Hadron era

A long time ago, the world was very hot. It was too hot for anything to live.

Tiny bits of stuff moved very fast. These bits were not yet joined together.

Then, the world cooled down a little. The bits began to join into pairs.

These pairs were made of matter and anti-matter. They stayed in a balance.

Soon, the heat dropped even more. The pairs hit each other and went away.

This left the world full of light and tiny bits. It was a very busy time.

A long time ago, the universe was very hot. Scientists used to think of a time called the hadron era. This era happened at the very start of everything. It began at a tiny fraction of a second. It ended at 10^-4 seconds.

During this time, the heat was very high. This heat made pairs of hadrons and anti-hadrons. Hadrons are tiny bits of matter. Anti-hadrons are the opposite kind of matter. These two kinds stayed in a balance.

Before this, the universe was in the quark epoch. In that time, it was too hot for hadrons to form. Quarks are even smaller bits. Quarks did not join together yet.

Then, the temperature began to drop. This change happened near 7x10^-5 seconds. When it cooled, the matter and anti-matter hit each other. This is called annihilation. This process makes the pairs go away.

After they went away, the universe changed again. This new time is called the lepton era. The universe was then full of light and neutrinos. Neutrinos are tiny bits that move through space.

The hadron era was a time in a very old idea about the universe. This idea is now considered obsolete, or out of date. It describes a specific part of the very early universe. Scientists once thought this era began at 10^-44 seconds or 10^-8 seconds. It lasted until about 10^-4 seconds had passed. This period helps us think about how the universe changed.

During this era, the universe was incredibly hot. This heat allowed for the creation of hadron and anti-hadron pairs. Hadrons are tiny bits of matter. Anti-hadrons are the opposite kind of matter. These pairs kept matter and anti-matter in thermal equilibrium. This means they stayed in a steady balance. The heat was the main thing driving this balance.

Our understanding of this time changed in the 1970s. Scientists discovered quarks and gluons during that decade. This discovery meant the old hadron model no longer made sense. We now know about the quark epoch that came before. During that epoch, the universe was too hot for hadrons. Quarks stayed separate and did not combine yet.

Real numbers help us see how brief this was. Hadron and anti-hadron pairs were only abundant for a short time. This happened between 5x10^-5 seconds and 7x10^-5 seconds. This specific window is called the QCD phase transition. At 7x10^-5 seconds, the temperature dropped below the pion mass. This cooling changed everything in the tiny universe.

As the universe cooled, a big change happened. Most hadrons and anti-hadrons hit each other. This is called an annihilation reaction. These reactions eliminated most of the pairs. This led to a new time called the lepton era. The universe became full of photons and neutrinos. It also had electron-positron pairs.

The hadron era describes a specific period in an obsolete model of the early universe. In physical cosmology, this era represents a stage in how scientists once thought the universe evolved. This model is no longer used because our understanding of subatomic particles has changed. However, studying this era helps us understand how our current models developed. The era was defined by the presence of hadrons and anti-hadrons. These are fundamental building blocks of matter and antimatter.

In this older model, the hadron era had specific starting and ending points. Some versions of the theory say it began at 10^-44 seconds. Other versions suggest it started later, at 10^-8 seconds. The era ended when the universe reached 10^-4 seconds of age. During this time, the universe was extremely hot. This intense heat allowed for the formation of hadron and anti-hadron pairs. These pairs stayed in thermal equilibrium. This means matter and antimatter existed in a steady balance.

To understand the mechanism, we must look at the temperature and particle interactions. High temperatures provided the energy needed to create hadron and anti-hadron pairs. As long as the heat remained high, these particles stayed in equilibrium. However, this balance was temporary. The universe was also undergoing a process called the QCD phase transition. This transition occurred between 5x10^-5 seconds and 7x10^-5 seconds. During this tiny window, hadron and anti-hadron pairs were abundant.

There were distinct stages that preceded and followed this era. Before the hadron era, there was the quark epoch. During the quark epoch, the universe was too hot for hadrons to exist. Quarks were the smaller particles that make up hadrons. Because of the extreme heat, quarks did not combine to form hadrons yet. Once the temperature dropped, the QCD phase transition allowed these particles to form. This transition marked a major change in the state of the universe.

Our scientific understanding changed significantly during the 1970s. During this decade, researchers discovered quarks and gluons. Quarks are the particles that form hadrons. Gluons are the particles that hold them together. This discovery proved that the old hadron-based model no longer made sense. We realized that the era of quarks must come before the era of hadrons. This shifted how cosmologists view the timeline of the early universe.

The end of the era was caused by a drop in temperature. At 7x10^-5 seconds, the temperature fell below the pion mass. A pion is a type of particle related to the structure of hadrons. When this temperature threshold was crossed, a major event occurred. Most of the hadrons and anti-hadrons underwent annihilation reactions. In an annihilation reaction, matter and antimatter destroy each other. This process eliminated most of the hadrons and anti-hadrons from the universe.

This annihilation led to a new period called the lepton era. The universe changed from being dominated by hadrons to being dominated by other particles. After the annihilation, the universe was filled with photons. Photons are particles of light. It was also filled with neutrinos, which are very light particles. Additionally, the universe contained electron-positron pairs. These are electrons and their antimatter counterparts. This transition shows how temperature dictates which particles can exist in the cosmos.