
John F. Donoghue- University of Massachusetts Amherst
John F. Donoghue
- University of Massachusetts Amherst
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266
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September 1980 - present
Publications
Publications (266)
The interactions of gravitons with spin-1 matter are calculated in parallel with the well known photon case. It is shown that graviton scattering amplitudes can be factorized into a product of familiar electromagnetic forms, and cross sections for various reactions are straightforwardly evaluated using helicity methods. Universality relations are i...
We consider scattering in quantum gravity and derive long-range classical and quantum contributions to the scattering of light-like bosons and fermions (spin-0, spin-1/2, spin-1) from an external massive scalar field, such as the Sun or a black hole. This is achieved by treating general relativity as an effective field theory and identifying the no...
We consider scattering in quantum gravity and derive long-range classical and quantum contributions to the scattering of light-like bosons and fermions (spin-0, spin-1/2, spin-1) from an external massive scalar field, such as the Sun or a black hole. This is achieved by treating general relativity as an effective field theory and identifying the no...
We explore the properties of non-local effective actions which include
gravitational couplings. Non-local functions originally defined in flat space
can not be easily generalized to curved space. The problem is made worse by the
calculational impossibility of providing closed form expressions in a general
metric. The technique of covariant perturba...
In this survey, we review some of the low energy quantum predictions of general relativity which are independent of details of the yet unknown high-energy completion of the gravitational interaction. Such predictions can be extracted using the techniques of effective field theory.
We show how modern methods can be applied to quantum gravity at low energy. We test how quantum corrections challenge the classical framework behind the equivalence principle (EP), for instance through introduction of nonlocality from quantum physics, embodied in the uncertainty principle. When the energy is small, we now have the tools to address...
We discuss the derivation of the trace anomaly using a non-local effective
action at one loop. This provides a simple and instructive form and emphasizes
infrared physics. We then use this example to explore several of the properties
of non-local actions, including displaying the action for the full non-local
energy-momentum tensor. As an applicati...
We consider the scattering of light-like matter in the presence of a heavy
scalar object (such as the sun or a black hole). By treating general relativity
as an effective field theory we directly compute the non-analytic parts of the
one-loop gravitational amplitude for the scattering of massless scalars or
photons from an external massive scalar f...
We derive the Regge behavior for the forward scattering amplitude in scalar field theory using the method of regions. We find that the leading Regge behavior to all orders can be obtained. Regge physics emerges from a kinematic region that involves the overlap of several modes, so that a careful treatment of the overlap regions is important. The mo...
We discuss cosmological effects of the quantum loops of massless particles,
which lead to temporal non-localities in the equations of motion governing the
scale factor a(t). For the effects discussed here, loops cause the evolution of
a(t) to depend on the memory of the curvature in the past with a weight that
scales initially as 1/(t-t'). As one o...
We compute the leading post-Newtonian and quantum corrections to the Coulomb
and Newtonian potentials using the full modern arsenal of on-shell techniques;
we employ spinor-helicity variables everywhere, use the Kawai-Lewellen-Tye
(KLT) relations to derive gravity amplitudes from gauge theory and use
unitarity methods to extract the terms needed at...
Describing the fundamental theory of particle physics and its applications, this book provides a detailed account of the Standard Model, focusing on techniques that can produce information about real observed phenomena. The book begins with a pedagogic account of the Standard Model, introducing essential techniques such as effective field theory an...
This is a pedagogical introduction to the treatment of quantum general
relativity as an effective field theory. It starts with an overview of the
methods of effective field theory and includes an explicit example. Quantum
general relativity matches this framework and I discuss gravitational examples
as well as the limits of the effective field theo...
We consider the phenomenology of a dimension-four operator that violates
electromagnetic gauge invariance. Its magnitude is severely constrained by the
lack of scattering of very low energy electromagnetic radiation off of the
Cosmic Microwave Background (CMB) and by the lack of an induced mass when
photons propagate in the CMB. We also discuss pos...
In effective field theories it is common to identify the onset of new physics
with the violation of tree-level unitarity. However, we show that this is
parametrically incorrect in the case of chiral perturbation theory, and is
probably theoretically incorrect in general. In the chiral theory, we explore
perturbative unitarity violation as a functio...
