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gr-qcApr 1, 2008
5
citations (OpenAlex)
authors
  • Vladimir Dzhunushaliev
  • Vladimir Folomeev
  • Shynaray Myrzakul
  • Ratbay Myrzakulov
institutions
  • FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
  • Kyrgyz-Russian Slavic University named after B.N. Yeltsin
  • L. N. Gumilyov Eurasian National University
arXiv abstractPDF
paper

Phantom thick brane in 5D bulk

arXiv:0804.0151 · doi:10.1142/S0217732308028296

Abstract

A model of a thick brane in 5D bulk supported by two phantom scalar fields is considered. The comparison with a thick brane supported by two usual scalar fields is carried out. The distinctions between a thick brane supported by one usual scalar field and our model have been pointed out.

unessential changes

References in corpus (8)

  • Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
  • Measurements of Omega and Lambda from 42 High-Redshift Supernovae
  • The Case for a Positive Cosmological Lambda-term
  • Late-time cosmology in (phantom) scalar-tensor theory: dark energy and the cosmic speed-up
  • Dark Matter and Dark Energy
  • Is there Supernova Evidence for Dark Energy Metamorphosis ?
  • Thick Brane Worlds and Their Stability
  • Phantom cosmology as a simple model with dynamical complexity

Cited by in corpus (4)

  • Thick brane solutions
  • Gravitational resonances in mimetic thick branes
  • Spinor brane
  • Z2-Symmetric Thick Brane with Specific Warp Function
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