Skip to content
DraconiticResearch
Search Sources API
197,768 studies31 sourcesUpdated 31 min ago
PreprintCC BY 4.0arXiv

Tomimatsu--Sato δ=2 Solution in Kaluza--Klein Theory

Abstract

We construct the Kaluza-Klein electric dressing of the Tomimatsu-Sato δ=2 vacuum spacetime by uplifting to five dimensions, boosting along the compact direction and reducing to Einstein-Maxwell-dilaton theory with coupling a=√3. It carries a nontrivial dilaton, unlike the known Einstein-Maxwell charged and magnetized Tomimatsu-Sato solutions. At leading order it shares the mass-charge-dilaton relations and gyromagnetic ratio g=2−tanh2α of the boosted Kerr black hole; the seed first shows up in the quadrupole. Using Mayerson's non-vacuum Geroch-Hansen multipoles, we derive the exact law M2(α)=1/2(1+cosh2α)M2(0), so the δ=2 quadrupole excess ΔM2=−1/4p2m2M survives every boost. In the Kodama-Hikida picture the Weyl segment ρ=0, |z|<κ is a singular rod with degenerate Killing horizons at its endpoints. There the boost function equals coshα, so the near-horizon geometry is a constant rescaling of the seed's: the horizons stay degenerate and non-rotating, their areas and Komar angular momenta scale by coshα, and the electric potential is 1/2tanhα. The electric flux through any closed surface is sinhαcoshα times the enclosed seed Komar mass, so the horizons and the ring singularity are uncharged and the rod carries all the charge; the boost-invariant identity M−ΦeQ=m follows. The ergosurface stays at f=0; a new curvature-singular boundary appears at f=coth2α, where the Kaluza-Klein circle becomes null. As the seed potential f is unbounded above near the ring, it exists for every nonzero boost: unlike for Kerr, no Kaluza-Klein boost of TS2 is a spacelike reduction everywhere. The excised region is compact, has the ring on its boundary and never reaches the horizons. Charging pointwise strengthens the causality violation near the rod.

Related

  1. Multi-rotating black holes with non-aligned angular momenta in 5D Kaluza-Klein theory
    Shinya Tomizawa, Hideo Furugori, Jun-ichi Sakamoto +1
    arXivPreprintCC BY 4.0Full textGravitation & general relativityHigh-energy & particle physicsarXiv
  2. Hamiltonian formulation of Carrollian Maxwell theory in Deformed Light-cone Kaluza-Klein-like Null reduction
    Limin Zeng
    arXivPreprintarXiv licenceFull textHigh-energy & particle physicsarXiv
  3. Near Threshold Kaluza-Klein Graviton Decays and the Dark Dimension
    Kevin Langhoff
    arXivPreprintCC BY 4.0Full textHigh-energy & particle physicsarXiv
  4. Evidence for Kaluza-Klein excitations of the graviton, gluon and quark at LHC
    Alain Le Yaouanc, François Richard
    arXivPreprintCC BY 4.0Full textHigh-energy & particle physicsarXivHAL
  5. Gauge-invariant thermodynamic description of rotating black strings in 5D minimal supergravity via Kaluza-Klein reduction
    Yang Yu, Peng-Ju Hu
    arXivPreprintCC BY-NC-ND 4.0Full textGravitation & general relativityHigh-energy & particle physicsarXiv
BibTeX
@misc{siahaan2026tomimatsusato,
  title = {{Tomimatsu--Sato $δ=2$ Solution in Kaluza--Klein Theory}},
  author = {Haryanto M. Siahaan and Masoud Ghezelbash},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.29277},
  eprint = {2610.29277},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.29277},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Tomimatsu--Sato δ=2 Solution in Kaluza--Klein Theory
AU  - Haryanto M. Siahaan
AU  - Masoud Ghezelbash
PY  - 2026
DA  - 2026/10/21
PB  - arXiv
DO  - 10.48550/arxiv.2610.29277
UR  - https://arxiv.org/abs/2610.29277
AB  - We construct the Kaluza-Klein electric dressing of the Tomimatsu-Sato δ=2 vacuum spacetime by uplifting to five dimensions, boosting along the compact direction and reducing to Einstein-Maxwell-dilaton theory with coupling a=√3. It carries a nontrivial dilaton, unlike the known Einstein-Maxwell charged and magnetized Tomimatsu-Sato solutions. At leading order it shares the mass-charge-dilaton relations and gyromagnetic ratio g=2−tanh^2α of the boosted Kerr black hole; the seed first shows up in the quadrupole. Using Mayerson's non-vacuum Geroch-Hansen multipoles, we derive the exact law M_2(α)=1/2(1+cosh^2α)M_2^(0), so the δ=2 quadrupole excess ΔM_2=−1/4p^2m^2M survives every boost. In the Kodama-Hikida picture the Weyl segment ρ=0, |z|<κ is a singular rod with degenerate Killing horizons at its endpoints. There the boost function equals coshα, so the near-horizon geometry is a constant rescaling of the seed's: the horizons stay degenerate and non-rotating, their areas and Komar angular momenta scale by coshα, and the electric potential is 1/2tanhα. The electric flux through any closed surface is sinhαcoshα times the enclosed seed Komar mass, so the horizons and the ring singularity are uncharged and the rod carries all the charge; the boost-invariant identity M−Φ_eQ=m follows. The ergosurface stays at f=0; a new curvature-singular boundary appears at f=coth^2α, where the Kaluza-Klein circle becomes null. As the seed potential f is unbounded above near the ring, it exists for every nonzero boost: unlike for Kerr, no Kaluza-Klein boost of TS_2 is a spacelike reduction everywhere. The excised region is compact, has the ring on its boundary and never reaches the horizons. Charging pointwise strengthens the causality violation near the rod.
ER  -