We review the present status of CP violation and critically assess the various tests of this symmetry which have been proposed. Future progress in the subject requires new experimental information distinct from the present measurement of the parameter ε. We find that there exist experiments which are potentially feasible, although all such experime...
The SU(3) chiral limit K → ππ matrix elements of the electroweak penguin operators, Q7,8, are determined using hadronic τ decay data, and dispersive and finite energy sum rules.
We show that there is no useful and universal definition of a running
gravitational constant, G(E), in the perturbative regime below the Planck
scale. By consideration of the loop corrections to several physical processes,
we show that the quantum corrections vary greatly, in both magnitude and sign,
and do not exhibit the required properties of a...
In the context of theories where particles can have different limiting
velocities, we review the running of particle speeds towards a common limiting
velocity at low energy. Motivated by the recent OPERA experimental results, we
describe a model where the neutrinos would deviate from the common velocity by
more than do other particles in the theory...
If the fundamental constants of nature have a cosmic spatial variation, there
will in general be extra forces with a preferred direction in space which
violate the equivalence principle. We show that the millimeter-precision Apache
Point Observatory Lunar Laser-ranging Operation provides a very sensitive probe
of such variation that has the capabil...
We display several examples of how fields with different limiting velocities
(the "speed of light") at a high energy scale can nevertheless have a common
limiting velocity at low energies due to the effects of interactions. We
evaluate the interplay of the velocities through the self-energy diagrams and
use the renormalization group to evolve the s...
The use of a running coupling constant in renormalizable theories is well
known, but the implementation of this idea for effective field theories with a
dimensional coupling constant is in general less useful. Nevertheless there are
multiple attempts to define running couplings including the effects of gravity,
with varying conclusions. We sort thr...
Light scalar particles with couplings of sub-gravitational strength, which can generically be called 'dilatons', can produce violations of the equivalence principle. However, in order to understand experimental sensitivities one must know the coupling of these scalars to atomic systems. We report here on a study of the required couplings. We give a...
We motivate the concept of emergent gauge symmetry and discuss ways that this concept can be tested. The key idea is that if a symmetry is emergent, one should look for small violations of this symmetry because the underlying fundamental theory does not contain the symmetry. We describe our recent work implementing this idea in the gravity sector....
We consider possible violations of the equivalence principle through the exchange of a light `dilaton-like' scalar field. Using recent work on the quark-mass dependence of nuclear binding, we find that the dilaton-quark-mass coupling induces significant equivalence-principle-violating effects varying like the inverse cubic root of the atomic number...
We discuss the kinematics of the particles that make up a Reggeon in field theory, using the terminology of the soft collinear effective theory (SCET). Reggeization sums a series of strongly ordered collinear emissions resulting in an overall Reggeon exchange that falls in the Glauber or Coulomb kinematic region. This is an extremely multiscale pro...
We make an estimate of the likelihood function for the Higgs vacuum expectation value (vev) by imposing anthropic constraints on the existence of atoms while allowing the other parameters of the standard model to also be variable. We argue that the most important extra ingredients are the Yukawa couplings, and for the intrinsic distribution of Yuka...
If general relativity is an emergent phenomenon, there may be small
violations of diffeomorphism invariance. We propose a phenomenology of
perturbatively small violations of general relativity by the inclusion of terms
which break general covariance. These can be tested by matching to the
Parametrized Post Newtonian (PPN) formalism. The most sensit...
In this talk, I describe and defend four non-standard claims about four effective field theories, and try to extract some lessons about the limits of effective field theory. The four theses (and a capsule diagnosis given in parentheses) are: 1) Kaon loops are not a reliable part of chiral perturbation theory (dimensional regularization does not kno...
Contaldi et al. [ C. R. Contaldi, M. Peloso, L. Kofman and A. Linde J. Cosmol. Astropart. Phys. 2003 002 ()] have suggested that an initial period of kinetic energy domination in single field inflation may explain the lack of CMB power at large angular scales. We note that in this situation it is natural that there also be a spatial gradient in the...
We explore the available parameter space of the minimal vectorial standard model. In this theory, the gauge currents are initially vectorial but the Higgs sector produces chiral mass eigenstates, leading to a set of heavy right-handed mirror particles. We describe the phenomenology of the residual parameter space and suggest that the model will be...
