Q-balls

E24266

Q-balls are hypothetical, stable, non-topological solitons predicted in certain quantum field theories, often considered as exotic candidates for dark matter or new physics beyond the Standard Model.

AI illustration

How this image was made

AI-generated illustration of Q-balls

This AI-generated illustration was produced by black-forest-labs/FLUX.2-dev (1024x1024) from a prompt written by openai/gpt-oss-120b from the entity's label + description.

Prompt

Generate an image of a q-balls (Q-balls are hypothetical, stable, non-topological solitons predicted in certain quantum field theories, often considered as exotic candidates for dark matter or new physics beyond the Standard Model.)

All labels observed (1)

Label Occurrences
Q-balls canonical 2

How this entity was disambiguated

Statements (49)

Predicate Object
instanceOf dark matter candidate ⓘ
hypothetical particle-like object ⓘ
non-topological soliton ⓘ
theoretical construct in quantum field theory ⓘ
canBeProducedIn early Universe phase transitions ⓘ
fragmentation of scalar condensates ⓘ
non-equilibrium dynamics after inflation ⓘ
canDecayInto fermions carrying same global charge ⓘ
standard model particles in unstable scenarios ⓘ
consideredAs candidate for new physics beyond the Standard Model ⓘ
exotic dark matter candidate ⓘ
hasProperty arise from attractive self-interactions of scalar fields ⓘ
can be absolutely stable in some models ⓘ
can be energetically favored over free quanta ⓘ
can be long-lived ⓘ
can be macroscopically large ⓘ
can be metastable in some models ⓘ
can have large quantum number Q ⓘ
can have thick-wall regime ⓘ
can have thin-wall regime ⓘ
carry scalar field charge ⓘ
classically stable ⓘ
conserved global charge ⓘ
localized field configuration ⓘ
minimize energy at fixed global charge ⓘ
non-topological ⓘ
time-dependent phase ⓘ
mathematicalDescription nonlinear solutions of scalar field equations with global symmetry ⓘ
mayContributeTo baryon asymmetry of the Universe in some models ⓘ
cosmological dark matter density ⓘ
predictedIn Affleck–Dine baryogenesis scenarios ⓘ
certain relativistic quantum field theories ⓘ
supersymmetric extensions of the Standard Model ⓘ
theories with complex scalar fields ⓘ
theories with global U(1) symmetry ⓘ
relatedTo Affleck–Dine condensate fragmentation ⓘ
baryogenesis ⓘ
baryon number carrying objects in some models ⓘ
dark matter phenomenology ⓘ
early Universe cosmology ⓘ
global charge conservation ⓘ
lepton number carrying objects in some models ⓘ
non-topological soliton solutions of scalar field equations ⓘ
searchesVia astrophysical constraints ⓘ
direct detection experiments for exotic massive particles ⓘ
indirect detection through decay products ⓘ
stabilityCondition energy per unit charge less than mass of corresponding free particle ⓘ
existence of suitable scalar potential with attractive self-interactions ⓘ
theoreticalOrigin minimization of energy functional at fixed conserved charge ⓘ

How these facts were elicited

Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.