Jump to ContentJump to Main Navigation
Show Summary Details
More options …

Zeitschrift für Naturforschung A

A Journal of Physical Sciences

Editor-in-Chief: Holthaus, Martin

Editorial Board: Fetecau, Corina / Kiefer, Claus

12 Issues per year


IMPACT FACTOR 2016: 1.432

CiteScore 2017: 1.30

SCImago Journal Rank (SJR) 2017: 0.403
Source Normalized Impact per Paper (SNIP) 2017: 0.632

Online
ISSN
1865-7109
See all formats and pricing
More options …
Volume 71, Issue 10

Issues

Accreting Scalar-Field Models of Dark Energy Onto Morris-Thorne Wormhole

Surajit ChattopadhyayORCID iD: http://orcid.org/0000-0002-5175-2873 / Antonio Pasqua / Irina Radinschi
Published Online: 2016-08-29 | DOI: https://doi.org/10.1515/zna-2016-0241

Abstract

The present paper reports a study on accreting tachyon, Dirac-Born-Infeld essence and h-essence scalar field models of dark energy onto Morris-Thorne wormhole. Using three different parameterisation schemes and taking H=H0+H1t, we have derived the mass of the wormhole for all of the three parameterisation schemes that are able to get hold of both quintessence and phantom behaviour. With suitable choice of parameters, we observed that accreting scalar field dark energy models are increasing the mass of the wormhole in the phantom phase and the mass is decreasing in the quintessence phase. Finally, we have considered accretion with power law form of scale factor and without any parameterisation scheme for the equation of state parameter and observed the fact that phantom-type dark energy supports the existence of wormholes.

Keywords: Accretion; Dark Energy; Morris-Thorne Wormhole

References

  • [1]

    A. G. Riess, A. V. Filippenko, P. Challis, A. Clocchiatti, A. Diercks, et al. Astron. J. 116, 1009 (1998).Google Scholar

  • [2]

    S. Perlmutter, G. Aldering, M. Della Valle, S. Deustua, R. S. Ellis, et al. Nature 391, 51 (1998).Google Scholar

  • [3]

    A. G. Riess, A. V. Filippenko, M. C. Liu, P. Challis, A. Clocchiatti, et al. Astrophys. J. 536, 62 (2000).Google Scholar

  • [4]

    D. N. Spergel, L. Verde, H. V. Peiris, E. Komatsu, M. R. Nolta, et al. Astrophys. J. Suppl. 148, 175 (2003) arXiv:astro-ph/0302209.Google Scholar

  • [5]

    E. Komatsu, J. Dunkley, M. R. Nolta, C. L. Bennett, B. Gold, et al. Astrophys. J. Suppl. 180, 330 (2009) arXiv:0803.0547 [astro-ph].Google Scholar

  • [6]

    E. J. Copeland, M. Sami, and S. Tsujikawa, Int. J. Mod. Phys. D 15, 1753 (2006).Google Scholar

  • [7]

    K. Bamba, S. Capozziello, S. Nojiri, and S. D. Odintsov, Astrophys. Space Sci. 342, 155 (2012).Google Scholar

  • [8]

    R. R. Caldwell and M. Kamionkowski, Ann. Rev. Nucl. Part. Sci. 59, 397 (2009).Google Scholar

  • [9]

    Y.-F. Cai, E. N. Saridakis, M. R. Setare, and J.-Q. Xia, Phys. Rept. 493, 1 (2010).Google Scholar

  • [10]

    J. A. Frieman, M. S. Turner, and D. Huterer, Annu. Rev. Astro. Astrophys. 46, 385 (2008).Google Scholar

  • [11]

    T. Padmanabhan, Gen. Rel. Grav. 40, 529 (2008).Google Scholar

  • [12]

    T. Padmanabhan, Curr. Sci. 88, 1057 (2005).Google Scholar

  • [13]

    S. Nojiri and S. D. Odintsov, Phys. Rep. 505, 59 (2011).Google Scholar

  • [14]

    V. Sahni and A. Starobinsky, Int. J. Mod. Phys. D 15, 2105 (2006).Google Scholar

  • [15]

    V. Sahni, A. Shafieloo, and A. A. Starobinsky, Astrophys. J. Lett. 793, L40 (2014).Google Scholar

  • [16]

    E. Elizalde, S. Nojiri, S. D. Odintsov, and P. Wang, Phys. Rev. D 71, 103504 (2005).Google Scholar

  • [17]

    D. Polarski, Int. J. Mod. Phys. D 22, 1330027 (2013).Google Scholar

  • [18]

