We report on our recent attempts to determine the short distance behaviors of general 2-baryon and 3-baryon forces, which are defined from the Nambu-Bethe-Salpeter(NBS) wave function, by using the operator product expansion and a renormalization group analysis in QCD. We have found that the repulsion at short distance increases as the number of valence quarks increases or when the number of different flavors involved decreases. This global tendency suggests a Pauli suppression principle among quark fields at work. §1. MotivationThe most fundamental quantity in nuclear physics is a force between nucleons, the nuclear force, from which major properties of nuclei are extracted. The phenomenological nuclear potentials, 1) which well describe nucleon-nucleon (NN) scattering at low energy, exhibit long-to-medium distance attractions, essential for the binding of atomic nuclei, as well as short distance repulsion (a repulsive core), important for the stability of nuclei against collapse. While the former properties have been explained by meson exchanges between nucleons, 2) the origin of the repulsive core 3) has not yet been well understood. Considerations of the fundamental degrees of freedom for nucleons, quarks and gluons, and their dynamics, QCD, are required to explain the properties between nucleons at such short distances.The recent observation of a neutron star as heavy as twice a solar mass 4) forces us to consider more general short distance repulsions among baryons, not only NN but also 3N, BB and 3B, where B represents an octet baryon which may include one or more strange quarks. This is because although the repulsive core of NN potentials is an important ingredient for the determination of the maximum mass of neutron stars, it alone seems insufficient to sustain the two-solar-mass neutron star. Moreover, an appearance of heavier strange quarks, converted from lighter up and down quarks via the weak interaction in such a high density environment, makes the equation of state softer in the core of the neutron star, so that the maximum mass of the neutron star is further reduced. It has already been pointed out that general BB potentials alone can not sustain the two-solar-mass neutron star. 5) It is also argued that the maximum mass of neutron stars can be increased if 3-body forces, typeset using PTPT E X.cls Ver.0.9