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5421
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5422
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5423“…We suggest that supersymmetric dark matter be used to set the energy scale of a linear $e^+ e^-$ collider. …”
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5424
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5425“…Phys. 23 (1997) 2057-2067 We investigate the possible connection between the very penetrating component, frequently accompanying the cosmic-ray exotic phenomena, and the hypothesis of the formation of strangelets, in the process of strangeness distillation, being the last stage of the evolution of the quark matter droplet. We find that the many-maxima long-range cascades observed in the homogeneous lead emulsion chambers of the Pamir and Chacaltaya experiments can be produced in the process of strangelet penetration through the apparatus.…”
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5426
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5427
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5428Publicado 2000“…The four building blocks of everyday matter form a family composed of the up-quark,the down-quark,the electron and the electron-neutrino.Similar particles,heavier but oth- erwise identical,are known to exist -grouped together in two further families.…”
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5429
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5430
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5431
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5432
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5433
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5434“…Light neutralino dark matter cannot be primarily Higgsino in composition. (37 refs).…”
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5435“…We study the production of charm mesons and other charm baryons from quark matter at CERN SPS and RHIC energies. Using quark coalescence models as hadronization mechanism, we predict particle ratios, absolute yields and transverse momentum spectra.…”
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5436
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5437
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5438
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5439
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5440por McDonald, John“…More generally, for the case where the S mass is at least partially due to a bare mass term, if m_{S} \approx 10 \eta^{2/3} MeV, corresponding to self-interacting dark matter, then in order not to overpopulate the Universe with thermally generated S scalars we require that lambda_{S} < 10^{-(9-10)}\eta^{-1/3}, making such scalars difficult to detect directly.…”
Publicado 2001
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