Quantum Anomalies in Dense Matter

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dc.creatorSon, D. T.
dc.creatorZhitnitsky, A. R.
dc.date2004-05-21
dc.date.accessioned2026-07-07T03:52:33Z
dc.date.available2026-07-07T03:52:33Z
dc.descriptionWe consider the effects of quantum anomalies involving the baryon current for high-density matter. In the effective Lagrangian, the anomaly terms describe the interaction of three light fields: the electromagnetic photons A_mu, neutral light Nambu-Goldstone bosons (pi, eta, eta'), and the superfluid phonon. The anomaly induced interactions lead to a number of interesting phenomena which may have phenomenological consequences observable in neutron stars.
dc.description4 pages
dc.identifierhttps://arxiv.org/abs/hep-ph/0405216
dc.identifierhttp://arxiv.org/abs/hep-ph/0405216
dc.identifierPhys.Rev. D70 (2004) 074018
dc.identifierdoi:10.1103/PhysRevD.70.074018
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/43507
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Theory
dc.titleQuantum Anomalies in Dense Matter
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