We motivate and explore the possibility that extra SU(N) gauge groups may exist independently of the Standard Model groups, yet not be subgroups of some grand unified group. We study the running of the coupling constants as a potential evidence for a common origin of all the gauge theories. Several different example are displayed. Some of the multi...
We motivate and explore the possibility that extra SU(N) gauge groups may exist independently of the Standard Model groups, yet not be subgroups of some grand unified group. We study the running of the coupling constants as a potential evidence for a common origin of all the gauge theories. Several different example are displayed. Some of the multi...
We make an estimate of the likelihood function for the Higgs vacuum expectation value by imposing anthropic constraints on the existence of atoms while allowing the other parameters of the Standard Model to also be variable. We argue that the most important extra ingredients are the Yukawa couplings, and for the intrinsic distribution of Yukawa cou...
Based on recent work on nuclear binding, we update and extend the anthropic constraints on the light quark masses, with results that are more tightly constrained than previously obtained. We find that heavy nuclei would fall apart (because the attractive nuclear central potential becomes too weak) if the sum of the light quark masses m_u+m_d would...
Many of the classic problems of particle physics appear in a very different light when viewed from the perspective of the multiverse. Most importantly the two great ``fine tuning'' problems that motivate the field are far less serious when one accounts for the required anthropic constraints which exist in a multiverse. However, the challenge then b...
We use results by Kirilin to comment that in general relativity the nonleading terms in the energy-momentum tensor of a particle depends on the parameterization of the gravitational field. The classical observables are parameterization independent after a change in coordinates. The quantum effects that emerge within the same calculation of the metr...
Chiral perturbation theory supplemented by the Omnes function is employed to
study the strength of the isoscalar central nuclear interaction, G_S, in the
chiral limit vs the physical case. A very large modification is seen, i.e.
eta_s = G_S ~ chiral /G_S ~ physical = 1.37 +- 0.10 . This large effect is seen
to arise dominantly at low energy from th...
In the phenomenological description of the nuclear interaction an important role is traditionally played by the exchange of a scalar I=0 meson, the sigma, of mass 500–600 MeV, which however is not seen clearly in the particle spectrum and which has a very ambiguous status in QCD. I show that a remarkably simple and reasonably controlled combination...
Even if quark and lepton masses are not uniquely predicted by the fundamental theory, as may be the case in the string theory landscape, nevertheless their pattern may reveal features of the underlying theory. We use statistical techniques to show that the observed masses appear to be representative of a scale invariant distribution, rho(m) ~ 1/m....
We use effective field theory techniques to examine the quantum corrections to the gravitational metrics of charged particles, with and without spin. In momentum space the masslessness of the photon implies the presence of non-analytic pieces , q2log(−q2), etc. in the form factors of the energy–momentum tensor. We show how the former reproduces the...
DOI:https://doi.org/10.1103/PhysRevD.71.069904
DOI:https://doi.org/10.1103/PhysRevD.71.069903
We discuss the calculation of the strange magnetic radius of the proton in chiral perturbation theory. In particular we investigate the low energy component of the loop integrals involving kaons. We separate the chiral calculation into a low energy part and a high energy component through use of a momentum space separation scale. This separation sh...
The classical effects that arise from the loop diagrams and the relationship between the classical terms and the long range effects of massless particles were investigated. The loop expansion associates factor of h̄ with each loop, which suggests the tree diagrams to associate with classical physics. It was observed that the presence of classical c...
The acoustic peak in the CMB power spectrum is sensitive to causal processes and cosmological parameters in the early universe up to the time of last scattering. We provide limits on correlated spatial variations of the peak height and peak position and interpret these as constraints on the spatial variation of the cosmological parameters (baryon d...
We present a model-independent determination of the SU(3)F chiral limit values of the K --> pipi matrix elements of the electroweak penguin operators Q7,8 in the Standard Model. This determination is accomplished using a combination of dispersive and finite energy sum rule techniques, with hadronic tau decay data as input. The consistency between i...
