Диссертация (1150860), страница 15
Текст из файла (страница 15)
Andrianov and D. Espriu, Phys. Lett. B(2009); Eur. Phys. J. C74,678,4162932 (2014).9. M. Ibe, S. Iwamoto, S. Matsumoto, T. Moroi and N. Yokozaki, JHEP1308,029 (2013) doi:10.1007/JHEP08(2013)029 [arXiv:1304.1483 [hep-ph]].10. O. Adriani et al. [PAMELA Collaboration], An anomalous positron102abundance in cosmic rays with energies 1.5-100 GeV, Nature458(2009)607 [arXiv:0810.4995 [astro-ph]].11. A. A. Abdo et al. [Fermi LAT Collaboration], Measurement of the CosmicRay e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi LargeArea Telescope, Phys.
Rev. Lett. 102 (2009) 181101 [arXiv:0905.0025 [astroph.HE]].12. D. Hooper, P. Blasi and P. D. Serpico, Pulsars as the Sources of High EnergyCosmic Ray Positrons, JCAP0901(2009) 025 [arXiv:0810.1527 [astro-ph]].13. P. Sikivie, An argument that the dark matter is axions, arXiv:1210.0040[astro-ph.CO].14. A. Arvanitaki and S. Dubovsky, Exploring the String Axiverse with PrecisionBlack Hole Physics, Phys. Rev. D83(2011) 044026 [arXiv:1004.3558 [hepth]].15. F.
E. Schunck and E. W. Mielke, General relativistic boson stars, Class.Quant. Grav.20(2003) R301 [arXiv:0801.0307 [astro-ph]].16. A. A. Andrianov, D. Espriu, P. Giacconi and R. Soldati, JHEP0909,057(2009) doi:10.1088/1126-6708/2009/09/057 [arXiv:0907.3709 [hep-ph]].17.
A. A. Andrianov, D. Espriu, F. Mescia and A. Renau, The Axion shield,Phys. Lett. B684(2010) 101 [arXiv:0912.3151 [hep-ph]].18. A. A. Andrianov, R. Soldati, Phys. Rev. D51,5961 (1995).19. V. A. Kostelecky, M. Mewes, Phys. Rev. D66,056005 (2002).20. G. M. Shore, Contemp. Phys.44,503 (2003).10321. N. Arkani-Hamed, H. C. Cheng, M. A. Luty, S. Mukohyama, JHEP0405,074 (2004);H. C. Cheng, M. A.
Luty, S. Mukohyama, J. Thaler, JHEP 0605, 076 (2006).22. J. Eby, P. Suranyi, C. Vaz, and L.C.R. Wijewardhana, arXiv: 1412.3430v2;A. Iwazaki, arXiv:1412.7825; Phys. Rev. D 91, 023008 (2015); P.H. Chavanis,arXiv:1412.0005.23. Grigory E.
Volovik, The Universe in a Helium Droplet, Clarendon Press,Oxford (2003) 530 pp.; JEPT Letters70(1999) 1.24. Leon Balents, Weyl Electron Kiss, Physics4(2011) 36.25. A. A. Burkov and L. Balents, Phys. Rev. Lett.107(2011) no.12, 127205.doi:10.1103/PhysRevLett.107.12720526. A.G.Grushin,Phys.Rev.D86,045001(2012)doi:10.1103/PhysRevD.86.045001 [arXiv:1205.3722 [hep-th]].27.
P. Goswami and S. Tewari, Axionic eld theory of (3+1)-dimensional Weylsemimetals, Phys. Rev. B 88 (2013) 245107.28. A.A. Burkov, Chiral anomaly and transport in Weyl metals, J. Phys. Condens.Matter29. R.27(2015) 113201; arXiv:1502.07609v1 [cond-mat.mes-hall].B.Laughlin,Phys.Rev.Lett.50,1395(1983).doi:10.1103/PhysRevLett.50.139530. A. A. Andrianov, P. Giacconi and R. Soldati, JHEP0202,030 (2002)doi:10.1088/1126-6708/2002/02/030 [hep-th/0110279].31. B.KorsandP.Nath,JHEP0507,doi:10.1088/1126-6708/2005/07/069 [hep-ph/0503208].069(2005)10432.
