED and High Power Lasers" (PDF). International Journal of Modern Physics A. 27 (15). arXiv:1111.5192. Bibcode:2012IJMPA..2760010H. doi:10.1142/S0217751X1260010X. S2CID 119198507.
  13. ^ Gagik Yu Kryuchkyan; Karen Z. Hatsagortsyan (2011). "Bragg Scattering of Light in Vacuum Structured by Strong Periodic Fields". Phys. Rev. Lett. (107th ed.) (published 27 July 2011). 107 (5): 053604. arXiv:1102.4013. Bibcode:2011PhRvL.107e3604K. doi:10.1103/PhysRevLett.107.053604. ISSN 0031-9007. PMID 21867070. S2CID 25991919. Wikidata Q27347258.
  14. ^ Berboucha, Meriame. "This Laser Could Rip Apart Empty Space". Forbes. Retrieved 2021-02-18.
  15. ^ I. O'Neill (2011). . Discovery News. Archived from the original on November 3, 2011.

schwinger, limit, quantum, electrodynamics, scale, above, which, electromagnetic, field, expected, become, nonlinear, limit, first, derived, earliest, theoretical, successes, fritz, sauter, 1931, discussed, further, werner, heisenberg, student, hans, heinrich,. In quantum electrodynamics QED the Schwinger limit is a scale above which the electromagnetic field is expected to become nonlinear The limit was first derived in one of QED s earliest theoretical successes by Fritz Sauter in 1931 1 and discussed further by Werner Heisenberg and his student Hans Heinrich Euler 2 The limit however is commonly named in the literature 3 for Julian Schwinger who derived the leading nonlinear corrections to the fields and calculated the rate of electron positron pair production in a strong electric field 4 The limit is typically reported as a maximum electric field or magnetic field before nonlinearity for the vacuum ofA Feynman diagram box diagram for photon photon scattering one photon scatters from the transient vacuum charge fluctuations of the other E c m e 2 c 3 q e ℏ 1 32 10 18 V m displaystyle E text c frac m text e 2 c 3 q text e hbar simeq 1 32 times 10 18 mathrm V mathrm m B c m e 2 c 2 q e ℏ 4 41 10 9 T displaystyle B text c frac m text e 2 c 2 q text e hbar simeq 4 41 times 10 9 mathrm T where me is the mass of the electron c is the speed of light in vacuum qe is the elementary charge and ħ is the reduced Planck constant These are enormous field strengths Such an electric field is capable of accelerating a proton from rest to the maximum energy attained by protons at the Large Hadron Collider in only approximately 5 micrometers The magnetic field is associated with birefringence of the vacuum and is exceeded on magnetars In vacuum the classical Maxwell s equations are perfectly linear differential equations This implies by the superposition principle that the sum of any two solutions to Maxwell s equations is another solution to Maxwell s equations For example two intersecting beams of light should simply add together their electric fields and pass right through each other Thus Maxwell s equations predict the impossibility of any but trivial elastic photon photon scattering In QED however non elastic photon photon scattering becomes possible when the combined energy is large enough to create virtual electron positron pairs spontaneously illustrated by the Feynman diagram in the adjacent figure This creates nonlinear effects that are approximately described by Euler and Heisenberg s nonlinear variant of Maxwell s equations A single plane wave is insufficient to cause nonlinear effects even in QED 4 The basic reason for this is that a single plane wave of a given energy may always be viewed in a different reference frame where it has less energy the same is the case for a single photon A single wave or photon does not have a center of momentum frame where its energy must be at minimal value However two waves or two photons not traveling in the same direction always have a minimum combined energy in their center of momentum frame and it is this energy and the electric field strengths associated with it which determine particle antiparticle creation and associated scattering phenomena Photon photon scattering and other effects of nonlinear optics in vacuum is an active area of experimental research with current or planned technology beginning to approach the Schwinger limit 5 It has already been observed through inelastic channels in SLAC Experiment 144 6 7 However the direct effects in elastic scattering have not been observed As of 2012 the best constraint on the elastic photon photon scattering cross section belonged to PVLAS which reported an upper limit far above the level predicted by the Standard Model 8 Proposals were made to measure elastic light by light scattering using the strong electromagnetic fields of the hadrons collided at the LHC 9 In 2019 the ATLAS experiment at the LHC announced the first definitive observation of photon photon scattering observed in lead ion collisions that