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@ARTICLE{Eto:490675,
      author       = {Eto, Minoru and Hamada, Yu and Jinno, Ryusuke and Nitta,
                      Muneto and Yamada, Masatoshi},
      title        = {{A}brikosov-{N}ielsen-{O}lesen strings from the
                      {C}oleman-{W}einberg potential},
      journal      = {Physical review / D},
      volume       = {106},
      number       = {11},
      issn         = {2470-0010},
      address      = {Melville, NY},
      publisher    = {Inst.},
      reportid     = {PUBDB-2022-07910, arXiv:2205.04394. YGHP-22-01.
                      KEK-TH-2418. IFT-UAM/CSIC-22-48. DESY-22-071},
      pages        = {116002},
      year         = {2022},
      note         = {ISSN 2470-0029 not unique: **2 hits**.40 pages, 19 figs;
                      v2: minor revision},
      abstract     = {We study properties of Abrikosov-Nielsen-Olesen (ANO)
                      strings with the Coleman-Weinberg (CW) potential, which we
                      call CW-ANO strings. While the scale-invariant scalar
                      potential has a topologically trivial vacuum admitting no
                      strings at the classical level, quantum correction allows
                      topologically nontrivial vacua and stable string solutions.
                      We find that the system of the CW potential exhibits
                      significant difference from that of the conventional
                      Abelian-Higgs model with the quadratic-quartic potential.
                      While a single-winding string is qualitatively similar in
                      both systems, and the static intervortex force between two
                      strings at large distance is attractive/repulsive in the
                      type-I/II regime for both, that between two CW-ANO strings
                      exhibits a nontrivial structure. It develops an energy
                      barrier between them at intermediate distance, implying that
                      the string with winding number $n > 1$ can constitute a
                      metastable bound state even in the type-II regime. We name
                      such a superconductor type-$\overline{1.5}$. We also discuss
                      implications to high-energy physics and cosmology.},
      keywords     = {correction: quantum (INSPIRE) / potential: scalar (INSPIRE)
                      / string (INSPIRE) / superconductivity (INSPIRE) / stability
                      (INSPIRE) / vacuum state (INSPIRE) / bound state (INSPIRE) /
                      structure (INSPIRE) / cosmological model (INSPIRE)},
      cin          = {T},
      ddc          = {530},
      cid          = {I:(DE-H253)T-20120731},
      pnm          = {611 - Fundamental Particles and Forces (POF4-611) / DFG
                      project G:(GEPRIS)390833306 - EXC 2121: Quantum Universe
                      (390833306) / DFG project G:(GEPRIS)390900948 - EXC 2181:
                      STRUKTUREN: Emergenz in Natur, Mathematik und komplexen
                      Daten (390900948)},
      pid          = {G:(DE-HGF)POF4-611 / G:(GEPRIS)390833306 /
                      G:(GEPRIS)390900948},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2205.04394},
      howpublished = {arXiv:2205.04394},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2205.04394;\%\%$},
      UT           = {WOS:000893201800002},
      doi          = {10.1103/PhysRevD.106.116002},
      url          = {https://bib-pubdb1.desy.de/record/490675},
}