AbstractThe QCD axion with fa at an intermediate scale, 109 GeV∼1012 GeV, seems in conflict with the gravity spoil of global symmetries and may face the axionic domain wall problem. We point out that the string compactifications with an anomalous U(1) gauge symmetry, allowing desirable chiral matter spectra, circumvent these two problems simultaneously
International audienceInspired by recent studies of high-scale decay constant or flavorful QCD axion...
The mass of the axion and its decay rate are known to depend only on the scale of Peccei-Quinn symme...
The recent detection of the cosmic microwave background polarimeter experiment BICEP2 of tensor fluc...
The QCD axion with fafa at an intermediate scale, 109 GeV∼1012 GeV109 GeV∼1012 GeV, seems in conflic...
AbstractThe recent BICEP2 result shows that the Universe once has gone through the vacuum with the G...
The recent BICEP2 result shows that the Universe once has gone through the vacuum with the GUT scale...
AbstractThe recent BICEP2 result shows that the Universe once has gone through the vacuum with the G...
The QCD axion couplings of various invisible axion models are presented. In particular, the exact gl...
In string compactifications, frequently the anomalous U(1) gauge symmetry appears which belongs to E...
It is pointed out that there exist a few problems to be overcome toward an observable sub-meV QCD ax...
The QCD axion solving the strong CP problem may originate from antisymmetric tensor gauge fields in ...
The mass of the axion and its decay rate are known to depend only on the scale of Peccei-Quinn symme...
The mass of the axion and its decay rate are known to depend only on the scale of Peccei-Quinn symme...
The QCD axion solving the strong CP problem may originate from antisymmetric tensor gauge fields in ...
International audienceInspired by recent studies of high-scale decay constant or flavorful QCD axion...
International audienceInspired by recent studies of high-scale decay constant or flavorful QCD axion...
The mass of the axion and its decay rate are known to depend only on the scale of Peccei-Quinn symme...
The recent detection of the cosmic microwave background polarimeter experiment BICEP2 of tensor fluc...
The QCD axion with fafa at an intermediate scale, 109 GeV∼1012 GeV109 GeV∼1012 GeV, seems in conflic...
AbstractThe recent BICEP2 result shows that the Universe once has gone through the vacuum with the G...
The recent BICEP2 result shows that the Universe once has gone through the vacuum with the GUT scale...
AbstractThe recent BICEP2 result shows that the Universe once has gone through the vacuum with the G...
The QCD axion couplings of various invisible axion models are presented. In particular, the exact gl...
In string compactifications, frequently the anomalous U(1) gauge symmetry appears which belongs to E...
It is pointed out that there exist a few problems to be overcome toward an observable sub-meV QCD ax...
The QCD axion solving the strong CP problem may originate from antisymmetric tensor gauge fields in ...
The mass of the axion and its decay rate are known to depend only on the scale of Peccei-Quinn symme...
The mass of the axion and its decay rate are known to depend only on the scale of Peccei-Quinn symme...
The QCD axion solving the strong CP problem may originate from antisymmetric tensor gauge fields in ...
International audienceInspired by recent studies of high-scale decay constant or flavorful QCD axion...
International audienceInspired by recent studies of high-scale decay constant or flavorful QCD axion...
The mass of the axion and its decay rate are known to depend only on the scale of Peccei-Quinn symme...
The recent detection of the cosmic microwave background polarimeter experiment BICEP2 of tensor fluc...
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