Dynamics with Infinitely Many Derivatives: The Initial Value Problem
arXiv:0709.3968 · doi:10.1088/1126-6708/2008/02/008
Abstract
Differential equations of infinite order are an increasingly important class of equations in theoretical physics. Such equations are ubiquitous in string field theory and have recently attracted considerable interest also from cosmologists. Though these equations have been studied in the classical mathematical literature, it appears that the physics community is largely unaware of the relevant formalism. Of particular importance is the fate of the initial value problem. Under what circumstances do infinite order differential equations possess a well-defined initial value problem and how many initial data are required? In this paper we study the initial value problem for infinite order differential equations in the mathematical framework of the formal operator calculus, with analytic initial data. This formalism allows us to handle simultaneously a wide array of different nonlocal equations within a single framework and also admits a transparent physical interpretation. We show that differential equations of infinite order do not generically admit infinitely many initial data. Rather, each pole of the propagator contributes two initial data to the final solution. Though it is possible to find differential equations of infinite order which admit well-defined initial value problem with only two initial data, neither the dynamical equations of p-adic string theory nor string field theory seem to belong to this class. However, both theories can be rendered ghost-free by suitable definition of the action of the formal pseudo-differential operator. This prescription restricts the theory to frequencies within some contour in the complex plane and hence may be thought of as a sort of ultra-violet cut-off.
40 pages, no figures. Added comments concerning fractional operators and the implications of restricting the contour of integration. Typos corrected
References in corpus (13)
- The Lee-Wick Standard Model
- Non-perturbative Gravity, Hagedorn Bounce & CMB
- Route to nonlocal cosmology
- Comments on Marginal Deformations in Open String Field Theory
- Bouncing and Accelerating Solutions in Nonlocal Stringy Models
- Dynamics in Nonlocal Cosmological Models Derived from String Field Theory
- Fading Gravity and Self-Inflation
- Nonlinear equations for p-adic open, closed, and open-closed strings
- Stretching the Inflaton Potential with Kinetic Energy
- Quantization of the Riemann Zeta-Function and Cosmology
- Rolling to the tachyon vacuum in string field theory
- Rolling Tachyon in Nonlocal Cosmology
- Disk Partition Function and Oscillatory Rolling Tachyons
Cited by in corpus (11)
- Cosmology of the Lifshitz universe
- Dynamics of Nonlocal Cosmology
- Newtonian limit of nonlocal cosmology
- Diffusing non-local inflation: Solving the field equations as an initial value problem
- Twisted Noncommutative Field Theory with the Wick-Voros and Moyal Products
- Predictions for Nongaussianity from Nonlocal Inflation
- Dynamics in nonlocal linear models in the Friedmann-Robertson-Walker metric
- Kinks of open superstring field theory
- Dynamics and Stability of Light-Like Tachyon Condensation
- Zeta Nonlocal Scalar Fields
- Towards effective Lagrangians for adelic strings