DOI:https://doi.org/10.1103/PhysRevD.69.129901
The standard picture of the loop expansion associates a factor of h-bar with each loop, suggesting that the tree diagrams are to be associated with classical physics, while loop effects are quantum mechanical in nature. We discuss examples wherein classical effects arise from loop contributions and display the relationship between the classical ter...
We discuss the chiral corrections to f_B and B_B with particular emphasis on
determining the portion of the correction that arises from long distance
physics. For very small pion and kaon masses all of the usual corrections are
truly long distance, while for larger masses the long distance portion
decreases. These chiral corrections have been used...
GLOSSARY B meson Elementary particle containing one heavy quark called a b quark as well as a lighter antiquark, or a ¯ b antiquark, and a light quark. The B mesons are about five times more massive than a proton. Charge conjugation invariance Invariance of physical laws under the process of interchanging particle and antiparticle. Decay Elementary...
At very early times, the universe was not in a vacuum state. Under the assumtion that the deviation from equillibrium was large, in particular that it is higher than the scale of inflation, we analyse the conditions for local transitions between states that are related to different vacua. All pathways lead to an attractor solution of a description...
We report on dispersive and finite energy sum rule analyses of the electroweak penguin matrix elements 〈(ππ)2|Q7,8|K0〉 in the chiral limit. We accomplish the correct perturbative matching (scale and scheme dependence) at NLO in αs, and we describe two different strategies for numerical evaluation.
Our dispersive sum rule calculation of the electroweak penguin contribution to ϵ′ϵ is reviewed. A more recent analysis based on the finite-energy sum rule approach is described. Finally, a new determination of the electroweak penguin contribution to ϵ′ϵ is presented.
It is possible that there may be differences in the fundamental physical parameters from one side of the observed universe to the other. I show that the cosmological constant is likely to be the most sensitive of the physical parameters to possible spatial (or temporal) variation, because a small variation in any of the other parameters produces a...
We perform a finite energy sum rule analysis of the flavor ud two-point V–A current correlator, ΔΠ(Q2). The analysis, which is performed using both the ALEPH and OPAL databases for the V–A spectral function, Δρ, allows us to extract the dimension six V–A OPE coefficient, a6, which is related to the matrix element of the electroweak penguin operator...
We perform a finite energy sum rule analysis of the flavor ud two-point V-A current correlator, Delta Pi (Q^2). The analysis, which is performed using both the ALEPH and OPAL databases for the V-A spectral function, Delta rho, allows us to extract the dimension six V-A OPE coefficient, a_6, which is related to the matrix element of the electroweak...
We examine the corrections to the lowest order gravitational interactions of massive particles arising from gravitational radiative corrections. We show how the masslessness of the graviton and the gravitational self interactions imply the presence of nonanalytic pieces sqrt{-q^2}, ln-q^2, etc. in the form factors of the energy-momentum tensor and...
We treat general relativity as an effective field theory, obtaining the full nonanalytic component of the scattering matrix potential to one-loop order. The lowest order vertex rules for the resulting effective field theory are presented and the one-loop diagrams which yield the leading nonrelativistic post-Newtonian and quantum corrections to the...
The pi° â gamma gamma decay width is analyzed within the combined framework of Chiral Perturbation Theory and the 1/N{sub c} expansion up to order(pâ¶) and order(pâ´ x 1/N{sub c}) in the decay amplitude. The eta' is explicitly included in the analysis. It is found that the decay width is enhanced by about 4% due to the isospin-breaking induced m...
We use effective field theory techniques to examine the quantum
corrections to the gravitational metrics of charged particles, with and
without spin. In momentum space the masslessness of the photon implies
the presence of non-analytic pieces ~√-q2,
q2log(-q2), etc. in the form factors of the
energy-momentum tensor. We show how the former reproduce...
We reconsider the dispersive evaluation of the weak matrix elements
<(ππ)I=2Q7,8K0> in the
chiral limit. The perturbative matching is accomplished fully within the
scheme dependence used in the two loop weak OPE calculations. The
effects of dimension eight (and higher dimension) operators are fully
accounted for. We perform a numerical determinatio...
We reconsider the dispersive evaluation of the weak matrix elements (ππ) I=2 |Q 7,8 |K 0 in the chiral limit. The perturbative matching is accomplished fully within the scheme dependence used in the two loop weak OPE calculations. The effects of dimension eight (and higher dimension) operators are fully accounted for. We perform a numerical determi...
