A pair-breaking mechanism of a superconductor under magnetic fields, namely, the origin of the upper critical field H c2 , can be categorized into the orbital effect and the paramagnetic effect, which have been separately discussed so far because the physical pictures are totally different. Here we propose a model that unifies these two origins into one formalism with a generalized physical picture. The obtained formula well describes the experimental results on the angle dependence of H c2 in a recently developed noncentrosymmetric superconductor, two-dimensional (2D) NbSe 2 , providing essential information on the spin states of Cooper pairs in 2D NbSe 2 . The proposed model is widely applicable to all superconductors, offering a powerful approach for comprehensive understanding of the origin of H c2 . Superconductivity is usually suppressed by application of external magnetic fields above the upper critical field H c2 . The origins of H c2 are classified into two pair-breaking effects, the orbital effect and the paramagnetic effect. In the limit of the strong orbital effect (the orbital limit), the kinetic energy loss due to the magnetic-field-driven cyclotron motion of electrons causes suppression of superconductivity by forming the vortices or Meissner current. In the paramagnetic limit, on the other hand, superconductivity is suppressed by the energy gain of the spin-aligned paramagnetic state, which exceeds the gain of the condensation energy of the Cooper pairs. Within the framework of the Bardeen-Cooper-Schrieffer (BCS) theory, this paramagnetic limit is called the Pauliparamagnetic limit and is set to be H P = 0