| J. Phys. A: Math. Gen. 38 No 18 (6 May 2005) L317-L323 |
| doi:10.1088/0305-4470/38/18/L03 |
| PII: S0305-4470(05)96395-6 |
Neutrix calculus and finite quantum field theory
Y Jack Ng and H van Dam
Institute of Field Physics, Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599-3255, USA
Email: yjng@physics.unc.edu
Received 7 March 2005, in final form 31 March 2005
Published 18 April 2005
| Abstract. In general, quantum field theories (QFT) require regularizations and infinite renormalizations due to ultraviolet divergences in their loop calculations. Furthermore, perturbation series in theories like quantum electrodynamics are not convergent series, but are asymptotic series. We apply neutrix calculus, developed in connection with asymptotic series and divergent integrals, to QFT, obtaining finite renormalizations. While none of the physically measurable results in renormalizable QFT is changed, quantum gravity is rendered more manageable in the neutrix framework. |
PACS numbers: 03.70. + k, 11.10.Gh, 11.10. - z
The procedure of regularization and renormalization is a big step forward in making sense of the infinities that one encounters in calculating perturbative series in quantum field theories. The result is a phenomenal success. For example, quantum electrodynamics (QED), the paradigm of relativistic quantum field theories, suitably regularized and renormalized, is arguably the most accurate theory ever devised by mankind. Yet in spite of the impressive phenomenological successes, the spectre of infinite renormalizations has convinced many, including such eminent physicists as Dirac and Schwinger, that we should seek a better mathematical and/or physical foundation for quantum field theory, without simultaneously tearing down the towering edifice we have built on the existing one. In another development, Dyson [1] has shown that the series as defined by the Feynman rules in QED is not a convergent series and has suggested that it is instead an asymptotic series in the fine structure constant α, i.e., in the number of internal integrals (for given outside lines). In this letter, we propose to apply neutrix calculus, in conjunction with Hadamard integrals, developed by J G van der Corput [2] in connection with asymptotic series and divergent integrals, to quantum field theories in general, and QED in particular, to obtain finite results for the coefficients in the perturbation series. (A more detailed discussion [3] will appear elsewhere.) The replacement of regular integrals by Hadamard integrals in quantum field theory appears to make good mathematical sense, as van der Corput observed that Hadamard integrals are the proper tool to calculate the coefficients of an asymptotic series. (Actually Hadamard integrals work equally well for convergent series.)
We begin by recalling the definition of asymptotic series [4]. The series f(x) = a0 + a1(x - b) + a2(x - b)2 + ··· for finite b is an asymptotic series if and only if there exists an n0 > 0, such that for n > n0,
with the remnant being at most ~(x - b)n + 1.
Next, following van der Corput [2], we define a neutrix as a class of negligible functions defined in a domain, which satisfies the following two conditions: (1) the neutrix is an additive group; (2) it does not contain any constant except 0. Let us illustrate the concept with the following example considered by Hadamard: for s real,
For s > 0, the integral converges even as ξ → 0. For s ≤ 0, Hadamard neglects ξs/s and log ξ as ξ → 0. Here we have a neutrix which we will call N(0), consisting of functions ν(ξ) =
(ξ) + c1ξs + c2log ξ, where
(ξ) → 0 as ξ → 0, and where c1, c2 and s are arbitrary constants. This results in writing
Note the analytic extension in the complex s plane of the answer for Re s > 0 to the entire complex plane with the exclusion of s = 0.
Before applying neutrices to QED, we need to consider the generalized Hadamard neutrix Ha defined to contain the negligible functions
where
(ξ) → 0 as ξ → a. Each of the functions U(ξ) is defined by an asymptotic series based on a:
Here χh, Ψh and integers kh ≥ 0 are independent of ξ, Re Ψh → ∞ as h → ∞ and
stands for
. An example is provided by
Similarly, we can define the Hadamard neutrix H∞ by equation (4) where now
(ξ) → 0 as ξ → ∞ and the function U(ξ) has a Hadamard development in powers of ξ - 1 in its asymptotic series:
where Re Ψh → - ∞ as h → ∞.
We can now demonstrate a very valuable property of the Hadamard neutrix. Recall that in the theory of distributions developed by Schwartz, generalized functions usually cannot be multiplied. Consider, for example, the one-dimensional Dirac delta function multiplying itself δ(x) × δ(x). This product is not mathematically meaningful because its Fourier transform diverges
where we have used the convolution rule in Fourier transform and have noted that the Fourier transform of the Dirac delta function is 1. In contrast, the Hadamard method does allow multiplication for a wide class of distributions. For the example of δ(x) × δ(x), the Hadamard-neutralized Fourier transform of the product
yields
a mathematically meaningful (though somewhat counter-intuitive) result!
