Skip to main content

The Quantum-to-Classical Transition of Primordial Cosmological Perturbations

  • Conference paper
  • First Online:
  • 632 Accesses

Part of the book series: Astrophysics and Space Science Proceedings ((ASSSP,volume 45))

Abstract

There is a widespread belief that the classical small inhomogeneities which gave rise to all structures in the Universe through gravitational instability originated from primordial quantum cosmological fluctuations. However, this transition from quantum to classical fluctuations is plagued with important conceptual issues, most of them related to the application of standard quantum theory to the Universe as a whole. In this contribution, it is shown how these issues can easily be overcome in the framework of the de Broglie-Bohm quantum theory. This theory is an alternative to standard quantum theory that provides an objective description of physical reality, where rather ambiguous notions of measurement or observer play no fundamental role, and which can hence be applied to the Universe as a whole. In addition, it allows for a simple and unambiguous characterization of the classical limit. This contribution is a compilation of the works done by Grasiele Santos, Ward Struyve and myself cited in Pinto-Neto et al. (Phys Rev D 85:083506, 2012; Phys Rev D 89:023517, 2014), where all details can be found.

This is a preview of subscription content, log in via an institution.

Buying options

Chapter
USD   29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD   189.00
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD   249.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD   249.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Learn about institutional subscriptions

Notes

  1. 1.

    In the de Broglie-Bohm approach, it is possible to obtain the effective theory of perturbations from the full quantization of the background geometry and linear perturbations, see Falciano and Pinto-Neto (2009).

  2. 2.

    In fact, as A 1 and A 2 depend on k, this assertion depends on the scale we are talking about. For an almost scale invariant spectrum of cosmological perturbations, the A 2 term is larger than the A 1 term for all scales of cosmological interest, which enforces the argumentation described below for the transition of quantum-to-classical behavior in bouncing models. Only for very short wavelengths can the A 1 term be bigger than A 2.

References

  • Albrecht, A., Ferreira, P., Joyce, M., Prokopec, T.: Phys. Rev. D 50, 4807 (1994). arXiv:astro-ph/9303001v2

    Google Scholar 

  • Bohm, D., Hiley, B.J.: The Undivided Universe. Routledge, New York (1993)

    MATH  Google Scholar 

  • Burgess, C.P., Holman, R., Hoover, D.: Phys. Rev. D 77, 063534 (2008). arXiv:astro-ph/0601646v1

    Google Scholar 

  • De Unánue, A., Sudarsky, D.: Phys. Rev. D 78, 043510 (2008). arXiv:0801.4702v2 [gr-qc]

    Google Scholar 

  • Dürr, D., Teufel, S.: Bohmian Mechanics. Springer, Berlin (2009)

    MATH  Google Scholar 

  • Falciano, F.T., Pinto-Neto, N.: Phys. Rev. D 79, 023507 (2009). arXiv:0810.3542v2 [gr-qc]

    Google Scholar 

  • Guth, A.H., Pi, S.-Y.: Phys. Rev. D 32, 1899 (1985)

    Article  ADS  MathSciNet  Google Scholar 

  • Holland, P.R.: The Quantum Theory of Motion. Cambridge University Press, Cambridge (1993)

    Book  Google Scholar 

  • Kiefer, C., Polarski, D.: Ann. Phys. 7, 137 (1998). arXiv:gr-qc/9805014v2

    Article  Google Scholar 

  • Kiefer, C., Polarski, D.: Adv. Sci. Lett. 2, 164 (2009). arXiv:0810.0087v2 [astro-ph]

    Article  Google Scholar 

  • Landau, S.J., Scóccola, C.G., Sudarsky, D.: Phys. Rev. D 85, 123001 (2012)

    Article  ADS  Google Scholar 

  • León, G., Sudarsky, D.: Class. Quantum Gravit. 27, 225017 (2010). arXiv:1003.5950v2 [gr-qc]

    Google Scholar 

  • León, G., Landau, S.J., Sudarsky, D.: Phys. Rev. D 88, 023526 (2013)

    Article  ADS  Google Scholar 

  • Lesgourgues, J., Polarski, D., Starobinsky, A.A.: Nucl. Phys. B 497, 479 (1997). arXiv:gr-qc/9611019v1

    Google Scholar 

  • Liddle, A.R., Lyth, D.H.: Cosmological Inflation and Large-Scale Structure. Cambridge University Press, New York (2000)

    Book  MATH  Google Scholar 

  • Lyth, D.H., Liddle, A.R.: The Primordial Density Perturbation. Cambridge University Press, Cambridge (2009)

    Book  MATH  Google Scholar 

  • Mukhanov, V.: Physical Foundations of Cosmology. Cambridge University Press, New York (2005)

    Book  MATH  Google Scholar 

  • Novello, M., Perez Bergliaffa, S.E.: Phys. Rep. 463, 127 (2008). arXiv:0802.1634v1 [astro-ph]

    Article  ADS  MathSciNet  Google Scholar 

  • Perez, A., Sahlmann, H., Sudarsky, D.: Class. Quantum Gravit. 23, 2317 (2006). arXiv:gr-qc/0508100v3

    Google Scholar 

  • Peter, P., Uzan, J.-P.: Primordial Cosmology. Oxford University Press, Oxford (2009)

    Google Scholar 

  • Peter, P., Pinho, E., Pinto-Neto, N.: Phys. Rev. D 75, 023516 (2007). arXiv:hep-th/0610205

    Google Scholar 

  • Pinto-Neto, N., Santos, G., Struyve, W.: Phys. Rev. D 85, 083506 (2012)

    Article  ADS  Google Scholar 

  • Pinto-Neto, N., Santos, G., Struyve, W.: Phys. Rev. D 89, 023517 (2014)

    Article  ADS  Google Scholar 

  • Polarski, D., Starobinsky, A.A.: Class. Quantum Gravit. 13, 377 (1996). arXiv:gr-qc/9504030v2

    Google Scholar 

  • Sudarsky, D.: Int. J. Mod. Phys. D 20, 509 (2011). arXiv:0906.0315v3 [gr-qc]

    Google Scholar 

  • Vitenti, S., Pinto-Neto, N.: Phys. Rev. D 85, 023524 (2012). arXiv:1111.0888 [astro-ph.CO]

    Google Scholar 

  • Weinberg, S.: Cosmology. Oxford University Press, New York (2008)

    MATH  Google Scholar 

Download references

Acknowledgements

I would like to thank CNPq of Brazil for financial support and Daniel Sudarsky for some illuminating discussions on this problem.

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Nelson Pinto-Neto .

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 2016 Springer International Publishing Switzerland

About this paper

Cite this paper

Pinto-Neto, N. (2016). The Quantum-to-Classical Transition of Primordial Cosmological Perturbations. In: Fabris, J., Piattella, O., Rodrigues, D., Velten, H., Zimdahl, W. (eds) The Cosmic Microwave Background. Astrophysics and Space Science Proceedings, vol 45. Springer, Cham. https://doi.org/10.1007/978-3-319-44769-8_11

Download citation

Publish with us

Policies and ethics