N. N. Bogolyubov, Sov. Phys. JETP 7, 41 (1958) [Zh. Eksp. Teor. Fiz.34,58 (1958)] [Front. Phys. 6, 399 (1961)].33. A. A. Andrianov, S. S. Kolevatov and R. Soldati, JHEP1111,007 (2011)doi:10.1007/JHEP11(2011)007 [arXiv:1109.3440 [hep-ph]].34. A. A. Andrianov and S. S. Kolevatov, Theor. Math. Phys.(2013) [Teor. Mat. Fiz.175,175,744357 (2013)] doi:10.1007/s11232-013-0060-y[arXiv:1212.5723 [hep-ph]].35. A. A. Andrianov, S. S. Kolevatov and R. Soldati, Teor. Mat.
Fiz.no. 3, 367-379 (2015) [Theor. Math. Phys.184,184,no. 3, 1213 (2015)].doi:10.1007/s11232-015-0329-436. A. A. Andrianov, D. Espriu and S. S. Kolevatov, Teor. Mat. Fiz.184,no. 3, 392 (2015) [Theor. Math. Phys.184,no. 3, 1234 (2015)].doi:10.1007/s11232-015-0330-y37. S. S. Kolevatov and A. A.
Andrianov, AIP Conf. Proc.1606,243 (2014).doi:10.1063/1.489114038. A. A. Andrianov, V. A. Andrianov, D. Espriu and S. S. Kolevatov,Eur. Phys. J. C76,no. 3, 169 (2016) doi:10.1140/epjc/s10052-016-4012-1[arXiv:1507.07087 [hep-ph]].39. S. S. Kolevatov, A. A. Andrianov and D. Espriu, AIP Conf. Proc.1701,080006 (2016). doi:10.1063/1.493869540. S. Kolevatov and A. Andrianov, PoS QFTHEP41. S.
Weinberg, Phys. Rev. D11,42. G. 't Hooft, Phys. Rev. Lett.G. 't Hooft, Phys. Rev. D064 (2013).3583 (1975). doi:10.1103/PhysRevD.11.358337,14,2013,8 (1976). doi:10.1103/PhysRevLett.37.83432 (1976) Erratum: [Phys. Rev. D18,(1978)]. doi:10.1103/PhysRevD.18.2199.3, 10.1103/PhysRevD.14.3432219910543. S. L. Adler, Phys. Rev.J.S.Belland177,R.2426 (1969). doi:10.1103/PhysRev.177.2426Jackiw,NuovoCim.A60,47(1969).doi:10.1007/BF02823296W. A.
Bardeen, Phys. Rev.44. W.A.Bardeen,184,1848 (1969). doi:10.1103/PhysRev.184.1848Nucl.Phys.B75,246(1974).doi:10.1016/0550-3213(74)90546-X45. C. G. Callan, Jr., R. F. Dashen and D. J. Gross, Phys. Lett. B 63, 334 (1976).doi:10.1016/0370-2693(76)90277-X46. V. Baluni, Phys.
Rev. D19,2227 (1979). doi:10.1103/PhysRevD.19.2227R. J. Crewther, P. Di Vecchia, G. Veneziano and E. Witten, Phys.Lett. B88,123 (1979) Erratum: [Phys. Lett. B91,487 (1980)].doi:10.1016/0370-2693(80)91025-4, 10.1016/0370-2693(79)90128-X47. J. M. Pendlebury et al., Phys. Rev. D92,no. 9, 092003 (2015)doi:10.1103/PhysRevD.92.092003 [arXiv:1509.04411 [hep-ex]].48. R.JackiwandC.Rebbi,Phys.Rev.Lett.37,172(1976).doi:10.1103/PhysRevLett.37.17249. R. D.
Peccei and H. R. Quinn, Phys. Rev. Lett.38,1440 (1977).doi:10.1103/PhysRevLett.38.1440R. D. Peccei and H. R. Quinn, Phys. Rev. D16,1791 (1977).doi:10.1103/PhysRevD.16.179150. S.Weinberg,Phys.Rev.Lett.40,223(1978).doi:10.1103/PhysRevLett.40.223F. Wilczek, Phys. Rev. Lett. 40, 279 (1978). doi:10.1103/PhysRevLett.40.27951. W.
