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2011, Physical Review D
We show how expansions in powers of Planck's constant = h/2π can give new insights into perturbative and nonperturbative properties of quantum field theories. Since is a fundamental parameter, exact Lorentz invariance and gauge invariance are maintained at each order of the expansion. The physics of the expansion depends on the scheme; i.e., different expansions are obtained depending on which quantities (momenta, couplings and masses) are assumed to be independent of. We show that if the coupling and mass parameters appearing in the Lagrangian density are taken to be independent of , then each loop in perturbation theory brings a factor of. In the case of quantum electrodynamics, this scheme implies that the classical charge e, as well as the fine structure constant are linear in. The connection between the number of loops and factors of is more subtle for bound states since the binding energies and bound-state momenta themselves scale with. The expansion allows one to identify equal-time relativistic bound states in QED and QCD which are of lowest order in and transform dynamically under Lorentz boosts. The possibility to use retarded propagators at the Born level gives valence-like wave-functions which implicitly describe the sea constituents of the bound states normally present in its Fock state representation.
We show that Schwinger's trick in quantum field theory can be extended to obtain the expression of the partition functions of a class of scalar theories in arbitrary dimensions. These theories correspond to the ones with linear combinations of exponential interactions, such as the potential $\mu^D\exp(\alpha\phi)$. The key point is to note that the exponential of the variation with respect to the external current corresponds to the translation operator, so that $$\exp\big(\alpha{\delta\over \delta J(x)}\big) \exp(-Z_0[J]) = \exp(-Z_0[J+\alpha_x])$$ We derive the scaling relations coming from the renormalization of $\mu$ and compute $\langle \phi(x)\rangle$, suggesting a possible role in a non-perturbative framework for the Higgs mechanism. It turns out that $\mu^D\exp(\alpha\phi)$ can be considered as master potential to investigate other potentials, such as $\lambda\phi^n$.
Physical review, 1975
The quantum mechanics of solitary-wave classical solutions of nonlinear wave equations is discussed in detail for the kink solution of two-dimensional P' field theory. The formalism provides a natural interpretation of an extended particle, the soliton, for the classical kink. The perturbation theory around the extended particle is developed and used to calculate the radiative corrections for the mass of soliton up to one loop. The mass renormalization is discussed in detail to show that the mass counterterm to the nonsoliton sector also does the job for the present case, i.e. one-soliton sector. Although our formalism is not manifestly Lorentzcovariant, the Lorentz covariance is shown explicitly by calculating the soliton energy for a fixed momentum. The paper also contains the perturbation calculation of matrix element of P fields between one-soliton states.
International Journal of Modern Physics A, 2001
This talk introduces perturbative quantum field on a heuristic level. It is directed at an audience familiar with elements of quantum mechanics, but not necessarily with high energy physics. It includes a discussion of the strategies behind experimental tests of fundamental theories, and of the field theory interpretations of these tests.
Physical review, 2016
Schwinger's formalism in quantum field theory can be easily implemented in the case of scalar theories in D dimension with exponential interactions, such as µ D exp(αφ). In particular, we use the relation exp α δ δJ(x) exp(−Z 0 [J]) = exp(−Z 0 [J + α x ]) with J the external source, and α x (y) = αδ(y − x). Such a shift is strictly related to the normal ordering of exp(αφ) and to a scaling relation which follows by renormalizing µ. Next, we derive a new formulation of perturbation theory for the potentials V (φ) = λ n! : φ n :, using the generating functional associated to : exp(αφ) :. The ∆(0)-terms related to the normal ordering are absorbed at once. The functional derivatives with respect to J to compute the generating functional are replaced by ordinary derivatives with respect to auxiliary parameters. We focus on scalar theories, but the method is general and similar investigations extend to other theories.
