  The Cygnus region, which contains massive molecular and atomic clouds and
young stars, is a promising Galactic neutrino source candidate. Cosmic rays
transport in the region can produce neutrinos and $\gamma$-rays. Recently, the
Large High Altitude Air Shower Observatory (LHAASO) detected an
ultrahigh-energy $\gamma$-ray bubble (Cygnus Bubble) in this region. Using
publicly available track events detected by the IceCube Neutrino Observatory in
7 years of full detector operation, we conduct searches for correlated neutrino
signals from the Cygnus Bubble with neutrino emission templates based on LHAASO
$\gamma$-ray observations. No significant signals were found for any employed
templates. With the 7 TeV $\gamma$-ray flux template, we set a flux upper limit
of 90% confidence level (C.L.) for the neutrino emission from the Cygnus Bubble
to be $5.7\times10^{-13}\, \mathrm{TeV}^{-1}\mathrm{cm}^{-2}\mathrm{s}^{-1}$ at
5 TeV.
