Related Experiment Video
Updated: Feb 21, 2026

10:00
Gradient Echo Quantum Memory in Warm Atomic Vapor
Published on: November 11, 2013
13.3K
Can a quantum state over time resemble a quantum state at a single time?
Dominic Horsman1, Chris Heunen2, Matthew F Pusey3
1Department of Physics, Durham University, Durham, UK.
Summary
Researchers explored defining a quantum joint state over time to unify space and time treatments in quantum theory. No construction met all criteria, but dropping Hermiticity yielded a unique solution satisfying the rest.
Area of Science:
- Quantum Physics
- Foundations of Quantum Mechanics
- Quantum Information Theory
Background:
- Standard quantum theory treats space and time asymmetrically.
- A joint state for composite systems at different times is not prescribed.
- Defining such a state could enhance the quantum-classical probability analogy.
Purpose of the Study:
- To investigate proposals for a quantum joint state over time.
- To establish criteria for a successful quantum joint state formalism.
- To determine if existing proposals meet these criteria.
Main Methods:
- Analysis of operator-based joint states over time.
- Evaluation of proposals by Leifer and Spekkens, Fitzsimons, Jones, and Vedral.
- Assessment against five defined criteria for a quantum joint state.
Main Results:
- No existing proposal satisfies all five criteria for a quantum joint state over time.
- The criteria include Hermiticity, probabilistic mixing, classical limit, single-time marginals, and associativity.
- Dropping the Hermiticity criterion leads to an essentially unique construction.
Conclusions:
- A universally applicable quantum joint state over time, analogous to composite systems at a single time, is not achievable under current frameworks.
- The requirement of Hermiticity appears to be a key obstacle.
- A modified formalism without Hermiticity offers a viable path forward for a more unified space-time treatment in quantum mechanics.
Related Concept Videos
The Quantum-Mechanical Model of an Atom
60.0K
Shortly after de Broglie published his ideas that the electron in a hydrogen atom could be better thought of as being a circular standing wave instead of a particle moving in quantized circular orbits, Erwin Schrödinger extended de Broglie’s work by deriving what is now known as the Schrödinger equation. When Schrödinger applied his equation to hydrogen-like atoms, he was able to reproduce Bohr’s expression for the energy and, thus, the Rydberg formula governing hydrogen spectra.
60.0K
The de Broglie Wavelength
33.9K
In the macroscopic world, objects that are large enough to be seen by the naked eye follow the rules of classical physics. A billiard ball moving on a table will behave like a particle; it will continue traveling in a straight line unless it collides with another ball, or it is acted on by some other force, such as friction. The ball has a well-defined position and velocity or well-defined momentum, p = mv, which is defined by mass m and velocity v at any given moment. This is the typical...
33.9K
Atomic Nuclei: Nuclear Spin State Overview
2.1K
NMR-active nuclei have energy levels called 'spin states' that are associated with the orientations of their nuclear magnetic moments. In the absence of a magnetic field, the nuclear magnetic moments are randomly oriented, and the spin states are degenerate. When an external magnetic field is applied, the spin states have only 2 + 1 orientations available to them. A proton with = ½ has two available orientations. Similarly, for a quadrupolar nucleus with a nuclear spin value of one, the...
2.1K
The Bohr Model
81.7K
Following the work of Ernest Rutherford and his colleagues in the early twentieth century, the picture of atoms consisting of tiny dense nuclei surrounded by lighter and even tinier electrons continually moving about the nucleus was well established. This picture was called the planetary model since it pictured the atom as a miniature “solar system” with the electrons orbiting the nucleus like planets orbiting the sun. The simplest atom is hydrogen, consisting of a single proton as the...
81.7K
Atomic Nuclei: Types of Nuclear Relaxation
1.0K
Nuclear relaxation restores the equilibrium population imbalance and can occur via spin–lattice or spin–spin mechanisms, which are first-order exponential decay processes.
In spin–lattice or longitudinal relaxation, the excited spins exchange energy with the surrounding lattice as they return to the lower energy level. Among several mechanisms that contribute to spin–lattice relaxation, magnetic dipolar interactions are significant. Here, the excited nucleus transfers...
In spin–lattice or longitudinal relaxation, the excited spins exchange energy with the surrounding lattice as they return to the lower energy level. Among several mechanisms that contribute to spin–lattice relaxation, magnetic dipolar interactions are significant. Here, the excited nucleus transfers...
1.0K
Atomic Nuclei: Nuclear Relaxation Processes
1.3K
In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis, the precessing magnetic moments are randomly oriented around the z-axis.
1.3K

