Remember Me
Or use your Academic/Social account:


You have just completed your registration at OpenAire.

Before you can login to the site, you will need to activate your account. An e-mail will be sent to you with the proper instructions.


Please note that this site is currently undergoing Beta testing.
Any new content you create is not guaranteed to be present to the final version of the site upon release.

Thank you for your patience,
OpenAire Dev Team.

Close This Message


Verify Password:
Verify E-mail:
*All Fields Are Required.
Please Verify You Are Human:

OpenAIRE is about to release its new face with lots of new content and services.
During September, you may notice downtime in services, while some functionalities (e.g. user registration, login, validation, claiming) will be temporarily disabled.
We apologize for the inconvenience, please stay tuned!
For further information please contact helpdesk[at]openaire.eu

fbtwitterlinkedinvimeoflicker grey 14rssslideshare1
Wang, Deng; Meng, Xin-He (2017)
Languages: English
Types: Preprint

Classified by OpenAIRE into

arxiv: General Relativity and Quantum Cosmology, Astrophysics::Cosmology and Extragalactic Astrophysics
We investigate the thin-shell wormholes constrained by cosmological observations for the first time in the literature. Without loss of generality, we study the thin-shell wormholes in $\omega$CDM model and analyze their stability under perturbations preserving the symmetry. Firstly, we constrain the $\omega$CDM model using a combination of Union 2.1 SNe Ia data, the latest $H(z)$ data and CMB data. Secondly, we use the constrained dark energy equation of state (EoS) $\omega$ which lies in $[-1.05,-0.89]$ to investigate thin-shell wormholes of various black hole spacetimes. We find that the stable Schwarzschild and Reinssner-Nordstr\"{o}m thin-shell wormholes constrained by cosmological observations do not exist. In addition, the method we developed can be applied into exploring the stable thin-shell wormholes from any black hole spacetime in the framework of any cosmological theory.
  • The results below are discovered through our pilot algorithms. Let us know how we are doing!

    • [1] M.S. Moris and K.S. Thorne, Am. J. Phys. 56, 395 (1988). [2] M. Visser, Lorentzian Wormholes: From Einstein to Hawking, (Springer, Berlin, 1997). [3] M. Visser et al., Phys. Rev. Lett. 90, 201102 (2003). [4] C. Barcelo and M. Visser, Int. J. Mod. Phys. D 11, 1553 (2002). [5] M. Visser, Phys. Rev. D 39, 3182 (1989).
    • [6] M. Visser, Nucl. Phys. B 328, 203 (1989).
    • [7] E. Poisson and M. Visser, Phys. Rev. D 52, 7318 (1995). [8] M. Ishak and K. Lake, Phys. Rev. D 65, 044011 (2002). [9] E. F. Eiroa, Phys. Rev. D 78, 024018 (2008).
    • [10] N. M. Garcia et al., Phys. Rev. D 86, 044026 (2012). [11] M. G. Richarte and C. Simeone, Phys. Rev. D 80, 104033 (2009). [12] G. A. S. Dias and J. P. S. Lemos, Phys. Rev. D 82, 084023 (2010). [13] J. P. S. Lemos et al., Phys. Rev. D 78, 044030 (2008). [14] E. F. Eiroa et al., Phys. Rev. D 70, 044008 (2004). [15] E. F. Eiroa et al., Phys. Rev. D 92, 044002 (2015). [16] A. G. Riess et al., Astron. J. 116, 1009 (1998).
    • [17] S. Perlmutter, M. S. Turner, and M. White, Phys. Rev. Lett. 83, 670 (1999). [18] F. S. N. Lobo, Phys. Rev. D 71, 084011 (2005).
    • [19] F. S. N. Lobo, Phys. Rev. D 71, 124022 (2005).
    • [20] F. S. N. Lobo, Phys. Rev. D 73, 064028 (2006).
    • [21] Deng Wang, Xinhe Meng, Eur. Phys. J. C 76, 171 (2016). [22] Hristu Culetu, [arXiv:1502.01589].
    • [23] Mubasher Jamil, Nuovo Cim.B 123, 599-603, (2008). [24] Deng Wang, Xinhe Meng, Eur. Phys. J. C 76, 484 (2016). [25] Deng Wang, Xinhe Meng, [arXiv: 1602.04699].
    • [26] N. Suzuki et al., Astrophys. J. 746, 85 (2012).
    • [27] M. Moresco et al., J. Cosmol. Astropart. Phys. 05, 014 (2016). [28] X. L. Meng et al., [arXiv: 1507.02517].
    • [29] Y. Wang and P. Mukherjee, Phys. Rev. D 76, 103533 (2007). [30] Y. Wang, Phys. Rev. D 77, 123525 (2008).
    • [31] L. Page et al., Astrophys. J. Suppl. Ser. 148, 233 (2003). [32] W. Hu and N. Sugiyama, Astrophys. J. 471, 542 (1996). [33] Y. Wang and S. Wang, Phys. Rev. D 88, 043522 (2013).
  • No related research data.
  • No similar publications.

Share - Bookmark

Cite this article

Collected from

Cookies make it easier for us to provide you with our services. With the usage of our services you permit us to use cookies.
More information Ok