Most past work on weak nonleptonic decays has mixed dimensional regularization in the weak operator product expansion with some form of a cutoff regularization in the evaluation of the matrix elements. Even with the usual technique of matching the two schemes, this combination misses physics at short distance which can be described by dimension eig...
I briefly describe two motivations, two mechanisms and two possible tests of the hypothesis that the physical parameters of the ground state of a theory can vary in different rerions of the universe.
I describe recent work with V. Cirigliano and E. Golowich on the effect of dimension eight operators on weak nonleptonic amplitudes. The basic mesage is that there is an inconsistency in the way that many calculations are traditionally performed. If one calculates matrix elements involving only physics below some scale μ, then one needs dimension e...
DOI:https://doi.org/10.1103/PhysRevD.63.059903
According to the weak form of the equivalence principle all objects fall at the same rate in a gravitational field. However, recent calculations in finite-temperature quantum field theory have revealed that at T>0 heavier and/or colder objects actually fall faster than their lighter and/or warmer counterparts. This unexpected result is demonstrated...
We expose a potential flaw in standard treatments of weak decay amplitudes, including that of epsilon'/epsilon. We show that (contrary to conventional wisdom) dimension-eight operators do contribute to weak amplitudes, at order G_F alpha_s and without 1/M_W^2 suppression. We demonstrate the existence of these operators with a simple weak hamiltonia...
One way that an anthropic selection mechanism may be manifest in a physical theory involves multiple domains in the universe with different values of the physical parameters. If this mechanism is to be relevant for understanding the small observed value of the cosmological constant, it may involve a mechanism by which some contributions to the cosm...
We show how the isospin vector and axialvector current spectral functions ρV,3 and ρA,3 can be used to determine in leading chiral order the low energy constants B7(3/2) and B8(3/2). This is accomplished by matching the Operator Product Expansion to the dispersive analysis of vacuum polarization functions. The data for the evaluation of these dispe...
An analysis of electromagnetic corrections to the (dominant) octet K[over →]ππ Hamiltonian using chiral perturbation theory is carried out. Relative shifts in amplitudes at the several percent level are found.
We express the leading electromagnetic corrections in K⃗ππ as integrals over the virtual photon squared momentum Q2. The high Q2 behavior is obtained via the operator product expansion. The low Q2 behavior is calculated using chiral perturbation theory. We model the intermediate Q2 region using resonance contributions in order to enforce the matchi...
We describe the influence of electromagnetism on the phenomenology of decays. This is required because the present data were analyzed without inclusion of electromagnetic radiative corrections,
and hence contain several ambiguities and uncertainties which we describe in detail. Our presentation includes a full description
of the infrared effects ne...
This talk describes some of the consequences for particle phenomenology of the hypothesis that the physical parameters may vary in different domains of the universe.
In kaon decay, electromagnetic radiative corrections can generate shifts in the apparent ΔI=3/2 amplitude of order αA0/A2∼22α. In order to know the true ΔI=3/2 amplitude for comparison with lattice calculations and phenomenology, one needs to subtract off this electromagnetic effect. We provide a careful estimate of the leading electromagnetic shif...
The quantum effective theory of general relativity, independent of the eventual full theory at high energy, expresses graviton-graviton scattering at one loop order O(E^4) with only one parameter, Newton's constant. Dunbar and Norridge have calculated the one loop amplitude using string based techniques. We complete the calculation by showing that...
Baryon chiral perturbation theory as conventionally applied has a well-known problem with the SU(3) chiral expansion in that loop diagrams generate very large SU(3) breaking corrections and greatly upset the subsequent phenomenology. We argue that the problem comes from the portions of loop integrals corresponding to propagation at such short dista...
We have previously analyzed the chiral predictions for the decay KL→π0γe+e- and discussed how experimental measurements of this process can help our understanding of chiral theories and of CP tests. Motivated by the possibility that the analogous muonic process may soon be measurable, we extend this calculation to the decay KL→π0γμ+μ-. Branching ra...
I give a very brief introduction to the use of effective field theory techniques in quantum calculations of general relativity. The gravitational interaction is naturally organized as a quantum effective field theory and a certain class of quantum corrections can be calculated. [Talk presented at the XXVIII International Conference on High Energy P...
