Virtual Meson Cloud of the Nucleon and Intrinsic Strangeness and Charm
نویسندگان
چکیده
We have applied the Meson Cloud Model (MCM) to calculate the charm and strange antiquark distribution in the nucleon. The resulting distribution, in the case of charm, is very similar to the intrinsic charm momentum distribution in the nucleon. This seems to corroborate the hypothesis that the intrinsic charm is in the cloud and, at the same time, explains why other calculations with the MCM involving strange quark distributions fail in reproducing the low x region data. From the intrinsic strange distribution in the nucleon we have extracted the strangeness radius of the nucleon, which is in agreement with other meson cloud calculations. PACS numbers 14.20.Dh 12.40.-y 14.65.-q Many years ago, it has been suggested by Sullivan [1] that some fraction of the nucleon's anti-quark sea distribution may be associated with non-perturbative processes like the pion e-mail: [email protected] e-mail: [email protected] e-mail: [email protected] e-mail: [email protected] e-mail: [email protected]
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