Naturalness (physics)

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In physics, naturalness is the property that the dimensionless ratios between free parameters or physical constants appearing in a physical theory should take values "of order 1" and that free parameters are not fine-tuned. That is, a natural theory would have parameter ratios with values like 2.34 rather than 234000 or 0.000234. This is in contrast to current theory like the standard model, where there are a number of parameters that vary by many orders of magnitude, and require extensive "fine-tuning" of those values in order for the theory to predict properties resembling those observed for the universe we live in.

The requirement that satisfactory theories should be "natural" in this sense is a current of thought initiated around the 1960s in particle physics. It is an aesthetic criterion, not a physical one, that arises from the seeming non-naturalness of the standard model and the broader topics of the hierarchy problem, fine-tuning, and the anthropic principle.

It is not always compatible with Occam's razor, since many instances of "natural" theories have more parameters than "fine-tuned" theories such as the Standard Model. Naturalness in physics is closely related to the issue of fine-tuning, and over the past decade many scientists[1][2][3][4][5] argued that the principle of naturalness is a specific application of Bayesian statistics.


In particle physics, the assumption of naturalness means that, unless a more detailed explanation exists, all conceivable terms in the effective action that preserve the required symmetries should appear in this effective action with natural coefficients.[6]

In an effective field theory, Λ is the cutoff scale, an energy or length scale at which the theory breaks down. Due to dimensional analysis, natural coefficients have the form

where d is the dimension of the field operator; and c is a dimensionless number which should be "random" and smaller than 1 at the scale where the effective theory breaks down. Further renormalization group running can reduce the value of c at an energy scale E, but by a small factor proportional to ln(E/Λ).

Some parameters in the effective action of the Standard Model seem to have far smaller coefficients than required by consistency with the assumption of naturalness, leading to some of the fundamental open questions in physics. In particular:

In addition, the coupling of the electron to the Higgs, the mass of the electron, is abnormally small, and to a lesser extent, the masses of the light quarks.

In models with large extra dimensions, the assumption of naturalness is violated for operators which multiply field operators that create objects which are localized at different positions in the extra dimensions.[7]

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  1. ^ Fowlie, Andrew; Balazs, Csaba; White, Graham; Marzola, Luca; Raidal, Martti (17 August 2016). "Naturalness of the relaxion mechanism". Journal of High Energy Physics. 2016 (8). doi:10.1007/JHEP08(2016)100. 
  2. ^ Fowlie, Andrew (10 July 2014). "CMSSM, naturalness and the ?fine-tuning price? of the Very Large Hadron Collider". Physical Review D. 90 (1). doi:10.1103/PhysRevD.90.015010. 
  3. ^ Fowlie, Andrew (15 October 2014). "Is the CNMSSM more credible than the CMSSM?". The European Physical Journal C. 74 (10). doi:10.1140/epjc/s10052-014-3105-y. 
  4. ^ . doi:10.1088/1126-6708/2009/03/075.  Missing or empty |title= (help)
  5. ^ Fichet, S. (18 December 2012). "Quantified naturalness from Bayesian statistics". Physical Review D. 86 (12). doi:10.1103/PhysRevD.86.125029. 
  6. ^ N. Seiberg (1993). "Naturalness versus supersymmetric non-renormalization theorems". Physics Letters B. 318 (3): 469–475. Bibcode:1993PhLB..318..469S. arXiv:hep-ph/9309335Freely accessible. doi:10.1016/0370-2693(93)91541-T. 
  7. ^ N. Arkani-Hamed, M. Schmaltz (2000). "Hierarchies without Symmetries from Extra Dimensions". Physical Review D. 61 (3): 033005. Bibcode:2000PhRvD..61c3005A. arXiv:hep-ph/9903417Freely accessible. doi:10.1103/PhysRevD.61.033005. 

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