    Y. L. Bolotin, A. Kostenko, O. A. Lemets, and D. A. Yerokhin, Int. J. Mod. Phys. D 24, 1530007 (2015).Google Scholar

  • [19]

    F. S. N. Lobo, Phys. Rev. D 73, 064028 (2006).Google Scholar

  • [20]

    B. Ratra and P. J. E. Peebles, Phys. Rev. D 37, 3406 (1988).Google Scholar

  • [21]

    K. Bamba, O. Razina, K. Yerzhanov, and R. Myrzakulov, Int. J. Mod. Phys. D 22, 1350023 (2013).Google Scholar

  • [22]

    V. Gorini, A. Yu. Kamenshchik, U. Moschella, and V. Pasquier, Phys. Rev. D 69, 123512 (2004).Google Scholar

  • [23]

    H. Wei, R.-G. Cai, and D.-F. Zeng, Class. Quant. Grav. 22, 3189 (2005).Google Scholar

  • [24]

    M. Jamil, P. K. F. Kuhfittig, F. Rahaman, and S. A. Rakib, Eur. Phys. J. C 67, 513 (2010).Google Scholar

  • [25]

    E. Guendelman and A. Kagnovich, Int. J. Mod. Phys. D 25, 1405 (2010).Google Scholar

  • [26]

    K. A. Bronnikov and J. P. S. Lemos, Phys. Rev. D 79, 104019 (2009).Google Scholar

  • [27]

    K. A. Bronnikov, V. G. Krechet, and J. P. S. Lemos, Phys. Rev. D 87, 084060 (2013).Google Scholar

  • [28]

    J. P. S. Lemos, F. S. N. Lobo, and S. Quinet de Oliveira, Phys. Rev. D 68, 064004 (2003).Google Scholar

  • [29]

    J. A. González, F. S. Guzmán, and O. Sarbach, Phys. Rev. D 80, 024023 (2009).Google Scholar

  • [30]

    P. K. F. Kuhfittig, Cent. Eur. J. Phys. 9, 1144 (2011).Google Scholar

  • [31]

    J. P. S. Lemos and F. S. N. Lobo, Phys. Rev. D 78, 044030 (2008).Google Scholar

  • [32]

    E. F. Eiroa and G. F. Aguirre, Eur. Phys. J. C 72, 2240 (2012).Google Scholar

  • [33]

    M. S. Morris, K. S. Thorne, and U. Yurtsever, Phy. Rev. Lett. 61, 1446 (1988).Google Scholar

  • [34]

    M. S. Morris and K. S. Thorne, Am. J. Phys. 56, 395 (1988).Google Scholar

  • [35]

    E. Babichev, V. Dokuchaev, and Y. Eroshenko, Phys. Rev. Lett. 93, 021102 (2004).Google Scholar

  • [36]

    P. F. Gonzalez-Diaz, Phys. Rev. Lett. 93, 071301 (2004).Google Scholar

  • [37]

    V. Faraoni and W. Israel, Phys. Rev. D 71, 064017 (2005).Google Scholar

  • [38]

    P. F. Gonzalez-Diaz, Phys. Rev. D 68, 084016 (2003).Google Scholar

  • [39]

    M. Jamil, D. Momeni, K. Bamba, and R. Myrzakulov, Int. J. Mod. Phys. D 21, 1250065 (2012).Google Scholar

  • [40]

    P. F. Gonzalez-Diaz, Phys. Lett. B 632, 159 (2006).Google Scholar

  • [41]

    F.C. Michel, Astrophys. Space Sci. 15, 153 (1972).Google Scholar

  • [42]

    E. Babichev, V. Dokuchaev, and Y. Eroshenko, Phys. Rev. Lett. 93, 021102 (2004).Google Scholar

  • [43]

    J. Bhadra and U. Debnath, Eur. Phys. J. C 72, 1912 (2012).Google Scholar

  • [44]

    U. Debnath, Eur. Phys. J. C 74, 2869 (2014).Google Scholar

  • [45]

    S. Chattopadhyay, D. Momeni, A. Altaibayeva, and R. Myrzakulov, Astrophys. Space Sci. 355, 2204 (2014).Google Scholar

  • [46]

    A. R. Cooray and D. Huterer, Astrophys. J. 513, L95 (1999).Google Scholar

  • [47]

    M. Chevallier and D. Polarski, Int. J. Mod. Phys. D 10, 213 (2001).Google Scholar

  • [48]

    E.V. Linder, Phys. Rev. Lett. 90, 091301 (2003).Google Scholar

  • [49]

    S. Linden and J.-M. Virey, Phys. Rev. D 78, 023526 (2008).Google Scholar

  • [50]

