  In the Randall-Sundrum model where the Standard Model fields are confined to
the TeV brane located at the orbifold point $\theta = \pi$ and the gravity
peaks at the Planck brane located at $\theta = 0$, the stabilized modulus
(radion) field is required to stabilize the size of the fifth spatial
dimension. It can be produced copiously inside the supernova core due to
nucleon-nucleon bremstrahlung, electron-positron and plasmon-plasmon
annihilations, which then subsequently decays to neutrino-antineutrino pair and
take away the energy released in SN1987A explosion. Assuming that the
supernovae cooling rate $\dot{\varepsilon} \le 7.288\times 10^{-27} \rm{GeV}$,
we find the lower bound on the radion vev $\vphi \sim 9.0$ TeV, 2.2 TeV and 0.9
TeV corresponding to the radion mass $m_\phi = 5$ GeV, 20 GeV and 50 GeV,
respectively.
