It is shown that the fusion of strings is a source of particle production in nucleus--nucleus collisions outside the kinematical limits of nucleon--nucleon collisions. This fact, together with another effect of string fusion, the reduction of multiplicities, sheds some light on two of the main problems of ultrahigh energy cosmic rays the chemical composition and the energy of the most energetic detected cosmic rays
Decaying topological defects, in particular cosmic strings, can produce a significant flux of high e...
The several types of strongly intensive correlation variables are studied in nuclear collisions at L...
Recently, models proposing superheavy particles $X$ as source of ultrahigh energy cosmic rays have a...
At high gluon or string densities, gluons' saturation or the strong interaction among strings, eithe...
The quark-gluon strings model succeeds in the description of multiple hadron production in the centr...
Presented at the XXV International School of Theoretical Physics "Particles and Astrophysics - Stand...
The flux is calculated of ultrahigh energy protons due to the process of cusp evaporation from cosmi...
String Fusion Model Code results for Pb--Pb central collisions at SPS energies including the string ...
We present a new solution for the problem of ultra high energy cosmic ray events with energy up to 3...
Measurements of proton and nuclear collisions at the Large Hadron Collider at nucleon-nucleon c.m. e...
In this work we argue that, in the interpretation of the energy dependence of the depth of the showe...
Recent experimental data on antibaryon production outside nucleon-nucleon kinematical limits have be...
28 pages, ReVTex, 5 postscript figures. Minor changes, some references added. Submitted to Phys. Rev...
We critically review the common belief that ultrahigh energy cosmic rays are protons or atomic nucle...
Cosmic rays from outer space enter the atmosphere with energies of up to 10^{11} GeV. The initial pa...
Decaying topological defects, in particular cosmic strings, can produce a significant flux of high e...
The several types of strongly intensive correlation variables are studied in nuclear collisions at L...
Recently, models proposing superheavy particles $X$ as source of ultrahigh energy cosmic rays have a...
At high gluon or string densities, gluons' saturation or the strong interaction among strings, eithe...
The quark-gluon strings model succeeds in the description of multiple hadron production in the centr...
Presented at the XXV International School of Theoretical Physics "Particles and Astrophysics - Stand...
The flux is calculated of ultrahigh energy protons due to the process of cusp evaporation from cosmi...
String Fusion Model Code results for Pb--Pb central collisions at SPS energies including the string ...
We present a new solution for the problem of ultra high energy cosmic ray events with energy up to 3...
Measurements of proton and nuclear collisions at the Large Hadron Collider at nucleon-nucleon c.m. e...
In this work we argue that, in the interpretation of the energy dependence of the depth of the showe...
Recent experimental data on antibaryon production outside nucleon-nucleon kinematical limits have be...
28 pages, ReVTex, 5 postscript figures. Minor changes, some references added. Submitted to Phys. Rev...
We critically review the common belief that ultrahigh energy cosmic rays are protons or atomic nucle...
Cosmic rays from outer space enter the atmosphere with energies of up to 10^{11} GeV. The initial pa...
Decaying topological defects, in particular cosmic strings, can produce a significant flux of high e...
The several types of strongly intensive correlation variables are studied in nuclear collisions at L...
Recently, models proposing superheavy particles $X$ as source of ultrahigh energy cosmic rays have a...