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It's generally believed that young and rapidly rotating pulsars are importantsites of particle's acceleration, in which protons can be accelerated torelativistic energy above the polar cap region if the magnetic moment isantiparallel to the spin axis($\vec{\mu}\cdot\vec{\Omega}<0$). To obtain thegalactic diffusive neutrinos and gamma-rays for TeV, firstly,we use MonteCarlo(MC) method to generate a sample of young pulsars with ages less than$10^6$ yrs in our galaxy ; secondly, the neutrinos and high-energy gamma-rayscan be produced through photomeson process with the interaction of energeticprotons and soft X-ray photons ($p+\gamma\rightarrow \Delta^+\rightarrown+\pi^+/p+\pi^0$) for single pulsar, and these X-ray photons come from theneutron star surface. The results suggest that the diffusive TeV flux ofneutrinos are lower than background flux, which indicated it is difficult to bedetected by the current neutrino telescopes.

Diffuse emission of TeV Neutrinos and Gamma-rays from young pulsars by Photo-meson interaction in the galaxy