Swampland (physics)

In physics, the term swampland refers to effective low-energy physical theories which are not compatible with string theory, in contrast to the so-called "string theory landscape" of compatible theories. In other words, the swampland is the set of consistent-looking theories with no consistent ultraviolet completion in string theory.

Developments in string theory suggest that the string theory landscape of false vacua is vast, so it is natural to ask if the landscape is as vast as allowed by consistent-looking effective field theories. Some authors, such as Cumrun Vafa,[1] suggest that is not the case and that the swampland is in fact much larger than the string theory landscape.

Swampland conjectures

The swampland conjectures are a set of conjectured criteria for theories in the string theory landscape. Some proposed swampland criteria:[2]

References

  1. Vafa, Cumrun (2005). "The String Landscape and the Swampland". arXiv:hep-th/0509212.
  2. Arkani-Hamed, Nima; Motl, Luboš; Nicolis, Alberto; Vafa, Cumrun (15 June 2007). "The String Landscape, Black Holes and Gravity as the Weakest Force". Journal of High Energy Physics. 2007 (6): 060. arXiv:hep-th/0601001. Bibcode:2007JHEP...06..060A. doi:10.1088/1126-6708/2007/06/060. S2CID 16415027.


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.