Nuclear Physics B, 1970
The connection between the field theory and the perturbation expansion of quantum electrodynamics is studied. As a starting point the usual Lagrangian is taken but with bare electron mass and the renormalization constant Z3 set equal to zero. This theory is essentially equivalent to the usual one; however, it does not contain any constant of nature and is dilatational and gauge invariant, both invariances being spontaneously broken. The various limiting procedures implied by the differentiation, the multiplication and the renormalization of the field operators in the Lagrangian are combined in a gauge invariant way to a single limit. Propagator equations are derived which are the usual renormalized ones, except for: (i) a natural cancellation of the quadratic divergence of the vacuum polarization; (ii) the presence of an effective cutoff at p ≈ ɛ-1; (iii) the replacement of the renormalization constants Z1 and Z2 by one gauge dependent function Z( ɛ2); (iv) the limit ɛ → 0 which has to be taken. The value Z(0) corresponds to the usual constants Z1 and Z2. It is expected that in general Z(0) = 0, but this poses no problem in the present formulation. It is argued that the function Z( ɛ2), which is determined by the equations, may render the vacuum polarization finite. One may eliminate the renormalization function from the propagator equations and then perform the limit ɛ → 0; this results in the usual perturbation series. However, the renormalization function is essential for an understanding of the high momentum behaviour and of the relation between the field theory and the perturbation expansion.
Nuclear Physics B, 1978
We construct an effective Hamiltonian at fixed momentum which can be used to calculate higher-order corrections to quantum states of localized classical solutions of scalar field theories in 1 + 1 dimensions. We use the quantization scheme discussed first by Creutz and also by Rothe and one of the present authors (J.B.). The effective Hamiltonian is similar to, but nevertheless different from the one obtained in the collective coordinate method. The agreement of the energy corrections at the two-loop level has been checked.
Cornell University - arXiv, 2020
A formal expansion for the Green's functions of an interacting quantum field theory in a parameter that somehow encodes its "distance" from the corresponding non-interacting one was introduced more than thirty years ago, and has been recently reconsidered in connection with its possible application to the renormalization of non-hermitian theories. Besides this new and interesting application, this expansion has special properties already when applied to ordinary (i.e. hermitian) theories, and in order to disentangle the peculiarities of the expansion itself from those of non-hermitian theories, it is worth to push further the investigation limiting first the analysis to ordinary theories. In the present work we study some aspects related to the renormalization of a scalar theory within the framework of such an expansion. Due to its peculiar properties, it turns out that at any finite order in the expansion parameter the theory looks as non-interacting. We show that when diagrams of appropriate classes are resummed, this apparent drawback disappears and the theory recovers its interacting character. In particular we have seen that with a certain class of diagrams, the weak-coupling expansion results are recovered, thus establishing a bridge between the two expansions.
Communications in Mathematical Physics, 2001
The perturbative treatment of quantum field theory is formulated within the framework of algebraic quantum field theory. We show that the algebra of interacting fields is additive, i.e. fully determined by its subalgebras associated to arbitrary small subregions of Minkowski space. We also give an algebraic formulation of the loop expansion by introducing a projective system A (n) of observables "up to n loops" where A (0) is the Poisson algebra of the classical field theory. Finally we give a local algebraic formulation for two cases of the quantum action principle and compare it with the usual formulation in terms of Green's functions.
NATO Science Series: B:, 2002
We review our recent work, hep-th/9803030, on the constraints imposed by global or local symmetries on perturbative quantum field theories. The analysis is performed in the Bogoliubov-Shirkov-Epstein-Glaser formulation of perturbative quantum field theory. In this formulation the S-matrix is constructed directly in the asymptotic Fock space with only input causality and Poincaré invariance. We reformulate the symmetry condition proposed in our earlier work in terms of interacting Noether currents.
OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information), 2018
The European Physical Journal C, 2001
In several preceding studies, the explicitly covariant formulation of light front dynamics was developed and applied to many observables. In the present study we show how in this approach the renormalization procedure for the first radiative correction can be carried out in a standard way, after separating out the contributions depending on the orientation of the light-front plane. We calculate the renormalized QED vertices γe − → e − and e + e − → γ and the electron self-energy and recover, in a straightforward way, the well known analytical results obtained in the ¿Feynman approach.
The European Physical Journal H, 2011
Relativistic quantum field theory is generally recognized to form the adequate theoretical frame for subatomic physics, with the Standard Model of Particle Physics as a major achievement. We point out that quantum field theory in its present form is not a monolithic theory, but rather consists of distinct facets, which aim at a common ideal goal. We give a short overview of the strengths and limitations of these facets. We emphasize the theory-dependent relation between the quantum fields, and the basic objects in the empirical domain, the particles. Given the marked conceptual differences between the facets, we argue to view these, and therefore also the Standard Model, as symbolic constructions. We finally note that this view of physical theories originated in the 19th century and is related to the emergence of the classical field as an autonomous concept.
