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Stability of cylindrical thin shell wormhole during evolution of universe from inflation to late time acceleration

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Regular Article - Theoretical Physics
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Abstract

In this paper, we consider the stability of cylindrical wormholes during evolution of universe from inflation to late time acceleration epochs. We show that there are two types of cylindrical wormholes. The first type is produced at the corresponding point where k black F-strings are transited to BIon configuration. This wormhole transfers energy from extra dimensions into our universe, causes inflation, loses it’s energy and vanishes. The second type of cylindrical wormhole is created by a tachyonic potential and causes a new phase of acceleration. We show that wormhole parameters grow faster than the scale factor in this era, overtake it at ripping time and lead to the destruction of universe at big rip singularity.

Keywords

Strings and branes phenomenology Phenomenology of Large extra dimensions 
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References

  1. [1]
    A. Einstein and N. Rosen, The Particle Problem in the General Theory of Relativity, Phys. Rev. 48 (1935) 73 [INSPIRE].CrossRefADSGoogle Scholar
  2. [2]
    M.S. Morris and K.S. Thorne, Wormholes in space-time and their use for interstellar travel: A tool for teaching general relativity, Am. J. Phys. 56 (1988) 395 [INSPIRE].CrossRefADSMATHMathSciNetGoogle Scholar
  3. [3]
    M. Visser, Traversable wormholes: Some simple examples, Phys. Rev. D 39 (1989) 3182 [arXiv:0809.0907] [INSPIRE].ADSMathSciNetGoogle Scholar
  4. [4]
    M. Visser, Traversable wormholes from surgically modified Schwarzschild space-times, Nucl. Phys. B 328 (1989) 203 [arXiv:0809.0927] [INSPIRE].CrossRefADSMathSciNetGoogle Scholar
  5. [5]
    M. Visser, Lorentzian Wormholes — from Einstein to Hawking, American Institute of Physics, New York, U.S.A. (1995).Google Scholar
  6. [6]
    G. Grignani, T. Harmark, A. Marini, N.A. Obers and M. Orselli, Heating up the BIon, JHEP 06 (2011) 058 [arXiv:1012.1494] [INSPIRE].CrossRefADSGoogle Scholar
  7. [7]
    G. Grignani, T. Harmark, A. Marini, N.A. Obers and M. Orselli, Thermodynamics of the hot BIon, Nucl. Phys. B 851 (2011) 462 [arXiv:1101.1297] [INSPIRE].CrossRefADSGoogle Scholar
  8. [8]
    M.R. Setare and A. Sepehri, Constructing warm inflationary model in finite temperature BIon, arXiv:1410.2552 [INSPIRE].
  9. [9]
    M.R. Setare and A. Sepehri, Constructing warm inflationary model in finite temperature BIon, arXiv:1410.2552 [INSPIRE].
  10. [10]
    A. Sepehri, F. Rahaman, A. Pradhan and I.H. Sardar, Emergence and Expansion of Cosmic Space in BIonic system, Phys. Lett. B 741 (2015) 92 [arXiv:1501.00428] [INSPIRE].CrossRefGoogle Scholar
  11. [11]
    E.F. Eiroa and C. Simeone, Cylindrical thin shell wormholes, Phys. Rev. D 70 (2004) 044008 [gr-qc/0404050] [INSPIRE].ADSMathSciNetGoogle Scholar
  12. [12]
    E.F. Eiroa and C. Simeone, Some general aspects of thin-shell wormholes with cylindrical symmetry, Phys. Rev. D 81 (2010) 084022 [arXiv:0912.5496] [INSPIRE].ADSGoogle Scholar
  13. [13]
