Supersymmetric Q-balls trapped in neutron stars or white dwarfs may cause the stars to explode. Trapping of Q-balls in neutron stars is shown to be less likely, but trapping in neutron star progenitors more likely than hitherto assumed, making neutron stars very sensitive Q-ball "detectors". White dwarfs only trap potentially dangerous Q-balls in a narrow parameter range
The properties and cosmological importance of a class of non-topological solitons, Q-balls, are stud...
Future experiments may discover new scalar particles with global charges and couplings that allow fo...
All supersymmetric generalizations of the Standard Model allow for stable non-topological solitons o...
Supersymmetric extensions of the Standard Model contain non-topological solitons, Q-balls, which can...
Stable baryonic Q-balls, which appear in supersymmetric extensions of the Standard Model, could form...
In this paper we present some features of Q-balls and we discuss their interactions with matter, and...
Collisions of non-topological solitons, Q-balls, are studied in the Minimal Supersymmetric Standard ...
MSSM predicts the existence of Q-balls, some of which can be entirely stable. Both stable and unstab...
Collisions of non-topological solitons, Q-balls, are studied in a typical potential in the Minimal S...
After a short review of Q-balls properties, in this paper we discuss their interaction with matter, ...
Supersymmetric models predict a natural dark-matter candidate, stable baryonic Q-balls. They could b...
In the MSSM with gravity mediated supersymmetry breaking, there may exist unstable but long-lived so...
The kilohertz frequencies of QPOs from accreting neutron star systems imply that they are generated ...
We obtain a new type of a stable Q ball in the context of gauge-mediated SUSY breaking in MSSM. It i...
The existence of deconfined quark matter in the superdense interior of neutron stars is a key questi...
The properties and cosmological importance of a class of non-topological solitons, Q-balls, are stud...
Future experiments may discover new scalar particles with global charges and couplings that allow fo...
All supersymmetric generalizations of the Standard Model allow for stable non-topological solitons o...
Supersymmetric extensions of the Standard Model contain non-topological solitons, Q-balls, which can...
Stable baryonic Q-balls, which appear in supersymmetric extensions of the Standard Model, could form...
In this paper we present some features of Q-balls and we discuss their interactions with matter, and...
Collisions of non-topological solitons, Q-balls, are studied in the Minimal Supersymmetric Standard ...
MSSM predicts the existence of Q-balls, some of which can be entirely stable. Both stable and unstab...
Collisions of non-topological solitons, Q-balls, are studied in a typical potential in the Minimal S...
After a short review of Q-balls properties, in this paper we discuss their interaction with matter, ...
Supersymmetric models predict a natural dark-matter candidate, stable baryonic Q-balls. They could b...
In the MSSM with gravity mediated supersymmetry breaking, there may exist unstable but long-lived so...
The kilohertz frequencies of QPOs from accreting neutron star systems imply that they are generated ...
We obtain a new type of a stable Q ball in the context of gauge-mediated SUSY breaking in MSSM. It i...
The existence of deconfined quark matter in the superdense interior of neutron stars is a key questi...
The properties and cosmological importance of a class of non-topological solitons, Q-balls, are stud...
Future experiments may discover new scalar particles with global charges and couplings that allow fo...
All supersymmetric generalizations of the Standard Model allow for stable non-topological solitons o...