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*[[List of baryons#Baryon resonance particles|Baryon resonance particles]] ...

...tle=Note on Unitary Symmetry in Strong Interactions. II —Excited States of Baryons— ==Baryons== ...

* [[List of baryons]] [[Category:Baryons]] ...

...]] problem, which is non-baryonic in nature.<ref>See [[Lambda-CDM model]]. Baryons make up only ~5% of the universe, while dark matter makes up 26.8%.</ref> ...mical elements]] in observations of the recent universe. Higher numbers of baryons in the early universe should produce higher ratios for helium, lithium, and ...

...Bethe–Salpeter equation|Bethe-Salpeter equation]]. While the amplitude for baryons is solved from the [[Faddeev equations|Faddeev equation]]. Information on t ...

...yons for 3 quark flavors u,d,s: Tuning to harmonic numbers of oscimodes of baryons |journal=EPJ Web of Conferences |date=2014 |volume=71 |pages=00090 |doi=10. ...

...ite journal|last1=Barkana|first1=Rennan|title=Possible interaction between baryons and dark-matter particles revealed by the first stars|journal=Nature|date=1 ...

...=B.|last11=Di Bari|first11=D.|year=1995|title=Results on the production of baryons with {{!}}S{{!}} = 1, 2, 3 and strange mesons in S-W collisions at 200 GeV/ ...

...nsisted of a hot, dense [[Plasma (physics)|plasma]] of [[electrons]] and [[baryons]] (which include protons and neutrons). [[Photons]] (light particles) trave ...]] and [[photons]]. The pressure results in spherical sound waves of both baryons and photons moving with a speed slightly over half the [[speed of light]]<r ...

..., initially with a cosmic matter budget around 95% cold dark matter and 5% baryons. However, in the 1990s various observations including galaxy clustering and ...

|title=A Schematic Model of Baryons and Mesons ...

...he dissipation of acoustic waves set up by inflation. In this process, the baryons heat up and transfer some of their excess energy to the ambient CMB photon ...ng]]), photons and baryons<ref> In the language of cosmologists, the term "baryons" includes the electrons even if the latter are leptons in particle physics ...

...were ''[[adiabatically]]'' damped. That is to say the ratios of photons to baryons remained constant during the damping process.<ref name=hu1213 /><ref name=m ...ber density (<math>\mathit{n}_\mathit{b}</math>). That means that the more baryons there were, and the more they were ionised, the shorter the average photon ...

...1|u=seconds}}).<ref name=Beringer-etal-2012-PDG-010001/><ref name=PDG-2007-baryons-LPL/> |title=Summary of baryons ...

...iverse that produced baryonic asymmetry, i.e. the imbalance of [[matter]] (baryons) and [[antimatter]] (antibaryons) in the observed universe. However, baryog ...

...|s2cid=261693972 }}</ref> In the early universe the chemical potential of baryons is assumed to be near zero and the transition near 170MeV converts a quark- ...

**[[Exotic baryon|Exotic baryons]] ...

|title=Electromagnetic properties of baryons in the supermultiplet scheme of elementary particles ...ccurate estimates for the magnetic moments of neutrons, protons, and other baryons.<ref name=Perk/> For a neutron, the magnetic moment is given by {{nobr|{{ma ...

...quarks and gluons. At low energies, however, proper degrees of freedom are baryons and mesons. Another example is the BEC/BCS crossover problem in [[condensed ...