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Hadron

The proton, the very building block that makes up the nuclei of every atom you have ever touched, is not a solid sphere but a chaotic, seething storm of energy. This particle, which constitutes the majority of the visible mass in the universe, is actually a composite subatomic particle known as a hadron. It is formed by two up quarks and one down quark, yet these three quarks contribute only a tiny fraction of the proton's total mass. The overwhelming weight of the proton comes from the binding energy of the strong nuclear force, a phenomenon so powerful that it creates a dense soup of massless virtual gluons and transient quark-antiquark pairs that constantly form and vanish within the particle. This internal energy, governed by the laws of quantum chromodynamics, is what gives matter its substance, proving that the solidity of the physical world is an illusion created by the intense activity of the strong force.

A New Name for Old Particles

The term hadron did not exist in the scientific lexicon until the 2nd of May 1962, when Soviet physicist L. B. Okun introduced it during a plenary talk at the International Conference on High Energy Physics at CERN. Before this moment, physicists struggled to categorize a growing zoo of subatomic particles that did not fit into the existing models of leptons or bosons. Okun coined the word from the Greek hadros, meaning thick or bulky, to describe these composite particles that were significantly heavier than electrons. The naming convention was immediately adopted to distinguish these new entities from the fundamental particles that had been known for decades. This linguistic shift marked a pivotal moment in particle physics, as it signaled the transition from a simple view of matter to a complex understanding of how quarks and gluons interact to form the building blocks of the universe.

The Colorless Requirement

Every hadron must possess zero total color charge, a strict rule known as color confinement that dictates how quarks can combine. Quarks carry a property called color charge, which comes in three varieties: red, green, and blue, along with their corresponding anticolors. For a hadron to exist in a stable state, these colors must cancel each other out perfectly, resulting in a colorless or white particle. This cancellation occurs in two primary ways: either through a combination of three quarks with different colors, such as red, green, and blue, or through a quark and an antiquark with matching colors and anticolors. This requirement ensures that quarks can never be observed in isolation, as the strong force becomes stronger as they are pulled apart, preventing any single quark from escaping the hadron. The result is a universe where all free particles are colorless, and the vibrant colors of quarks remain hidden within the confines of the hadron.

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HadronsNuclear physics

Common questions

What is a hadron and what is it made of?

A hadron is a composite subatomic particle formed by quarks and gluons. It is composed of two up quarks and one down quark for protons, or other combinations of quarks and antiquarks.

When was the term hadron first introduced in science?

The term hadron was introduced on the 2nd of May 1962 by Soviet physicist L. B. Okun. He presented the term during a plenary talk at the International Conference on High Energy Physics at CERN.

How are hadrons categorized into different families?

Hadrons are categorized into two broad families called baryons and mesons based on the number of quarks they contain. Baryons consist of three quarks while mesons consist of a quark and an antiquark pair.

Why are most hadrons unstable and what is the exception?

Most free hadrons are unstable and decay within fractions of a second due to the strong force. The proton is the only known exception that appears to be stable for at least 10 to the power of 34 years.

What happens to hadrons at very high temperatures and pressures?

At very high temperatures and pressures, hadrons disappear as quarks and gluons break free from confinement. This state is known as quark-gluon plasma and occurs in the energy range between 1 gigaelectronvolt and 1 teraelectronvolt.

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The Baryon and Meson Divide

Hadrons are categorized into two broad families based on the number of quarks they contain, creating a fundamental division between baryons and mesons. Baryons are composed of an odd number of valence quarks, typically three, and include the proton and neutron, which form the nuclei of atoms. Because they contain an odd number of quarks, baryons are fermions, meaning they have half-integer spin and obey the Pauli exclusion principle. Mesons, on the other hand, contain an even number of valence quarks, usually a quark and an antiquark pair, and are classified as bosons with integer spin. This distinction determines how these particles behave in the universe, with baryons making up the bulk of matter and mesons often acting as force carriers or short-lived intermediaries. The discovery of exotic hadrons, such as the Z(4430) tetraquark state found in 2007 and the pentaquark states confirmed in 2015, has challenged the traditional boundaries between these two families, suggesting that nature may allow for more complex combinations than previously thought.

The Race for Stability

Almost all free hadrons are unstable and decay into other particles within fractions of a second, with the exception of the proton, which appears to be stable for at least 10 to the power of 34 years. Free neutrons, the other common baryon, have a half-life of about 611 seconds and a mean lifetime of 879 seconds before decaying into a proton, an electron, and an antineutrino. This instability is a defining characteristic of hadron physics, as the strong force that binds quarks together also drives the rapid decay of most hadronic resonances. These resonances, which are excited states of hadrons, decay within about 10 to the power of minus 23 seconds, making them some of the shortest-lived particles in existence. The only known exception to this rule is the free proton, which may be the only stable hadron in the universe, ensuring that the matter we see today can persist over cosmic timescales.

Collisions and Cosmic Showers

Hadron physics is studied by colliding hadrons with each other or with the nuclei of dense, heavy elements like lead or gold, creating particle showers that reveal the inner workings of the strong force. These collisions, performed in facilities such as the Large Hadron Collider, allow physicists to observe the debris of the interaction and reconstruct the properties of the original particles. A similar process occurs naturally in the upper atmosphere, where cosmic rays collide with rarefied gas particles to produce muons and mesons such as pions. These natural collisions provide a continuous stream of data that complements the controlled experiments conducted in laboratories. The study of hadrons through these collisions has led to the discovery of new particles and the confirmation of theoretical predictions, pushing the boundaries of our understanding of the fundamental forces that govern the universe.

The Phase of Asymptotic Freedom

At very high temperatures and pressures, hadrons may disappear as quarks and gluons break free from their confinement, entering a state known as quark-gluon plasma. This phenomenon, predicted by the theory of quantum chromodynamics, occurs because the strength of the strong interaction diminishes with energy, a property known as asymptotic freedom. Experimental confirmation of this behavior has been achieved in the energy range between 1 gigaelectronvolt and 1 teraelectronvolt, where quarks and gluons no longer remain bound within hadrons. In this phase, the distinction between individual hadrons vanishes, and the quarks and gluons move freely, creating a state of matter that may have existed in the early universe just moments after the Big Bang. The study of this phase provides insights into the conditions of the early universe and the fundamental nature of the strong force.