Inflation theory posits that the universe grew exponentially from quantum fluctuations to astronomical scales producing gravitational waves. The primary goal of CLASS is to detect and characterize the polarization pattern (“B-modes”) expected to be imprinted on the CMB by the inflationary gravitational waves. CLASS is unique in its goal to measure B-modes over the full range of angular scales affected by these primordial waves and also over a range of wavelengths (1.4–7 mm) that allows CLASS to distinguish the primordial B-modes from local polarized emission from our galaxy.
When the universe was less than a tenth of its current age, stars in the first galaxies formed. They emitted light that ionized the intergalactic gas during an epoch called reionization. This ionized gas adds further polarization to the CMB. By measuring this polarization, CLASS will determine when galaxies first lit up.
Neutrinos are among the lightest and most elusive particles in nature. Like the CMB, a cosmic neutrino background pervades space as a relic of the early universe and affects the growth of cosmic large-scale structure (LSS). The CLASS result on reionization together with CMB intensity data constrain the primordial density fluctuations from which the LSS grew. Comparing these primordial seeds of LSS to measurements of the LSS itself provides powerful insights into the neutrino (specifically its mass).
The CMB travels to us over 13.77 billion years from the edge of the observable universe. During this long journey, subtle processes, previously undetected, can alter the CMB polarization in measurable ways. Grand Unified Theories predict the generation of new forms of energy (quantum fields) in the early universe that could interact with the CMB (e.g., by a Chern-Simons mechanism) to rotate its linear polarization, an effect that CLASS is well suited to measure. In this way, CLASS searches for new fundamental interactions and pushes the boundaries of physical theory.
Measurements of the CMB intensity have led to claims of cosmic anomalies at large angular scales. Whether these claims result from statistical flukes or point the way to new physics beyond current theories can be determined by checking whether the purported intensity anomalies have associated polarization anomalies at large angular scales. The CLASS polarization measurement is uniquely positioned to answer this exciting question.
The CLASS survey will also improve our understanding of our Milky Way The proposed survey images 70% of the sky, an area including much of the Milky Way and the nearby Magellanic Clouds.
The CLASS data will be made publicly available. Because it covers nearly the entire sky, the CLASS data will combine with other astronomical surveys to extend the scientific impact beyond our project’s substantial intrinsic benefits.