    J. A. Vazquez, M. Bridges, M. P. Hobson, and A. N. Lasenby, JCAP 1209, 020 (2012).Google Scholar

  • [51]

    H. K. Jassal, J. S. Bagla, and T. Padmanabhan, Mon. Not. Roy. Astron. Soc. 356, L11 (2005).Google Scholar

  • [52]

    U. Debnath, Eur. Phys. J. C 75, 449 (2015).Google Scholar

  • [53]

    R. Biswas and U. Debnath, Astrophys. Space Sci. 353, 721 (2014).Google Scholar

  • [54]

    S. Nojiri and S. D. Odintsov, Phys. Rev. D 74, 086005 (2006).Google Scholar

  • [55]

    A. Sen, J. High Energy Phys. 4, 048 (2002).Google Scholar

  • [56]

    A. Sen, J. High Energy Phys. 7, 065 (2002).Google Scholar

  • [57]

    J. S. Bagla, H. K. Jassal, and T. Padmanabhan, Phys. Rev. D 67, 063504 (2003).Google Scholar

  • [58]

    E. J. Copeland, M. R. Garousi, M. Sami, and S. Tsujikawa, Phys. Rev. D 71, 043003 (2005).Google Scholar

  • [59]

    V. Gorini, A. Kamenshchik, U. Moschella, and V. Pasquier, Phys. Rev. D 69, 123512 (2004).Google Scholar

  • [60]

    S. Chattopadhyay, Astrophys. Space Sci. 331, 651 (2011).Google Scholar

  • [61]

    J. Martin and M. Yamaguchi, Phys. Rev. D 77, 123508 (2008).Google Scholar

  • [62]

    S. Chattopadhyay and U. Debnath, Int. J. Mod. Phys. A 25, 5557 (2010).Google Scholar

  • [63]

    S. Chattopadhyay and U. Debnath, Int. J. Theor. Phys. 49, 1465 (2010).Google Scholar

  • [64]

    S. Nojiri, O. Obregon, S. D. Odintsov, and K. E. Osetrin, Phys. Lett. B 449, 173 (1999).Google Scholar

  • [65]

    S. Nojiri, O. Obregon, S. D. Odintsov, and K. E. Osetrin, Phys. Lett. B 458, 19 (1999).Google Scholar

  • [66]

    S. Nojiri and I. Oda, Mod. Phys. Lett. A 9, 959 (1994).Google Scholar

  • [67]

    H. Wei and R-G. Cai, Phys. Rev. D 72, 123507 (2005).Google Scholar

  • [68]

    H. Wei, N. Tang, and S. Nan Zhang, Phys. Rev. D 75, 043009 (2007).Google Scholar

  • [69]

    S. V. Sushkov, Phys. Rev. D 71, 043520 (2005).Google Scholar

  • [70]

    S. V. Sushkov and S.-W. Kim, Gen. Rel. Grav. 36, 1671 (2004).Google Scholar

  • [71]

    P. F. Gonzalez-Diaz and J. A. Jimenez-Madrid, Phys. Lett. B 596, 16 (2004).Google Scholar

  • [72]

    V. Folomeev and V. Dzhunushaliev, Phys. Rev. D 89, 064002 (2014).Google Scholar

  • [73]

    S. Nojiri and S. D. Odintsov, Phys. Rev. D 70, 103522 (2004).Google Scholar

  • [74]

    E. Elizalde, S. Nojiri, and S. D. Odintsov, Phys. Rev. D 70, 043539 (2004).Google Scholar

  • [75]

    S. Nojiri and S. D. Odintsov, Phys. Rev. D 72, 023003 (2005).Google Scholar

  • [76]

    L. P. Chimento and R. Lazkoz, Mod. Phys. Lett. A 19, 2479 (2004).Google Scholar

  • [77]

    E. N. Saridakis and S. V. Sushkov, Phys. Rev. D 81, 083510 (2010).Google Scholar

  • [78]

    S. Nojiri, S. D. Odintsov, and S. Tsujikawa, Phys. Rev. D 71, 063004 (2005).Google Scholar

About the article

Received: 2016-06-17

Accepted: 2016-07-24

Published Online: 2016-08-29

Published in Print: 2016-10-01


Citation Information: Zeitschrift für Naturforschung A, Volume 71, Issue 10, Pages 949–960, ISSN (Online) 1865-7109, ISSN (Print) 0932-0784, DOI: https://doi.org/10.1515/zna-2016-0241.

Export Citation

©2016 Walter de Gruyter GmbH, Berlin/Boston.Get Permission

Comments (0)

Please log in or register to comment.
Log in