Skip to main content

Cosmology of Massive Gravity in the Decoupling Limit

  • Chapter
  • First Online:
Theoretical and Observational Consistency of Massive Gravity

Part of the book series: Springer Theses ((Springer Theses))

  • 484 Accesses

Abstract

In this chapter we will aim the ambitious task of addressing the burdensome problems of cosmology using the framework of massive gravity. More concrete, we will try to answer the questions of whether or not massive gravity can produce a theoretically reliable self-accelerated geometry and whether or not it can also resolve the cosmological constant problem.

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

Access this chapter

eBook
USD 16.99
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Hardcover Book
USD 109.99
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

Institutional subscriptions

Notes

  1. 1.

    Recall that we excluded the helicity-1 part since it only appears quadratically.

References

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Lavinia Heisenberg .

Rights and permissions

Reprints and permissions

Copyright information

© 2015 Springer International Publishing Switzerland

About this chapter

Cite this chapter

Heisenberg, L. (2015). Cosmology of Massive Gravity in the Decoupling Limit. In: Theoretical and Observational Consistency of Massive Gravity. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-18935-2_2

Download citation

Publish with us

Policies and ethics