When axionic strings carry a global charge, domain walls bounded by such strings may not be allowed to decay completely. This happens in particular in some models where a composite axion-like particle is the pseudo-Nambu-Goldstone boson of chiral symmetry breaking of an extra quark flavor. In this case the global symmetry is the extra flavor baryonic symmetry. The corresponding axionic domain walls can carry a baryonic charge: they represent the low energy description of the baryons made by the extra quark flavor. Basic properties of these particles, such as spin, mass scale, size are discussed. The corresponding charged axionic strings are explicitly constructed and studied in a specific calculable model.Comment: 6 page
International audienceInspired by recent studies of high-scale decay constant or flavorful QCD axion...
We propose an extra-dimension framework on the orbifold $S^1/Z_2$ for understanding the origin of th...
The story of the Axion traces back to the so-called U(1) problem in QCD. In fact, QCD, restricted to...
We explore the effective theory of an axion in a gauged baryon number symmetry extension of the Stan...
The damping of the axionic string motion due to the surrounding plasma is estimated by a detailed ca...
I discretize axion string configuration coupled to a Dirac fermion, which in the continuum binds a m...
I review the dark energy solutions by a very light pseudoscalar called "quintessential axion". For t...
Axion-like particles (ALPs), a compelling candidate for dark matter (DM), are the pseudo Nambu-Golds...
We argue that demanding a consistent cosmological history, including the absence of domain walls and...
We propose a new scenario of baryogenesis, in which annihilation of axion domain walls generates a...
We show that axion domain wall is ferromagnetic in the universe with nonvanishing baryon number or l...
AbstractThe recent BICEP2 result shows that the Universe once has gone through the vacuum with the G...
The QCD axion with fafa at an intermediate scale, 109 GeV∼1012 GeV109 GeV∼1012 GeV, seems in conflic...
We are discussing some aspects of the magnetic monopoles and cosmic strings interactions with axion ...
Discrete symmetries play an important role in several extensions of the Standard Model (SM) of parti...
International audienceInspired by recent studies of high-scale decay constant or flavorful QCD axion...
We propose an extra-dimension framework on the orbifold $S^1/Z_2$ for understanding the origin of th...
The story of the Axion traces back to the so-called U(1) problem in QCD. In fact, QCD, restricted to...
We explore the effective theory of an axion in a gauged baryon number symmetry extension of the Stan...
The damping of the axionic string motion due to the surrounding plasma is estimated by a detailed ca...
I discretize axion string configuration coupled to a Dirac fermion, which in the continuum binds a m...
I review the dark energy solutions by a very light pseudoscalar called "quintessential axion". For t...
Axion-like particles (ALPs), a compelling candidate for dark matter (DM), are the pseudo Nambu-Golds...
We argue that demanding a consistent cosmological history, including the absence of domain walls and...
We propose a new scenario of baryogenesis, in which annihilation of axion domain walls generates a...
We show that axion domain wall is ferromagnetic in the universe with nonvanishing baryon number or l...
AbstractThe recent BICEP2 result shows that the Universe once has gone through the vacuum with the G...
The QCD axion with fafa at an intermediate scale, 109 GeV∼1012 GeV109 GeV∼1012 GeV, seems in conflic...
We are discussing some aspects of the magnetic monopoles and cosmic strings interactions with axion ...
Discrete symmetries play an important role in several extensions of the Standard Model (SM) of parti...
International audienceInspired by recent studies of high-scale decay constant or flavorful QCD axion...
We propose an extra-dimension framework on the orbifold $S^1/Z_2$ for understanding the origin of th...
The story of the Axion traces back to the so-called U(1) problem in QCD. In fact, QCD, restricted to...