A. Bardeen, S.-H. H. Tye and J. A. M. Vermaseren, Phys. Lett. B 76, 580(1978). doi:10.1016/0370-2693(78)90859-610652. W. A. Bardeen, R. D. Peccei and T. Yanagida, Nucl. Phys. B 279, 401 (1987).doi:10.1016/0550-3213(87)90003-453. Y.etAsanoal.,Phys.Lett.B107,159(1981).doi:10.1016/0370-2693(81)91172-254. J.
E. Kim, Phys. Rev. Lett.43,103 (1979). doi:10.1103/PhysRevLett.43.10355. M. A. Shifman, A. I. Vainshtein and V. I. Zakharov, Nucl. Phys. B166,493(1980). doi:10.1016/0550-3213(80)90209-656. M. Dine, W. Fischler and M. Srednicki, Phys. Lett. B104(1981) 199.doi:10.1016/0370-2693(81)90590-657. A. R. Zhitnitsky, Sov. J. Nucl. Phys. 31, 260 (1980) [Yad. Fiz.
31, 497 (1980)].58. K. A. Olive et al. [Particle Data Group Collaboration], Chin. Phys. C38,090001 (2014). doi:10.1088/1674-1137/38/9/09000159. M. Giannotti, I. Irastorza, J. Redondo and A. Ringwald, arXiv:1512.08108[astro-ph.HE].60. J. Preskill, M. B. Wise and F. Wilczek, Phys. Lett. B120,127 (1983).doi:10.1016/0370-2693(83)90637-8L.F.AbbottandP.Sikivie,Phys.Lett.B120,133(1983).137(1983).doi:10.1016/0370-2693(83)90638-XM.DineandW.Fischler,Phys.Lett.B120,doi:10.1016/0370-2693(83)90639-161. P.
Fox, A. Pierce and S. D. Thomas, hep-th/0409059.62. P. A. R. Ade et al. [Planck Collaboration], arXiv:1502.01589 [astro-ph.CO].63. K. van Bibber, P. M. McIntyre, D. E. Morris and G. G. Raelt, Phys. Rev.D39,2089 (1989). doi:10.1103/PhysRevD.39.208910764. E.Ariket al. [CAST Collaboration], JCAP0902,008(2009)doi:10.1088/1475-7516/2009/02/008 [arXiv:0810.4482 [hep-ex]].65.
I.G.Irastorzaetal.,JCAP1106,013(2011)doi:10.1088/1475-7516/2011/06/013 [arXiv:1103.5334 [hep-ex]].66. G. W. Fraser, A. M. Read, S. Sembay, J. A. Carter and E. Schyns, Mon.Not. Roy. Astron. Soc.445,no. 2, 2146 (2014) doi:10.1093/mnras/stu1865[arXiv:1403.2436 [astro-ph.HE]].67. S. J. Asztalos et al. [ADMX Collaboration], Nucl. Instrum.
Meth. A656,39(2011) doi:10.1016/j.nima.2011.07.019 [arXiv:1105.4203 [physics.ins-det]].68. R. Ballou et al., arXiv:1410.2566 [hep-ex].69. R. Bahre et al., JINST 8, T09001 (2013) doi:10.1088/1748-0221/8/09/T09001[arXiv:1302.5647 [physics.ins-det]].70. E. Zavattini et al. [PVLAS Collaboration], Phys.
Rev. Lett.110406(2006)Erratum:[Phys.Rev.Lett.99,12990196,(2007)]doi:10.1103/PhysRevLett.99.129901, 10.1103/PhysRevLett.96.110406 [hepex/0507107].71. A. A. Belavin, A. M. Polyakov, A. S. Schwartz and Y. S. Tyupkin, Phys. Lett.B59,85 (1975). doi:10.1016/0370-2693(75)90163-X72. F. R. Klinkhamer and N. S. Manton, Phys. Rev.
![](https://s.studizba.com/z.php?f=/templates/si/i/noavatar.png&w=100&h=100&t=1"){kind=avatar}
