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The economical and organizational debates about open access have mostly been concerned with journals. This is not surprising since the open access movement can be seen largely as a response to the serials crisis. Recently the open access debate has been extended to include access to government produced data in different forms. In this presentation I'll critically look at some economic and organizational issues pertaining to the open access provision of bibliographical data.
In keeping with the views of its guru, Stephen Harnard, the open access movement is only prepared to discuss the two models of the "green road" and the "golden road" as sole alternatives for the future of scientific publishing. The "golden road" is put forward as the royal road for solving the journals crisis. However, no one has drawn attention to the fact that the golden road represents a purely socialist solution to a free-market problem and thus continues the "samizdat" tradition of underground literature in the former Eastern bloc. The present paper reveals the alarmingly low level at which the open access movement intends to publish top-class results from science and research, and the low degree of professionalism with which they are satisfied.
Der Vortrag wurde am 5th Frankfurt Scientific Symposium gehalten (22-23 Oktober 2005). Die Betrachtung des Videos ist (leider) nur mit den Browsern Internet Explorer ab 5.0, Netscape Navigator ab 7.0 oder Internet Explorer ab 5.2.2 für MaC möglich (s. Dokument 1.html). Die gesamten Tagungsbeiträge sind unter http://publikationen.ub.uni-frankfurt.de/volltexte/2005/1992/ abrufbar.
Within the scenario of large extra dimensions, the Planck scale is lowered to values soon accessible. Among the predicted effects, the production of TeV mass black holes at the LHC is one of the most exciting possibilities. Though the final phases of the black hole’s evaporation are still unknown, the formation of a black hole remnant is a theoretically well motivated expectation. We analyze the observables emerging from a black hole evaporation with a remnant instead of a final decay. We show that the formation of a black hole remnant yields a signature which differs substantially from a final decay. We find the total transverse momentum of the black hole event to be significantly dominated by the presence of a remnant mass providing a strong experimental signature for black hole remnant formation.