A proton is a stable subatomic particle, symbol , H+, or 1H+ with a positive electric charge of +1 e (elementary charge). Its mass is slightly less than the mass of a neutron and approximately times the mass of an electron (the proton-to-electron mass ratio). Protons and neutrons, each with a mass of approximately one dalton, are jointly referred to as nucleons (particles present in atomic nuclei).
One or more protons are present in the nucleus of every atom. They provide the attractive electrostatic central force which binds the atomic electrons. The number of protons in the nucleus is the defining property of an element, and is referred to as the atomic number (represented by the symbol Z). Since each element is identified by the number of protons in its nucleus, each element has its own atomic number, which determines the number of atomic electrons and consequently the identity and chemical characteristics of the element.
The word proton is Greek for "first", and the name was given to the hydrogen nucleus by Ernest Rutherford in 1920. In previous years, Rutherford had discovered that the hydrogen nucleus (known to be the lightest nucleus) could be extracted from the nuclei of nitrogen by atomic collisions. Protons were therefore a candidate to be a fundamental or elementary particle, and hence a building block of nitrogen and all other heavier atomic nuclei.
Although protons were originally considered to be elementary particles, in the modern Standard Model of particle physics, protons are known to be composite particles, containing three valence quarks, and together with neutrons are now classified as hadrons. Protons are composed of two up quarks of charge +e each, and one down quark of charge −e. The rest masses of quarks contribute only about 1% of a proton's mass. The remainder of a proton's mass is due to quantum chromodynamics binding energy, which includes the kinetic energy of the quarks and the energy of the gluon fields that bind the quarks together. The proton charge radius is around but two different kinds of measurements give slightly different values.N Baryons
At sufficiently low temperatures and kinetic energies, free protons will bind electrons in any matter they traverse.
Free protons are routinely used for accelerators for proton therapy or various particle physics experiments, with the most powerful example being the Large Hadron Collider.
Description
Protons are spin- fermions and are composed of three valence quarks, making them baryons (a sub-type of hadrons). The two up quarks and one down quark of a proton are held together by the strong force, mediated by gluons. A modern perspective has a proton composed of the valence quarks (up, up, down), the gluons, and transitory pairs of sea quarks. Protons have a positive charge distribution, which decays approximately exponentially, with a root mean square charge radius of about 0.8 fm.
Protons and neutrons are both nucleons, which may be bound together by the nuclear force to form atomic nuclei. The nucleus of the most common isotope of the hydrogen atom (with the chemical symbol "H") is a lone proton. The nuclei of the heavy hydrogen isotopes deuterium and tritium contain one proton bound to one and two neutrons, respectively. All other types of atomic nuclei are composed of two or more protons and various numbers of neutrons.
History The concept of a hydrogen-like particle as a constituent of other atoms was developed over a long period. As early as 1815, William Prout used early values of atomic weight to devise what later researchers called Prout's hypothesis: all atoms are composed of integer combinations of hydrogen atoms (which he called "protyles"). When more accurate values of the atomic weights were measured, the integer relationship failed. Nevertheless the concept continued to intrigue scientists and would eventually emerge again a century later.
In 1886, Eugen Goldstein discovered canal rays (also known as anode rays) exiting from perforations in the discharge tube. Wilhelm Wien in 1898 showed that these rays had a charge opposite to the negative electrons discovered by J. J. Thomson, but with a much higher mass to charge ratio. Later that year Thomson was able to determine a value for the magnitude of the electric charge, e, and show that the canal rays included material with charge-to-mass ratio (q/m) consistent with the hydrogen ion.
Following the discovery of the atomic nucleus by Ernest Rutherford in 1913, Antonius van den Broek proposed that the place of each element in the periodic table (its atomic number) is equal to its nuclear charge. Van den Broek speculated that the nucleus contained alpha particles with four positive charges and two electrons, the first version of the nuclear-electron hypothesis. (The modern model of two positive protons and two neutrons would take many years to discover). Also in 1913 Niels Bohr presented a theory of atomic structure which predicted electronic transitions related to nuclear charge. This was confirmed experimentally by Henry Moseley in 1913 when he showed that the energy of X-ray spectra lines of many elements followed a pattern based on atomic number.
In 1919, after a long series of sporadic experiments interrupted by WWI, Rutherford discovered what he called artificial disintegration of nitrogen atoms. Using alpha particles from radium to strike air, Rutherford detected scintillation on a zinc sulfide screen at a distance, up to 28 cm, well beyond the distance of alpha-particle range of travel but instead corresponding to the range of travel of hydrogen atoms. By 1920 he concluded that these hydrogen nuclei were a constituent part of the nitrogen nucleus. This result has been described as the discovery of protons.