There is a "toy" weak matrix element which can be expressed as an integral over the vector and axial vector spectral functions, ae V (s) Gamma ae A (s). I review our recent evaluation of these spectral functions, the study of four "Weinberg" sum rules and the calculation of this matrix element. [Talk presented at the XXVIII International Conference...
In theories in which different regions of the universe can have different values of certain physical parameters, we would naturally find ourselves in a region where they take values favorable for life. We explore the range of such viable values of the mass parameter in the Higgs potential, μ2. For μ2<0, the requirement that complex elements be form...
The use of SU(3) chiral perturbation theory in the analysis of low energy
meson-baryon interactions is discussed. It is emphasized that short distance
effects, arising from propagation of Goldstone bosons over distances smaller
than a typical hadronic size, are model-dependent and can lead to a lack of
convergence in the SU(3) chiral expansion if t...
Baryon chiral perturbation theory as conventionally applied using dimensional regularization has a well-known problem with the convergence of the SU(3) chiral expansion. One can reformulate the theory equally rigorously using a momentum-space cutoff and we show that the convergence is thereby greatly improved for reasonable values of the cutoff. In...
The quantum theory of General Relativity at low energy exists and is of the form called "effective field theory". In this talk I describe the ideas of effective field theory and its application to General Relativity.
One of the puzzles of the Standard Model is why the mass parameter which
determines the scale of the Weak interactions is closer to the scale of QCD
than to the Grand Unification or Planck scales. We discuss a novel approach to
this problem which is possible in theories in which different regions of the
universe can have different values of the phy...
In theories in which the parameters of the low energy theory are not unique, perhaps having different values in different domains of the universe as is possible in some inflationary models, the fermion masses would be distributed with respect to some weight. In such a situation the specifics of the fermion masses do not have a unique explanation, y...
The decay KL→π0γe+e- occurs at a higher rate than the nonradiative process KL→π0e+e-, and hence can be a background to CP violation studies using the latter reaction. It also has interest in its own right in the context of chiral perturbation theory, through its relation to the decay KL→π0γγ. The leading order chiral loop contribution to KL→π0γe+e-...
We provide a new estimate of the long-distance component to the radiative transition BâÏγ. Our mechanism involves the soft scattering of on-shell hadronic products of nonleptonic B decay, as in the chain BâÏÏâÏγ. We employ a phenomenological fit to scattering data to estimate the effect. The specific intermediate states considered here modify...
I discuss the progress in the use of analytic techniques for low energy QCD, in particular as applied to kaon physics. These methods are becoming increasingly powerful and we have gained a good deal of control over the difficult hadronic interactions. There are continuing developments, and I speculate on the ways that these techniques may become ye...
We use dispersive techniques to address the behavior of the pion form factor
as $Q^2 \to \infty$ and $Q^2 \to 0$. We perform the matching with the
constraints of perturbative QCD and chiral perturbation theory in the high
energy and low energy limits, leading to four sum rules. We present a version
of the dispersive input which is consistent with t...
We use the Cottingham method to calculate the pion and kaon electromagnetic mass differences with as few model dependent inputs as possible. The constraints of chiral symmetry at low energy, QCD at high energy and experimental data in between are used in the dispersion relation. We find excellent agreement with experiment for the pion mass differen...
We propose a QCD-based model for calculation of the non-perturbative corrections to the factorization approximation in the decays of heavy mesons. In the framework of the model, factorization in pseudoscalar transitions holds exactly at the leading order leaving the opportunity to calculate non-leading corrections consistently. Comment: 10 pages, R...
By using very general and well established features of soft strong interactions we show, contrary to conventional expectations, that (i) soft final state interactions (FSI) do not disappear for large $m_B$, (ii) inelastic rescattering is expected to be the main source of soft FSI phases, and (iii) flavor off-diagonal FSI are suppressed by a power o...
In quantum field theory there is now a well developed technique, effective field theory, which allows one to obtain low energy quantum predictions in ``non-renormalizable'' theories, using only the degrees of freedom and interactions appropriate for those energies. Whether or not general relativity is truly fundamental, at low energies it is automa...