In doing quantum field theory in configuration space, we multiply operator-valued distributions of quantum fields. Or, in a slightly different interpretation, we multiply singular functions such as Feynman propagators. As we will see, the use of neutrix calculus allows one to put these products on a mathematically sound basis. Let us now generalize the above discussion for one-dimensional Dirac delta functions to the case of (3 + 1)-dimensional Feynman propagators
where H(2) is the Hankel function of the second kind and we use the ( + + + - ) metric. The Fourier transform of Δ + (x) × Δ + (x) (which appears in certain quantum loop calculations) is given by
where
with the second expression of D obtained after a Wick rotation. But D is logarithmically divergent. Hence Δ + (x) × Δ + (x) is not mathematically well defined. Let us now see how the Hadamard-van der Corput method gives mathematical meaning to this product. Obviously, it is in the calculation of the logarithmically divergent D where we apply neutrix calculus. Introducing the dimensionless variable q = k2/m2, we bring in H∞ to write D as
where we have recalled that, for q → ∞, log q is negligible in the Hadamard neutrix H∞. It follows that, in the neutralized version, Δ + (x) × Δ + (x) ~ δ(4)(x) + regular part (where δ(4)(x) is the four-dimensional Dirac delta function), a much more mathematically palatable object.
As the first example in the application of neutrices to QED, let us consider the one-loop contribution to the electron's self-energy
where m is the electron bare mass and we have given the photon a fictitious mass λ to regularize infrared divergences. Expanding Σ(p) about γ · p = - m,
one finds (cf results found in [5])
where α = e2/4π is the fine structure constant and D is given by equations (15) and (16) in the pre-neutralized and neutralized forms, respectively. We note that
, the last piece of Σ(p) in equation (18), is finite. Mass renormalization and wavefunction renormalization are given by
and ψren = Z - 1/22ψ respectively with
. Now, since D = - 1 is finite, it is abundantly clear that the renormalizations are finite in the framework of neutrix calculus. There is no need for a separate discussion of the electron vertex function renormalization constant Z1 due to the Ward identity Z1 = Z2.
The one-loop contribution to vacuum polarization is given by
A standard calculation [5] shows that Πμν takes on the form
where ημν is the flat metric ( + + + - ),
and
with
and D given by equation (15). Just as D is rendered finite upon invoking neutrix calculus (see equation (16)), so is D ':
since both q and log q, for q → ∞, are negligible in H∞. Thus neutrix calculus yields a finite renormalization for both the photon mass and the photon wavefunction Aμren = Z - 1/23 Aμ (and consequently also for charge eren = Z1/23 e) where Z - 13 = 1 - Π(0). In electron-electron scattering by the exchange of a photon with energy-momentum k, vacuum polarization effects effectively replace e2 by e2/(1 - Π(k2)), i.e.,
Equation (24) can be used, for k2
m2, to show that
Thus we have obtained the correct running of the coupling [6] with energy-momentum in the framework of neutrices. In fact, the only effect of neutrix calculus, when applied to QED (and other renormalizable theories), is to convert infinite renormalizations (obtained without using neutrix calculus) to mathematically well-defined finite renormalizations. As far as we can tell, all (finite) physically observable results of QED are recovered. In passing we mention that the use of neutralized integrals does not affect the results of axial triangle anomalies.
As shown by the appearance of photon mass in the above discussion of vacuum polarization, the application of neutrix calculus to the energy-momentum cutoff regularization, though straightforward and natural, is ill suited for more complicated theories like those involving Yang-Mills fields. For those theories, one should use other more convenient regularization schemes. It is amusing to note that already in 1961 van der Corput suggested that, instead of finding the appropriate neutrices, one can continue analytically in any variable (presumably including the dimension of integrations) contained in the problem of tackling apparent divergences to calculate the coefficients of the corresponding asymptotic series. In hind sight, one recognizes that this was the approach taken by 't Hooft and Veltman who spearheaded the use of dimensional regularizations [6]. Let us now explore using neutrix calculus in conjunction with the dimensional regularization scheme. In that case, negligible functions will include 1/
where
= 4 - n is the deviation of spacetime dimensions from 4. In the one-loop calculations for QED, the internal energy-momentum integration is now over n dimensions. The forms of Σ(p) and Πμν remain the same as given by equations (18) and (22), but now with δm2 = 0. Using the approximation for the gamma function,
, where γ ≊ 0.577 is the Euler-Mascheroni constant, and the approximation f
≊ 1 +
log f, for
1, one finds
where D0 = m2x2 + λ2(1 - x), and
By design, the generalized neutrix calculus renders all the renormalizations finite. Again, all physically measurable results of QED appear to be recovered. In this letter we have explicitly considered QED to one-loop only. But we expect that higher-loop calculations can be handled in the same way according to neutrix calculus. It will be interesting to see explicitly whether neutrix calculus, applied to higher-loop calculations, can provide new insights in the issue of overlapping divergences.