In this paper the nonperturbative analysis of the spectrum for one-particle excitations of the electronpositron field (EPF) is considered in the paper. A standard form of the quantum electrodynamics (QED) is used but the charge of the "bare" electron e0 is supposed to be of a large value (e0 ≫ 1). It is shown that in this case the quasi-particle can be formed with a non-zero averaged value of the scalar component of the electromagnetic field (EMF). Self-consistent equations for the distribution of charge density in the "physical" electron (positron) are derived. A variational solution of these equations is obtained and it defines the finite renormalization of the charge and mass of the electron (positron). It is found that the coupling constant α0 between EPF and EMF and mass m0 of the "bare" electron can be connected with the observed values of the fine structure constant α and the mass of the "physical" electron m as follows (h = c = 1): 2
Zenodo (CERN European Organization for Nuclear Research), 2024
This analysis shows that divergence issues in QFT can be resolved without mass and charge renormalization by postulating a two-component theory of the vacuum whose net energy and charge are zero. For the free fields, the quantum vacuum is uniformly homogeneous and isotropic, but interacting fields break the uniformity as vacuum energy is redistributed. For an irreducible self-interaction amplitude Ω, infinite field actions divide the vacuum into positive and negative self-energy components such that the net vacuum energy correction to a scattering process is finite in the presence of external fields but vanishes for free particles. For each particle mass in a loop, two mass states dressed with vacuum energy, are constructed for fermion and boson self-energy processes. For electroweak interactions, the stabilized amplitude Ω^ = Ω - <Ω> includes a correction for a vacuum energy deficit within an infinitesimal near-field (INF) region, where <Ω> is given by an average of Ω over dressed mass levels. For QCD, strong interactions redistribute vacuum energy so that there is a surplus in the INF with a corresponding deficit in the surrounding far-field resulting in a sign reversal of Ω^ relative to QED and asymptotic freedom. Stabilized amplitudes are shown to agree with renormalization for radiative corrections in Abelian and non-Abelian gauge theories.
Lecture Notes in Physics, 2007
We comment on the present status, the concepts and their limitations, and the successes and open problems of the various approaches to a relativistic quantum theory of elementary particles, with a hindsight to questions concerning quantum gravity and string theory.
2002
This paper proves that it is possible to build a Lagrangian for quantum electrodynamics which makes it explicit that the photon mass is eventually set to zero in the physical part on observational ground. Gauge independence is achieved upon considering the joint effect of gauge-averaging term and ghost fields. It remains possible to obtain a counterterm Lagrangian where the only non-gauge-invariant term is proportional to the squared divergence of the potential, while the photon propagator in momentum space falls off like k −2 at large k which indeed agrees with perturbative renormalizability. The resulting radiative corrections to the Coulomb potential in QED are also shown to be gauge-independent.
2021
Present day quantum field theory (QFT) is founded on canonical quantization, which has served quite well, but also has led to several issues. The free field describing a free particle (with no interaction term) can suddenly become nonrenormalizable the instant a suitable interaction term appears. For example, using canonical quantization, φ 4 4, has been deemed a “free” theory with no difference from a truly free field [1, 2, 3]. Using the same model, affine quantization has led to a truly interacting theory [4]. This fact alone asserts that canonical and affine tools of quantization deserve to be open to their procedures together as a significant enlargement of QFT.
Physics Letters B, 1993
The true variables in QED are the transverse photon components and Dirac's physical electron, constructed out of the fermionic field and the longitudinal components of the photon. We calculate the propagators in terms of these variables to one loop and demonstrate their gauge invariance. The physical electron propagator is shown not to suffer from infrared divergences in any gauge. In general, all physical Green's functions are gauge invariant and infrared-finite.
Modern Physics Letters A, 2006
It has been argued by Dyson that the perturbation theory in coupling constant in QED cannot be convergent. We find that similar albeit slightly different arguments lead to the divergence of the series of 1/N f expansion in QED.
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