# Difference between revisions of "Zeta-function method for regularization"

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When one comes to specific calculations, the zeta-function regularization method relies on the existence of simple formulas for obtaining the analytic continuation above. These consist of the reflection formula of the corresponding zeta-function in each case, together with some other fundamental expressions, as the Jacobi theta-function identity, Poisson's resummation formula and the famous Chowla–Selberg formula [[#References|[a2]]]. However, some of these formulas are restricted to very specific zeta-functions, and it often turned out that for some physically important cases the corresponding formulas did not exist in the literature. This has required a painful process (it has taken over a decade already) of generalization of previous results and derivation of new expressions of this kind [[#References|[a5]]], [[#References|[a6]]]. [[#References|[a1]]]. | When one comes to specific calculations, the zeta-function regularization method relies on the existence of simple formulas for obtaining the analytic continuation above. These consist of the reflection formula of the corresponding zeta-function in each case, together with some other fundamental expressions, as the Jacobi theta-function identity, Poisson's resummation formula and the famous Chowla–Selberg formula [[#References|[a2]]]. However, some of these formulas are restricted to very specific zeta-functions, and it often turned out that for some physically important cases the corresponding formulas did not exist in the literature. This has required a painful process (it has taken over a decade already) of generalization of previous results and derivation of new expressions of this kind [[#References|[a5]]], [[#References|[a6]]]. [[#References|[a1]]]. | ||

+ | |||

+ | Elizalde and others have extended the Zeta regularization algorithm to include divergent integrals \being{equation} \int_{a}^{\infty}x^{m}dx \end{equation} by using the recurrence equation | ||

+ | |||

+ | \begin{equation} \begin{array}{l} | ||

+ | \int\nolimits_{a}^{\infty }x^{m-s} dx =\frac{m-s}{2} \int\nolimits_{a}^{\infty }x^{m-1-s} dx +\zeta (s-m)-\sum\limits_{i=1}^{a}i^{m-s} +a^{m-s} \\ | ||

+ | -\sum\limits_{r=1}^{\infty }\frac{B_{2r} \Gamma (m-s+1)}{(2r)!\Gamma (m-2r+2-s)} (m-2r+1-s)\int\nolimits_{a}^{\infty }x^{m-2r-s} dx \end{array} \end{equation} | ||

+ | |||

+ | this is the natural extension to integrals of the Zeta regularization algorithm | ||

====References==== | ====References==== | ||

<table><TR><TD valign="top">[a1]</TD> <TD valign="top"> A.A. Bytsenko, G. Cognola, L. Vanzo, S. Zerbini, "Quantum fields and extended objects in space-times with constant curvature spatial section" ''Phys. Rept.'' , '''266''' (1996) pp. 1–126</TD></TR><TR><TD valign="top">[a2]</TD> <TD valign="top"> E. Elizalde, "Multidimensional extension of the generalized Chowla–Selberg formula" ''Commun. Math. Phys.'' , '''198''' (1998) pp. 83–95</TD></TR><TR><TD valign="top">[a3]</TD> <TD valign="top"> S.W. Hawking, "Zeta function regularization of path integrals in curved space time" ''Commun. Math. Phys.'' , '''55''' (1977) pp. 133–148</TD></TR><TR><TD valign="top">[a4]</TD> <TD valign="top"> M. Nakahara, "Geometry, topology, and physics" , Inst. Phys. (1995) pp. 7–8</TD></TR><TR><TD valign="top">[a5]</TD> <TD valign="top"> E. Elizalde, S.D. Odintsov, A. Romeo, A.A. Bytsenko, S. Zerbini, "Zeta regularization techniques with applications" , World Sci. (1994)</TD></TR><TR><TD valign="top">[a6]</TD> <TD valign="top"> E. Elizalde, "Ten physical applications of spectral zeta functions" , Springer (1995)</TD></TR></table> | <table><TR><TD valign="top">[a1]</TD> <TD valign="top"> A.A. Bytsenko, G. Cognola, L. Vanzo, S. Zerbini, "Quantum fields and extended objects in space-times with constant curvature spatial section" ''Phys. Rept.'' , '''266''' (1996) pp. 1–126</TD></TR><TR><TD valign="top">[a2]</TD> <TD valign="top"> E. Elizalde, "Multidimensional extension of the generalized Chowla–Selberg formula" ''Commun. Math. Phys.'' , '''198''' (1998) pp. 83–95</TD></TR><TR><TD valign="top">[a3]</TD> <TD valign="top"> S.W. Hawking, "Zeta function regularization of path integrals in curved space time" ''Commun. Math. Phys.'' , '''55''' (1977) pp. 133–148</TD></TR><TR><TD valign="top">[a4]</TD> <TD valign="top"> M. Nakahara, "Geometry, topology, and physics" , Inst. Phys. (1995) pp. 7–8</TD></TR><TR><TD valign="top">[a5]</TD> <TD valign="top"> E. Elizalde, S.D. Odintsov, A. Romeo, A.A. Bytsenko, S. Zerbini, "Zeta regularization techniques with applications" , World Sci. (1994)</TD></TR><TR><TD valign="top">[a6]</TD> <TD valign="top"> E. Elizalde, "Ten physical applications of spectral zeta functions" , Springer (1995)</TD></TR></table> |

