Physical Publicly Verifiable Randomness from Pulsars
J. R. Dawson (1, 2), George Hobbs (1), Yansong Gao (3), Seyit, Camtepe (4), Josef Pieprzyk (4, 5), Yi Feng (6, 7), Luke Tranfa (1 and, 2), Sarah Bradbury (1, 8), Weiwei Zhu (6, 7), Di Li (6, 7, 9)., ((1) CSIRO Space, Astronomy, (2) Department of Physics, Astronomy and

TL;DR
This paper explores using pulsar signals as a natural, publicly verifiable source of randomness, providing a quantum-resistant alternative for cryptographic and other applications.
Contribution
It demonstrates that pulsar flux densities can generate verifiable random sequences and compares extraction methods across multiple observatories, addressing noise effects.
Findings
Pulsar signals pass standard randomness tests.
Same bit sequences can be obtained at different observatories.
Radiometer noise impacts bit error rates.
Abstract
We demonstrate how radio pulsars can be used as random number generators. Specifically, we focus on publicly verifiable randomness (PVR), in which the same sequence of trusted and verifiable random numbers is obtained by multiple parties. PVR is a critical building block for many processes and algorithms (including cryptography, scientific trials, electoral audits and international treaties). However, current approaches (based on number theory) may soon become vulnerable to quantum computers, motivating a growing demand for PVR based on natural physical phenomena. In this context, we explore pulsars as a potential physical PVR source. We first show that bit sequences extracted from the measured flux densities of a bright millisecond pulsar can pass standardised tests for randomness. We then quantify three illustrative methods of bit-extraction from pulsar flux density sequences, using…
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Taxonomy
TopicsRadio Astronomy Observations and Technology
