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What is Quantum Field Theory, and What Did We Think It Is?
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This is a talk presented at the conference ``Historical and Philosophical Reflections on the Foundations of Quantum Field Theory,'' at Boston University, March 1996. It will be published in the proceedings of this conference.
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Cited by 6 Pith papers
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Twisted Feynman Integrals: from generating functions to spin-resummed post-Minkowskian dynamics
Twisted Feynman integrals are introduced with graded Symanzik polynomials, classified as exponential periods, and shown to have geometry not inferable from generalized Baikov leading singularities.
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Path integral measure and RG equations for gravity
With a corrected path-integral measure and an on-shell running scale, the Einstein-Hilbert truncation of quantum gravity has only the Gaussian fixed point, removing the asymptotic safety fixed point.
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Scattering Observables from Few-Body Densities and Application in Light Nuclei
TDA factorization with public DensityScattering code and SRG-And-Back scheme yields scattering observables on 3H, 3He, 4He, 6Li from chiral potentials with uncertainties below 6%.
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Gravitational form factors of the Higgs boson
The one-loop electroweak gravitational form factors of the Higgs give a finite theta2 and an energy radius r^2 approximately 1.44e-6 GeV^-2, with theta1 requiring an EFT counterterm.
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Diffeomorphism invariance of the effective gravitational action
A careful calculation shows that the Fradkin-Vilkovisky path integral measure is diffeomorphism invariant, while the Fujikawa measure is not.
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From Nuclear Matter with Quenched $g_A$ to Compact-Star Matter with a Signal for Emergent Hidden Scale Symmetry
The paper argues that quenched g_A ≈ 1 in nuclei and the pseudo-conformal sound speed v_s^2/c^2 ≈ 1/3 in compact stars are parallel signals of one emergent hidden scale symmetry.
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