In the framework of quantum field theory for the four fundamental forces, the divergence problem is particularly severe for quantum gravity. Using dimensional regularization, 't Hooft and Veltman [7] found that pure gravity is one-loop renormalizable, but in the presence of a scalar field, renormalization was lost. For the latter case, they found that the counterterm evaluated on the mass shell is given by
with R being the Ricci scalar. Similar results for the cases of Maxwell fields and Dirac fields etc (supplementing the Einstien field) were obtained [8]. It is natural to enquire whether the application of neutrix calculus could improve the situation. The result is that now essentially the divergent
- 1 factor is replaced by - γ + constant.
It has not escaped our notice that neutrix calculus may ameliorate the hierarchy problem in particle physics. The hierarchy problem is due to the fact that the Higgs scalar self-energies diverge quadratically, leading to a stability problem in the standard model of particle physics. But neutrix calculus treats quadratic divergences no different from logarithmic divergences, since both divergences belong to (the negligible functions of) the neutrix. Neutrix calculus may also ameliorate the cosmological constant problem in quantum gravity. The cosmological constant problem can be traced to the quartic divergences in zero-point fluctuations from all quantum fields. But again, neutrix calculus treats quartic divergences no different from logarithmic divergences. Indeed, for a theory of gravitation with a cosmological constant term, the cosmological constant receives at most a finite renormalization from the quantum loops in the framework of neutrix calculus.
We conclude with a comment on what neutrix calculus means to the general question of renormalizability of a theory. We recall that a theory is renormalizable if, in loop calculations, the counterterms vanish or if they are proportional to terms in the original Lagrangian (the usual renormalization through rescaling). It is still renormalizable if, to all loops, the counterterms are of a new form, but only a finite number of such terms exist. By this standard, neutrix calculus does not change the renormalizability of a theory, since it merely changes potentially infinite renormalizations to finite renormalizations. On the other hand, non-renormalizable terms, i.e., terms with positive superficial degree of divergence, are tolerated in neutralized quantum field theory. In a sense it is a pity that we have lost renormalizability as a physical restrictive criterion in the choice of sensible theories. However, we believe that this is actually not as big a loss as it may first appear. Quite likely, all realistic theories now in our possession are actually effective field theories [9, 10]. They appear to be renormalizable field theories because, at energies now accessible, or more correctly, at sufficiently low energies, all the non-renormalizable interactions are highly suppressed. By tolerating non-renormalizable terms, neutrix calculus has freed us from the past dogmatic and rigid requirement of renormalizability. (Having said that, given a choice between renormalizable field theories and effective field theories, we still prefer the former to the latter because of the former's compactness and predictive power. But the point is that both types of theories can be accommodated in the framework of neutrix calculus.) Furthermore, if the application of neutrix calculus to loop calculations results in a term of a new form (like the Pauli term in QED) that is finite, then we have a prediction which, in principle, can be checked against experiments to confirm or invalidate the theory in question. For the latter case, we will have to modify the theory by including a term of that form in the Lagrangian, making the parameter associated with the new term an adjustable parameter rather than one that is predicted by the theory. This loss of predictive power is again not as big a loss as one may dread.
Lastly we should emphasize that, for renormalizable theories as well as non-renormalizable theories (like quantum gravity?), neutrix calculus is a useful tool to the extent that it is relevant for asymptotic series and lessens the divergence of the theories. On the basis of our study so far, we tentatively conclude that neutrix calculus has banished infinities from quantum field theory, rendering perturbative quantum field theory mathematically meaningful.
Acknowledgments
We thank J J Duistermaat E M de Jager T Levelt and T W Ruijgrok for encouragement and for kindly providing us with relevant references of the work by J G van der Corput. We thank C Bender and K A Milton for useful discussions. We also thank L Ng and X Calmet for their help in the preparation of this manuscript. We are grateful to the late Paul Dirac and Julian Schwinger for inspiring us to look for a better mathematical foundation for quantum field theory. This work was supported in part by DOE and by the Bahnson Fund of University of North Carolina at Chapel Hill.
ReferencesY Jack Ng and H van Dam 2005 J. Phys. A: Math. Gen. 38 L317
A Jaroń-Becker et al 2003 J. Phys. B: At. Mol. Opt. Phys. 36 L375
M A Furman 2006 New J. Phys. 8 279
Jonathan P. Gardner et al. 2000 The Astronomical Journal 119 486
T. H. Jarrett et al. 2007 The Astronomical Journal 133 979
J. T. Armstrong et al. 2001 The Astronomical Journal 121 476
J Kikuchi et al 2004 J. Phys.: Condens. Matter 16 L167
Lars M Johansen 2004 J. Opt. B: Quantum Semiclass. Opt. 6 L21
Debra A. Fischer and Jeff Valenti 2005 ApJ 622 1102
Peter F Nelson 2009 Environ. Res. Lett. 4 041002