Ultraviolet dimensional reduction of spacetime with zero-point length
نویسندگان
چکیده
Abstract Among the many disparate approaches towards quantum gravity, reduction of spacetime dimension in ultraviolet regime is expected to be a common thread. The spectral defined context diffusion processes on manifold. We show that with zero-point length has 3.5 when characteristic time size length. (negatively) diverges for an even shorter time, thus preventing reliable physical interpretation deep regime. thermodynamic by realizing free energy $$F(\beta )$$ F ( β ) field or ideal gas at finite temperature ( $$\beta ^{-1}$$ - 1 ) D dimensions scales as $$F\sim \beta ^{-D}$$ ∼ D . Using Schwinger’s proper formalism, we incorporating length, reduces 1.5 near Planck scale and then 1 This signifies “phase-transition” which (massless) bosonic four essentially behaves like radiation $$w=1/3$$ w = / 3 low energies, whereas scale, it equivalently having equation state parameter $$w=2$$ 2 Furthermore, can deduced from potential $$V_D(r)$$ V r interaction between two point-like sources separated distance r its scaling depends Comparing behavior conventional Yukawa-like potentials short distances, appears either 2 3 depending use massive massless force carriers probes.
منابع مشابه
Duality and Zero-Point Length of Spacetime
The action for a relativistic free particle of mass m receives a contribution 2mds from a path of infinitesimal length ds. Using this action in a path integral, one can obtain the Feynman propagator for a spinless particle of mass m. Assuming that the path integral amplitude is invariant under the “duality” transformation ds ! LPyds, one can calculate the modified Feynman propagator. I show tha...
متن کاملFinite entanglement entropy from the zero-point area of spacetime
The calculation of entanglement entropy S of quantum fields in spacetimes with horizon shows that, quite generically, S is (a) proportional to the area A of the horizon and (b) divergent. I argue that this divergence, which arises even in the case of Rindler horizon in flat spacetime, is yet another indication of a deep connection between horizon thermodynamics and gravitational dynamics. In an...
متن کاملVacuum polarization in the Schwarzschild spacetime and dimensional reduction
A massless scalar field minimally coupled to gravity and propagating in the Schwarzschild spacetime is considered. After dimensional reduction under spherical symmetry the resulting 2D field theory is canonically quantized and the renormalized expectation values 〈Tab〉 of the relevant energy-momentum tensor operator are investigated. Asymptotic behaviours and analytical approximations are given ...
متن کاملDimensional Reduction via Noncommutative Spacetime: Bootstrap and Holography
Unlike noncommutative space, when space and time are noncommutative, it seems necessary to modify the usual scheme of quantum mechanics. We propose in this paper a simple generalization of the time evolution equation in quantum mechanics to incorporate the feature of a noncommutative spacetime. This equation is much more constraining than the usual Schrödinger equation in that the spatial dimen...
متن کاملInformation-theoretic natural ultraviolet cutoff for spacetime.
Fields in spacetime could be simultaneously discrete and continuous, in the same way that information can. It has been shown that the amplitudes phi(x(n)) that a field takes at a generic discrete set of points x(n) can be sufficient to reconstruct the field phi(x) for all x, namely, if there exists a certain type of natural ultraviolet (UV) cutoff in nature, and if the average spacing of the sa...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: European Physical Journal C
سال: 2022
ISSN: ['1434-6044', '1434-6052']
DOI: https://doi.org/10.1140/epjc/s10052-022-10313-0