ar X iv : 0 80 5 . 19 70 v 1 [ he p - ph ] 1 4 M ay 2 00 8 Macro - coherent two photon and radiative neutrino pair emission

ar X iv : 0 80 5 . 19 86 v 1 [ qu an t - ph ] 1 4 M ay 2 00 8 Cooper Pair Boxes Weakly Coupled to External Environments

We study the behaviour of charge oscillations in Superconducting Cooper Pair Boxes weakly interacting with an environment. We found that, due to the noise and dissipation induced by the environment, the stability properties of these nanodevices differ according to whether the charge oscillations are interpreted as an effect of macroscopic quantum coherence, or semiclassically in terms of the Gr...

ar X iv : 0 70 8 . 33 71 v 1 [ he p - ph ] 2 4 A ug

Dark matter is usually distinguished from ordinary matter by an odd-even parity, i.e. the discrete symmetry Z 2. The new idea of Z 3 dark matter is proposed with a special application to generating radiative Majorana neutrino masses in two-loop order.

ar X iv : 0 90 5 . 29 23 v 1 [ he p - ph ] 1 8 M ay 2 00 9 Adler sum rule

The Adler sum rule states that the integral over energy of a difference of neutrino-nucleon and antineutrino-nucleon structure functions is a constant, independent of the four-momentum transfer squared. This constancy is a consequence of the local commutation relations of the time components of the hadronic weak current, which follow from the underlying quark structure of the standard model.

ar X iv : 0 90 1 . 10 80 v 1 [ he p - ph ] 8 J an 2 00 9 Tri - Bimaximal lepton mixing with A 4 ⋉ ( Z 2 )

We consider a model based on A4 ⋉ (Ze ×Zμ ×Zτ ) flavor symmetry for TriBimaximal lepton mixing with two scalar A4-triplets whose vacuum expectation values have the same alignment. Neutrino masses are generated through effective dimension five Weinberg operators. Charged leptons mass hierarchies are generated with an additional Froggatt-Nielsen U(1)F flavor symmetry under which right-handed lept...

ar X iv : 0 70 5 . 31 41 v 1 [ as tr o - ph ] 2 2 M ay 2 00 7 The SARG Planet Search