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The laser star hypothesis is a hypothesis put forward by the physicist Y. P. Varshni in the early to mid 1970s in response to several developments in astrophysical and earth-based research, coupled with the acknowledgement of the fundamental difficulties suffered by the existing body of work on quasar. Modern observations have shown that stars with highly-energetic solar winds may be capable of natural lasing. This, along with laboratory based experimental and theoretical work involving plasma lasers, has lent support to the laser star hypothesis. Late twentieth century and early twenty-first century observations, coupled with reviews of previous observations in light of the decades-old discoveries made by experimental plasma physicists, demonstrate that the classical quasar model suffers many problems that have persistently been dealt with in an ad hoc fashion. The laser star hypothesis is not a per se challenge to the classical hypotheses regarding quasars, but is an overarching hypothesis which implies that many, if not all, quasar, or " quasi stellar objects," are instead laser stars. Indeed, the hypothesis was developed within the first ten years of the initial discovery of quasars.

1 Overview

Since the development of plasma lasers in the 1980s, the growing consensus has been that, due to the fully-ionized nature of the lasing medium, there seems to be no upper limit to the power output of such lasers. Plasma lasers are self-organizing, but not always coherent. Lasing media amplify anything within their bandwidth range, including spontaneous emissions in the medium itself, and plasma lasers are known to spontaneously produce polychromatic spectra. This is the proposed action which results in quasar activity. Within the laser star model, observational evidence exists which indicates that some quasars populate the local Virgo cluster, and may even be within the Milky Way galaxy.

2 Publications

3 External links





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