Frontiers of Dark Energy

TL;DR

This paper reviews the current understanding of dark energy, its possible origins, and how cosmological observations can help distinguish between different theoretical models of cosmic acceleration.

Contribution

It discusses how to connect theoretical models of dark energy with observational data and explores the frontiers of new physics revealed by current and upcoming experiments.

Findings

Dark energy causes accelerated cosmic expansion.

Observations can differentiate between vacuum and alternative dark energy models.

Current data illuminates new physics frontiers.

Abstract

Cosmologists are just beginning to probe the properties of the cosmic vacuum and its role in reversing the attractive pull of gravity to cause an acceleration in the expansion of the cosmos. The cause of this acceleration is given the generic name of dark energy, whether it is due to a true vacuum, a false, temporary vacuum, or a new relation between the vacuum and the force of gravity. Despite the common name, the distinction between these origins is of utmost interest and physicists are actively engaged in finding ways to use cosmological observations to distinguish which is the true, new physics. Here we will discuss how to relate the theoretical ideas to the experimental constraints, how to understand the influences of dark energy on the expansion and structure in the universe, and what frontiers of new physics are being illuminated by current and near-term data.