    E.F. Eiroa and C. Simeone, Brans-Dicke cylindrical wormholes, Phys. Rev. D 82 (2010) 084039 [arXiv:1008.0382] [INSPIRE].ADSGoogle Scholar
  14. [14]
    M.G. Richarte, Cylindrical Wormholes with Positive Cosmological Constant, Phys. Rev. D 88 (2013) 027507 [arXiv:1308.2651] [INSPIRE].ADSGoogle Scholar
  15. [15]
    K.A. Bronnikov and J.P.S. Lemos, Cylindrical wormholes, Phys. Rev. D 79 (2009) 104019 [arXiv:0902.2360] [INSPIRE].ADSGoogle Scholar
  16. [16]
    N.M. Garcia, F.S.N. Lobo and M. Visser, Generic spherically symmetric dynamic thin-shell traversable wormholes in standard general relativity, Phys. Rev. D 86 (2012) 044026 [arXiv:1112.2057] [INSPIRE].ADSGoogle Scholar
  17. [17]
    E. Rubín de Celis, O.P. Santillan and C. Simeone, Probing global aspects of a geometry by the self-force on a charge: cylindical thin-shell wormholes, Phys. Rev. D 86 (2012) 124009 [arXiv:1210.4149] [INSPIRE].ADSGoogle Scholar
  18. [18]
    S.H. Mazharimousavi, M. Halilsoy and Z. Amirabi, Stability of generic cylindrical thin shell wormholes, Phys. Rev. D 89 (2014) 084003 [arXiv:1403.2861] [INSPIRE].ADSGoogle Scholar
  19. [19]
    G. Grignani, T. Harmark, A. Marini and M. Orselli, Thermal DBI action for the D3-brane at weak and strong coupling, JHEP 03 (2014) 114 [arXiv:1311.3834] [INSPIRE].CrossRefADSMathSciNetGoogle Scholar
  20. [20]
    A. Sen, Dirac- Born-Infeld action on the tachyon kink and vortex, Phys. Rev. D 68 (2003) 066008 [hep-th/0303057] [INSPIRE].ADSGoogle Scholar
  21. [21]
    M.R. Garousi, D-brane \( \overline{D} \) -brane effective action and brane interaction in open string channel, JHEP 01 (2005) 029 [hep-th/0411222] [INSPIRE].CrossRefADSMathSciNetGoogle Scholar
  22. [22]
    A. Dhar and P. Nag, Sakai-Sugimoto model, Tachyon Condensation and Chiral symmetry Breaking, JHEP 01 (2008) 055 [arXiv:0708.3233] [INSPIRE].CrossRefADSMathSciNetGoogle Scholar
  23. [23]
    A. Dhar and P. Nag, Tachyon condensation and quark mass in modified Sakai-Sugimoto model, Phys. Rev. D 78 (2008) 066021 [arXiv:0804.4807] [INSPIRE].ADSGoogle Scholar
  24. [24]
    M.R. Setare, A. Sepehri and V. Kamali, Constructing warm inflationary model in brane-antibrane system, Phys. Lett. B 735 (2014) 84 [arXiv:1405.7949] [INSPIRE].CrossRefADSGoogle Scholar
  25. [25]
    C.-j. Kim, H.B. Kim, Y.-b. Kim and O.-K. Kwon, Electromagnetic string fluid in rolling tachyon, JHEP 03 (2003) 008 [hep-th/0301076] [INSPIRE].CrossRefADSMathSciNetGoogle Scholar
  26. [26]
    F. Leblond and A.W. Peet, SD brane gravity fields and rolling tachyons, JHEP 04 (2003) 048 [hep-th/0303035] [INSPIRE].CrossRefADSMathSciNetGoogle Scholar
  27. [27]
    N.D. Lambert, H. Liu and J.M. Maldacena, Closed strings from decaying D-branes, JHEP 03 (2007) 014 [hep-th/0303139] [INSPIRE].CrossRefADSMathSciNetGoogle Scholar
  28. [28]
    R.R. Caldwell, M. Kamionkowski and N.N. Weinberg, Phantom energy and cosmic doomsday, Phys. Rev. Lett. 91 (2003) 071301 [astro-ph/0302506] [INSPIRE].CrossRefADSGoogle Scholar

Copyright information

© The Author(s) 2015

Authors and Affiliations

  1. 1.Department of Science, Campus of BijarUniversity of KurdistanBijarIran
  2. 2.Faculty of PhysicsShahid Bahonar UniversityKermanIran

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