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BiBTeX citation export for MOPAB033: Monochromatization of e⁺e⁻ Colliders with a Large Crossing Angle

@inproceedings{telnov:ipac2021-mopab033,
  author       = {V.I. Telnov},
  title        = {{Monochromatization of e⁺e⁻ Colliders with a Large Crossing Angle}},
  booktitle    = {Proc. IPAC'21},
  pages        = {152--154},
  eid          = {MOPAB033},
  language     = {english},
  keywords     = {emittance, resonance, collider, luminosity, radiation},
  venue        = {Campinas, SP, Brazil},
  series       = {International Particle Accelerator Conference},
  number       = {12},
  publisher    = {JACoW Publishing, Geneva, Switzerland},
  month        = {08},
  year         = {2021},
  issn         = {2673-5490},
  isbn         = {978-3-95450-214-1},
  doi          = {10.18429/JACoW-IPAC2021-MOPAB033},
  url          = {https://jacow.org/ipac2021/papers/mopab033.pdf},
  note         = {https://doi.org/10.18429/JACoW-IPAC2021-MOPAB033},
  abstract     = {{The relative center-of-mass energy spread at e⁺e⁻ colliders is much larger than the widths of narrow resonances, which greatly lowers the resonance production rates of J/Psi, Psi-prime, Upsililon(nS), n=1-3. Thus, a significant reduction of the center-of-mass energy spread would open up great opportunities in the search for new physics in rare decays of narrow resonances, the search for new narrow states with small partial e⁺e⁻ width. The existing monochromatization scheme is only suitable for head-on collisions, while e⁺e⁻ colliders with crossing angles (the so-called Crab Waist collision scheme) can provide much higher luminosity. In this report, a new monochromatization method for colliders with a large crossing angle is discussed*. The contribution of the beam energy spread to the spread of the center-of-mass energy is canceled by introducing an appropriate energy-angle correlation at the interaction point; the relative RMS mass spread of about (3-5)10⁻⁶ seems possible. Limitations of the proposed method are also considered. This monochromatization scheme is very attractive for the Upsilon-meson region and below.}},
}