produced fields as large as 1025 V m well in excess of the Schwinger limit 10 Observation of a cross section larger or smaller than that predicted by the Standard Model could signify new physics such as axions the search of which is the primary goal of PVLAS and several similar experiments ATLAS observed more events than expected potentially evidence that the cross section is larger than predicted by the Standard Model but the excess is not yet statistically significant 11 The planned funded ELI Ultra High Field Facility which will study light at the intensity frontier is likely to remain well below the Schwinger limit 12 although it may still be possible to observe some nonlinear optical effects 13 The Station of Extreme Light SEL is another laser facility under construction which should be powerful enough to observe the effect 14 Such an experiment in which ultra intense light causes pair production has been described in the popular media as creating a hernia in spacetime 15 See also editJulian Schwinger Schwinger effect Sokolov Ternov effect Vacuum polarizationReferences edit F Sauter 1931 Uber das Verhalten eines Elektrons im homogenen elektrischen Feld nach der relativistischen Theorie Diracs Zeitschrift fur Physik 82nd ed published November 1931 69 11 12 742 764 Bibcode 1931ZPhy 69 742S doi 10 1007 BF01339461 ISSN 1434 6001 S2CID 122120733 Wikidata Q60698281 Werner Heisenberg Hans Heinrich Euler 1936 Folgerungen aus der Diracschen Theorie des Positrons Zeitschrift fur Physik in German 98th ed published November 1936 98 11 12 714 732 Bibcode 1936ZPhy 98 714H doi 10 1007 BF01343663 ISSN 1434 6001 S2CID 120354480 Wikidata Q28794438 English translation Mark Buchanan 2006 Thesis Past the Schwinger limit Nature Physics 2nd ed published November 2006 2 11 721 Bibcode 2006NatPh 2 721B doi 10 1038 nphys448 ISSN 1745 2473 S2CID 119831515 Wikidata Q63918589 a b J Schwinger 1951 On Gauge Invariance and Vacuum Polarization Phys Rev 82nd ed published June 1951 82 5 664 679 Bibcode 1951PhRv 82 664S doi 10 1103 PhysRev 82 664 ISSN 0031 899X Wikidata Q21709192 Stepan S Bulanov Timur Esirkepov Alexander G Thomas James K Koga Sergei V Bulanov 2010 On the Schwinger limit attainability with extreme power lasers Phys Rev Lett 105th ed published 24 November 2010 105 22 220407 arXiv 1007 4306 doi 10 1103 PhysRevLett 105 220407 ISSN 0031 9007 PMID 21231373 S2CID 36857911 Wikidata Q27447776 C Bula K T McDonald E J Prebys et al 1996 Observation of Nonlinear Effects in Compton Scattering Phys Rev Lett 76th ed published 22 April 1996 76 17 3116 3119 Bibcode 1996PhRvL 76 3116B doi 10 1103 PhysRevLett 76 3116 ISSN 0031 9007 PMID 10060879 Wikidata Q27450530 C Bamber S J Boege T Koffas et al 1999 Studies of nonlinear QED in collisions of 46 6 GeV electrons with intense laser pulses Phys Rev D 60th ed published 8 October 1999 60 9 092004 Bibcode 1999PhRvD 60i2004B doi 10 1103 PhysRevD 60 092004 ISSN 1550 7998 Wikidata Q27441586 G ZAVATTINI U GASTALDI R PENGO G RUOSO F DELLA VALLE E MILOTTI 20 June 2012 Measuring the magnetic birefringence of vacuum the PVLAS experiment International Journal of Modern Physics A 27 15 1260017 arXiv 1201 2309 doi 10 1142 S0217751X12600172 ISSN 0217 751X Wikidata Q62555414 David d Enterria Gustavo G da Silveira 2013 Observing Light by Light Scattering at the Large Hadron Collider Phys Rev Lett 111th ed published 22 August 2013 111 8 080405 arXiv 1305 7142 Bibcode 2013PhRvL 111h0405D doi 10 1103 PhysRevLett 111 080405 ISSN 0031 9007 PMID 24010419 S2CID 43797550 Wikidata Q85643997 ATLAS Collaboration 17 March 2019 ATLAS observes light scattering off light G Aad et al 31 July 2019 Observation of Light by Light Scattering in Ultraperipheral Pb Pb Collisions with the ATLAS Detector Physical Review Letters 123 5 052001 arXiv 1904 03536 Bibcode 2019PhRvL 123e2001A doi 10 1103 PhysRevLett 123 052001 PMID 31491300 S2CID 260811101 Heinzl T 2012 Strong Field QED and High Power Lasers PDF International Journal of Modern Physics A 27 15 arXiv 1111 5192 Bibcode 2012IJMPA 2760010H doi 10 1142 S0217751X1260010X S2CID 119198507 Gagik Yu Kryuchkyan Karen Z Hatsagortsyan 2011 Bragg Scattering of Light in Vacuum Structured by Strong Periodic Fields Phys Rev Lett 107th ed published 27 July 2011 107 5 053604 arXiv 1102 4013 Bibcode 2011PhRvL 107e3604K doi 10 1103 PhysRevLett 107 053604 ISSN 0031 9007 PMID 21867070 S2CID 25991919 Wikidata Q27347258 Berboucha Meriame This Laser Could Rip Apart Empty Space Forbes Retrieved 2021 02 18 I O Neill 2011 A Laser to Give the Universe a Hernia Discovery News Archived from the original on November 3 2011 Retrieved from https en wikipedia org w index php title Schwinger limit amp oldid 1170885323, wikipedia, wiki, book, books, library,

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