Why did matter survive the Big Bang's total annihilation?

The Ghostly Particles That May Have Unbalanced the Universe · 11:43 · Video: SciShow · Watch at the source

In short: Shortly after the Big Bang, matter and antimatter should have wiped each other out completely. Yet, galaxies, stars, and humans exist. Scientists now suspect the answer lies within neutrinos—ghostly particles that rarely interact with anything, yet may have tipped the cosmic scales in favor of matter.

The standard model of particle physics suggests that matter and antimatter were present in equivalent quantities during the universe's infancy. Had this equilibrium persisted, total annihilation would have occurred, resulting in nothing besides radiation. Instead, matter somehow survived, a mystery that remains one of the deepest questions in cosmology. This imbalance is a fundamental mystery in cosmology. Without this survival, the cosmos would consist only of radiation.

A recent breakthrough has come from a global collaboration between the T2K experiment in Japan and the NOvA experiment in the United States. By combining years of data from these two massive, long-baseline experiments, researchers achieved unprecedented precision in studying neutrino oscillation. This is the process where neutrinos change their 'flavors' as they travel through space. This joint effort was recently published in the journal Nature. It represents a significant milestone for the scientific community.

This high-precision data offers a potential explanation for why matter triumphed over antimatter. Physicists are looking for a 'crack' in the standard model—the framework that catalogues all known particles and forces. While the standard model is a monumental success, it fails to connect gravity to the other three fundamental forces. Understanding how neutrinos behave might finally reveal why the universe's evolution favored the existence of matter over total annihilation. This research could potentially challenge existing scientific theories. Such findings might necessitate the formulation of a superior model.

Investigating these particles is difficult due to their properties; every second, hundreds of trillions of solar neutrinos traverse the human body, yet they seldom interact. Detecting them requires either incredibly intense sources or massive detectors to catch a rare interaction. These elusive particles are known for being notoriously ghostly. Their incredibly small masses contribute to their elusive nature.

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