It is proposed that the fireballs invoked to explain the Centauro events are bubbles of a metastable superdense state of nuclear matter, created in high energy (E approximately 10 to the 15th power eV) cosmic ray collisions at the top of the atmosphere. If these bubbles are created with a Lorentz factor gamma approximately equals 10 at their CM frame, the objections against the origin of these events in cosmic ray interactions are overcome. A relationship then between their lifetime, tau, and the threshold energy for bubble formation, E sub th, appears to be insensitive to the value of tau and always close to E sub th approximately 10 to 15th power eV. Finally it is speculated that these bubbles might be manifestations of the SU(2) x U(1) f...
Massive stars blow powerful winds and eventually explode as supernovae. By doing so, they inject ene...
There are two processes of matter creation after inflation that may be relevant to the resolution of...
A re-examination of the energy cosmic ray spectrum above $10^{20}$ eV is presented. The overall data...
It is proposed that the fireballs invoked to explain the Centauro events are bubbles of a metastable...
The cosmic-ray exotic event "Centauro-I" is reexamined. Kopenkin et al. [Phys. Rev. D 68, 052007 (20...
The requirements for observing Centauro-like phenomena and their role as possible probes of deeply p...
Presentation made at the 26th International Cosmic Ray Conference, ICRC '99We discuss the possible m...
We speculate that, in very high energy hadronic collisions, large fireballs may be produced with int...
It is shown that high-energy features of the cosmic ray spectrum, in particular the kink around 4 Pe...
In this chapter I give an overview of shock acceleration, including a discussion of the maximum ener...
We propose that the origin of ultra-high energy cosmic rays beyond the GZK cutoff and the origin of ...
We show that a simple scaling model of very forward particle production, consistent with accelerator...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
It has been recently proposed that dark matter in the Universe might consist of nuggets of quarks wh...
It has been known for more than a century that the interstellar medium is full of charged particles ...
Massive stars blow powerful winds and eventually explode as supernovae. By doing so, they inject ene...
There are two processes of matter creation after inflation that may be relevant to the resolution of...
A re-examination of the energy cosmic ray spectrum above $10^{20}$ eV is presented. The overall data...
It is proposed that the fireballs invoked to explain the Centauro events are bubbles of a metastable...
The cosmic-ray exotic event "Centauro-I" is reexamined. Kopenkin et al. [Phys. Rev. D 68, 052007 (20...
The requirements for observing Centauro-like phenomena and their role as possible probes of deeply p...
Presentation made at the 26th International Cosmic Ray Conference, ICRC '99We discuss the possible m...
We speculate that, in very high energy hadronic collisions, large fireballs may be produced with int...
It is shown that high-energy features of the cosmic ray spectrum, in particular the kink around 4 Pe...
In this chapter I give an overview of shock acceleration, including a discussion of the maximum ener...
We propose that the origin of ultra-high energy cosmic rays beyond the GZK cutoff and the origin of ...
We show that a simple scaling model of very forward particle production, consistent with accelerator...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
It has been recently proposed that dark matter in the Universe might consist of nuggets of quarks wh...
It has been known for more than a century that the interstellar medium is full of charged particles ...
Massive stars blow powerful winds and eventually explode as supernovae. By doing so, they inject ene...
There are two processes of matter creation after inflation that may be relevant to the resolution of...
A re-examination of the energy cosmic ray spectrum above $10^{20}$ eV is presented. The overall data...