When Rutherford described his results at the British Association for the Advancement of Science August 1920 he was asked by Oliver Lodge for a new name for the positive hydrogen nucleus to avoid confusion with the neutral hydrogen atom. Rutherford initially suggested both proton (the neuter singular of the Greek word for "first", ) and prouton (after Prout). Rutherford later reported that the meeting had accepted his suggestion that the hydrogen nucleus be named the "proton", following Prout's word "protyle". The first use of the word "proton" in the scientific literature appeared in 1920.OED
Rutherford initially assumed that the alpha particle merely knocked a proton out of nitrogen, turning it into carbon. Patrick Blackett's cloud chamber images in 1925 demonstrated that the alpha particle was absorbed. If the alpha particle were not absorbed, then three charged particles, a negatively charged carbon, a proton, and an alpha particle, would be expected. The three charged particles would create three tracks in the cloud chamber, but only two tracks in the cloud chamber were observed. Blackett proposed that the alpha particle is absorbed by the nitrogen atom. Heavy oxygen (17O), not carbon, was the product. This was the first reported nuclear reaction, .
Occurrence One or more bound protons are present in the nucleus of every atom. Free protons are found naturally in a number of situations in which energies or temperatures are high enough to separate them from electrons, for which they have some affinity. Free protons occur occasionally on Earth: thunderstorms can produce protons with energies of up to several tens of megaelectronvolt. Free protons exist in plasmas in which temperatures are too high to allow them to combine with electrons. Free protons of high energy and velocity make up 90% of cosmic rays, which propagate through the interstellar medium. Free protons are emitted directly from atomic nuclei in some rare types of radioactive decay. Protons also result (along with electrons and antineutrinos) from the radioactive decay of free neutrons, which are unstable.
Stability
The spontaneous decay of free protons has never been observed, and protons are therefore considered stable particles according to the Standard Model. However, some grand unified theories (GUTs) of particle physics predict that proton decay should take place with lifetimes between 1031 and 1036 years. The experimental lower bound for the mean lifetime is .S. Navas et al. (Particle Data Group), Phys. Rev. D 110, 030001 (2024) and 2025 update. p
The mean lifetime measures decay to any product. Lifetimes for decay to specific products is also measured. For example, experiments at the Super-Kamiokande detector in Japan gave lower limits for proton mean lifetime of for decay to an antimuon and a neutral pion, and for decay to a positron and a neutral pion.
Protons are known to transform into neutrons through the process of electron capture (also called inverse beta decay). For free protons, this process does not occur spontaneously but only when energy is supplied. The equation is: + → +
The process is reversible; neutrons can convert back to protons through beta decay, a common form of radioactive decay. In fact, a free neutron decays this way, with a mean lifetime of about 15 minutes. A proton can also transform into a neutron through beta plus decay (β+ decay).
According to quantum field theory, the mean proper lifetime of protons becomes finite when they are accelerating with proper acceleration , and decreases with increasing . Acceleration gives rise to a non-vanishing probability for the transition . This was a matter of concern in the later 1990s because is a scalar that can be measured by the inertial and coaccelerated observers. In the inertial frame, the accelerating proton should decay according to the formula above. However, according to the coaccelerated observer the proton is at rest and hence should not decay. This puzzle is solved by realizing that in the coaccelerated frame there is a thermal bath due to Fulling–Davies–Unruh effect, an intrinsic effect of quantum field theory. In this thermal bath, experienced by the proton, there are electrons and antineutrinos with which the proton may interact according to the processes: , and . Adding the contributions of each of these processes, one should obtain .
Mass Electron ratio
The proton-electron mass ratio is a fundamental dimensionless physical constant μ = Astrophysical measurements show this value has been constant as far back as 10 billions years ago.
Quauntum chromodynamics In quantum chromodynamics, the modern theory of the nuclear force, most of the mass of protons and neutrons is explained by special relativity. The mass of a proton is about 80–100 times greater than the sum of the rest masses of its three valence quarks, while the gluons have zero rest mass. The extra energy of the quarks and gluons in a proton, as compared to the rest energy of the quarks alone in the QCD vacuum, accounts for almost 99% of the proton's mass. The rest mass of a proton is, thus, the invariant mass of the system of moving quarks and gluons that make up the particle, and, in such systems, even the energy of massless particles confined to a system is still measured as part of the rest mass of the system.
Two terms are used in referring to the mass of the quarks that make up protons: current quark mass refers to the mass of a quark by itself, while constituent quark mass refers to the current quark mass plus the mass of the gluon particle field surrounding the quark. These masses typically have very different values. The kinetic energy of the quarks that is a consequence of confinement is a contribution (see Mass in special relativity). Using lattice QCD calculations, the contributions to the mass of the proton are the quark condensate (~9%, comprising the up and down quarks and a sea of virtual strange quarks), the quark kinetic energy (~32%), the gluon kinetic energy (~37%), and the anomalous gluonic contribution (~23%, comprising contributions from condensates of all quark flavors).
The constituent quark model wavefunction for the proton is