Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-21T15:45:58.884Z Has data issue: false hasContentIssue false
  • English
  • Français

Planck frequencies as Schelling points in SETI – Erratum

Published online by Cambridge University Press:  19 November 2020

Jason T. Wright
Rights & Permissions [Opens in a new window]

Abstract

An abstract is not available for this content. As you have access to this content, full HTML content is provided on this page. A PDF of this content is also available in through the ‘Save PDF’ action button.
Type
Erratum
Information
International Journal of Astrobiology , Volume 19 , Issue 6 , December 2020 , pp. 515 - 518
Check for updates
Copyright
Copyright © The Author(s), 2020. Published by Cambridge University Press

The Publisher apologises that due to a typesetting error all instances of μ were rendered as m in Tables 2 and 5, making the units of some entries incorrect by a factor of 103.

Additionally, there are missing minus signs in equations (5) and (7) in Tables 2 and 5, as well as in the table notes of Tables 3 and 4. The correct equations are:

(5)$$n_{\hbar , e} = - {\rm ln\;}( {E / E _{P} {\rm }} ) $$
(7)$$n_{h, e} = -\ln \;\left({E/\sqrt {hc^5\;/G } } \right)$$

The correct tables are as below

Table 2. The Planck frequency comb with ${\hbar} \rightarrow h$

$n_{h, \alpha } =\log {( E/\sqrt {hc^5/G}) }/ \! \log {( e^2/( ch) ) }$.

This set contains no convenient lines in the optical or near-infrared.

Table 3. The Planck frequency comb with $\hbar \rightarrow h$ and base e

$n_{h, e} =-\ln {( E/\sqrt {hc^5/G}) }$.

Table 4. The Planck frequency comb with base e

$n_{\hbar, e} =- \ln {( E/E_{\rm P}) }$.

Table 5. The Rydberg frequency comb $n_{R} = \log _\alpha {( E/( m_{\rm e}c^2/2) ) }$.

References

Wright, JT (2020) Planck frequencies as Schelling points in SETI. International Journal of Astrobiology 1–10. doi: 10.1017/S1473550420000221.Google Scholar
Figure 0

Table 2. The Planck frequency comb with ${\hbar} \rightarrow h$$n_{h, \alpha } =\log {( E/\sqrt {hc^5/G}) }/ \! \log {( e^2/( ch) ) }$.This set contains no convenient lines in the optical or near-infrared.

Figure 1

Table 3. The Planck frequency comb with $\hbar \rightarrow h$ and base e$n_{h, e} =-\ln {( E/\sqrt {hc^5/G}) }$.

Figure 2

Table 4. The Planck frequency comb with base e$n_{\hbar, e} =- \ln {( E/E_{\rm P}) }$.

Figure 3

Table 5. The Rydberg frequency comb $n_{R} = \log _\alpha {( E/( m_{\rm e}c^2/2) ) }$.