## Revision as of 22:18, 20 March 2013

*zeta-function regularization*

Regularization and renormalization procedures are essential issues in contemporary physics — without which it would simply not exist, at least in the form known today (2000). They are also essential in supersymmetry calculations. Among the different methods, zeta-function regularization — which is obtained by analytic continuation in the complex plane of the zeta-function of the relevant physical operator in each case — might well be the most beautiful of all. Use of this method yields, for instance, the vacuum energy corresponding to a quantum physical system (with constraints of any kind, in principle). Assuming the corresponding Hamiltonian operator, , has a spectral decomposition of the form (think, as simplest case, of a quantum harmonic oscillator): , with some set of indices (which can be discrete, continuous, mixed, multiple, etc.), then the quantum vacuum energy is obtained as follows [a5], [a6]:

where is the zeta-function corresponding to the operator . The formal sum over the eigenvalues is usually ill-defined, and the last step involves analytic continuation, inherent to the definition of the zeta-function itself. These mathematically simple-looking relations involve very deep physical concepts (no wonder that understanding them took several decades in the recent history of quantum field theory, QFT). The zeta-function method is unchallenged at the one-loop level, where it is rigorously defined and where many calculations of QFT reduce basically (from a mathematical point of view) to the computation of determinants of elliptic pseudo-differential operators (DOs, cf. also Pseudo-differential operator) [a2]. It is thus no surprise that the preferred definition of determinant for such operators is obtained through the corresponding zeta-function.

When one comes to specific calculations, the zeta-function regularization method relies on the existence of simple formulas for obtaining the analytic continuation above. These consist of the reflection formula of the corresponding zeta-function in each case, together with some other fundamental expressions, as the Jacobi theta-function identity, Poisson's resummation formula and the famous Chowla–Selberg formula [a2]. However, some of these formulas are restricted to very specific zeta-functions, and it often turned out that for some physically important cases the corresponding formulas did not exist in the literature. This has required a painful process (it has taken over a decade already) of generalization of previous results and derivation of new expressions of this kind [a5], [a6]. [a1].

Elizalde and others have extended the Zeta regularization algorithm to include divergent integrals \being{equation} \int_{a}^{\infty}x^{m}dx \end{equation} by using the recurrence equation

\begin{equation} \begin{array}{l} \int\nolimits_{a}^{\infty }x^{m-s} dx =\frac{m-s}{2} \int\nolimits_{a}^{\infty }x^{m-1-s} dx +\zeta (s-m)-\sum\limits_{i=1}^{a}i^{m-s} +a^{m-s} \\ -\sum\limits_{r=1}^{\infty }\frac{B_{2r} \Gamma (m-s+1)}{(2r)!\Gamma (m-2r+2-s)} (m-2r+1-s)\int\nolimits_{a}^{\infty }x^{m-2r-s} dx \end{array} \end{equation}

this is the natural extension to integrals of the Zeta regularization algorithm

#### References

[a1] | A.A. Bytsenko, G. Cognola, L. Vanzo, S. Zerbini, "Quantum fields and extended objects in space-times with constant curvature spatial section" Phys. Rept. , 266 (1996) pp. 1–126 |

[a2] | E. Elizalde, "Multidimensional extension of the generalized Chowla–Selberg formula" Commun. Math. Phys. , 198 (1998) pp. 83–95 |

[a3] | S.W. Hawking, "Zeta function regularization of path integrals in curved space time" Commun. Math. Phys. , 55 (1977) pp. 133–148 |

[a4] | M. Nakahara, "Geometry, topology, and physics" , Inst. Phys. (1995) pp. 7–8 |

[a5] | E. Elizalde, S.D. Odintsov, A. Romeo, A.A. Bytsenko, S. Zerbini, "Zeta regularization techniques with applications" , World Sci. (1994) |

[a6] | E. Elizalde, "Ten physical applications of spectral zeta functions" , Springer (1995) |

**How to Cite This Entry:**

Zeta-function method for regularization.

*Encyclopedia of Mathematics.*URL: http://www.encyclopediaofmath.org/index.php?title=Zeta-function_method_for_regularization&oldid=13101