Skip to content
DraconiticResearch
Search Sources API
203,234 studies31 sourcesUpdated 36 min ago
PreprintCC BY 4.0arXiv

Magnetic field effect on neutral color superconductivity as a mechanism to boost the inner magnetic field of magnetars

Abstract

In this paper, we review the impact of a strong magnetic field on the neutral two-flavor color superconducting (2SC) phase of dense quark matter. Using a Nambu-Jona-Lasinio (NJL) model approach in the mean-field approximation, we first solve the gap equations for the diquark condensate Δ and the electric chemical potential μe under a uniform external magnetic field, and discuss the coupled evolution of the chiral and diquark order parameters. We then evaluate the field-dependent Meissner masses of the rotationally charged gluons for a wide range of densities and moderate diquark coupling strengths. Combining the "zero-mode problem" mechanism with the neutrality condition, we show that the gluon masses become tachyonic even at moderate magnetic-field values, signaling a chromomagnetic instability in density regions where the system was stable at zero field. This instability can be resolved through the restructuring of the ground state with the formation of a gluon vortex condensate. A remarkable consequence of the vortex configuration is the paramagnetic amplification of the in-medium magnetic field: seed fields of the order of 1015 G can be enhanced by up to two orders of magnitude, reaching ∼ 1017 G, precisely the range predicted for magnetar cores. We compare this microscopic mechanism with the conventional dynamo explanation and discuss how it offers a plausible explanation for the extremely high magnetic fields expected to be realized in magnetar interiors.

Versions

Related

  1. Non-axisymmetric Transport of Magnetic Flux Tubes: A Mechanism for Joy's Law and Poloidal Field Generation via Meridional Flows
    Andrey G. Tlatov
    arXivPreprintCC BY 4.0Full textSolar & stellar physicsarXiv
  2. Interior Magnetic Fields in Magnetars and Radio Pulsars
    Raj Kishor Joshi, Brynmor Haskell, William Cook +1
    arXivPreprintarXiv licenceFull textHigh-energy astrophysicsarXiv
  3. Angular structure of finite-field vacuum birefringence in magnetars
    Shahram Abbassi, S. R. Valluri
    arXivPreprintarXiv licenceFull textHigh-energy astrophysicsarXiv
  4. Magnetic-field constraints for four magnetic cataclysmic variables from simultaneous continuum and cyclotron modeling
    Jiamao Lin, Wenyuan Guo, Yongkang Sun +2
    Astronomy & AstrophysicsPeer-reviewedPublisher termsSolar & stellar physicsCrossref
  5. Isochrones in primordial magnetic field evolution
    A. Brandenburg, M. Cielo, O. Iarygina +1
    Astronomy & AstrophysicsPeer-reviewedPublisher termsCosmologyCrossref
BibTeX
@misc{feng2026magnetic,
  title = {{Magnetic field effect on neutral color superconductivity as a mechanism to boost the inner magnetic field of magnetars}},
  author = {Bo Feng},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.32028},
  eprint = {2610.32028},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.32028},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Magnetic field effect on neutral color superconductivity as a mechanism to boost the inner magnetic field of magnetars
AU  - Bo Feng
PY  - 2026
DA  - 2026/10/23
PB  - arXiv
DO  - 10.48550/arxiv.2610.32028
UR  - https://arxiv.org/abs/2610.32028
AB  - In this paper, we review the impact of a strong magnetic field on the neutral two-flavor color superconducting (2SC) phase of dense quark matter. Using a Nambu-Jona-Lasinio (NJL) model approach in the mean-field approximation, we first solve the gap equations for the diquark condensate Δ and the electric chemical potential μ_e under a uniform external magnetic field, and discuss the coupled evolution of the chiral and diquark order parameters. We then evaluate the field-dependent Meissner masses of the rotationally charged gluons for a wide range of densities and moderate diquark coupling strengths. Combining the "zero-mode problem" mechanism with the neutrality condition, we show that the gluon masses become tachyonic even at moderate magnetic-field values, signaling a chromomagnetic instability in density regions where the system was stable at zero field. This instability can be resolved through the restructuring of the ground state with the formation of a gluon vortex condensate. A remarkable consequence of the vortex configuration is the paramagnetic amplification of the in-medium magnetic field: seed fields of the order of 10^15 G can be enhanced by up to two orders of magnitude, reaching ∼ 10^17 G, precisely the range predicted for magnetar cores. We compare this microscopic mechanism with the conventional dynamo explanation and discuss how it offers a plausible explanation for the extremely high magnetic fields expected to be realized in magnetar interiors.
ER  -