Are Niven Rings Around Pulsars Detectable?

Are the Dyson rings around pulsars detectable?

Authors:

Osmanov

Abstract:
In the previous paper (Osmanov 2016) (henceforth Paper-I) we have extended the idea of Freeman Dyson and have shown that a supercivilization has to use ring-like megastructures around pulsars instead of a spherical shell. In this work we reexamine the same problem in the observational context and we show that facilities of modern IR telescopes (VLTI and WISE) might efficiently monitor the nearby zone of the solar system and search for the IR Dyson-rings up to distances of the order of 0.2kpc, corresponding to the current highest achievable angular resolution, 0.001mas. In this case the total number of pulsars in the observationally reachable area is about 64±21. We show that pulsars from the distance of the order of ∼1kpc are still visible for WISE as point-like sources but in order to confirm that the object is the neutron star, one has to use the UV telescopes, which at this moment cannot provide enough sensitivity.

Improving on the Kardashev Scale

Kardashev's Classification at 50+: A Fine Vehicle with Room for Improvement

Authors:

Cirkovic et al

Abstract:

We review the history and status of the famous classification of extraterrestrial civilizations given by the great Russian astrophysicist Nikolai Semenovich Kardashev, roughly half a century after it has been proposed. While Kardashev's classification (or Kardashev's scale) has often been seen as oversimplified, and multiple improvements, refinements, and alternatives to it have been suggested, it is still one of the major tools for serious theoretical investigation of SETI issues. During these 50+ years, several attempts at modifying or reforming the classification have been made; we review some of them here, together with presenting some of the scenarios which present difficulties to the standard version. Recent results in both theoretical and observational SETI studies, especially the G-hat infrared survey (2014-2015), have persuasively shown that the emphasis on detectability inherent in Kardashev's classification obtains new significance and freshness. Several new movements and conceptual frameworks, such as the Dysonian SETI, tally extremely well with these developments. So, the apparent simplicity of the classification is highly deceptive: Kardashev's work offers a wealth of still insufficiently studied methodological and epistemological ramifications and it remains, in both letter and spirit, perhaps the worthiest legacy of the SETI "founding fathers".

Hunting for Macro-artefacts (Dyson Spheres, etc) for SETI

Reconsidering macro-artefacts in SETI searches

Author:

Jones

Abstract:

The observation of macro-artefacts at interstellar distances offers an alternative search paradigm to SETI programs such as radio astronomy and laser detection. Potential artefacts range from space infrastructure deployed by advanced technological civilizations to deliberate attempts to use artefacts as signals and biomarkers of intelligent life. Passive observations of macro-artefacts could overcome problems with active transmission messaging such as temporal and spatial constraints.

Artefacts could be detected without being spatially resolved by telescopes. Spectral analyses could yield evidence of disruption of the natural electromagnetic spectra of stars by artefacts. Some artefacts could generate diffraction and interference patterns uncharacteristic of natural phenomena. Thus, detecting macro-artefacts is potentially feasible with current astronomical infrastructure.

The construction of large macro-artefacts could be achieved with technological and industrial capabilities that are roughly equivalent to present-day Earth. Thus, the accessibility of macro-artefacts for both transmission and reception can be reconsidered as potentially equivalent to conventional SETI strategies.

Hunting for Dyson Spheres With IRAS