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Miller WB. A scale-free universal relational information matrix (N-space) reconciles the information problem: N-space as the fabric of reality. Commun Integr Biol 2023; 16:2193006. [PMID: 37188326 PMCID: PMC10177686 DOI: 10.1080/19420889.2023.2193006] [Citation(s) in RCA: 5] [Impact Index Per Article: 2.5] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/17/2023] [Revised: 03/14/2023] [Accepted: 03/15/2023] [Indexed: 05/17/2023] Open
Abstract
Cellular measurement is a crucial faculty in living systems, and exaptations are acknowledged as a significant source of evolutionary innovation. However, the possibility that the origin of biological order is predicated on an exaptation of the measurement of information from the abiotic realm has not been previously explored. To support this hypothesis, the existence of a universal holographic relational information space-time matrix is proposed as a scale-free unification of abiotic and biotic information systems. In this framework, information is a universal property representing the interactions between matter and energy that can be subject to observation. Since observers are also universally distributed, information can be deemed the fundamental fabric of the universe. The novel concept of compartmentalizing this universal N-space information matrix into separate N-space partitions as nodes of informational density defined by Markov blankets and boundaries is introduced, permitting their applicability to both abiotic and biotic systems. Based on these N-space partitions, abiotic systems can derive meaningful information from the conditional settlement of quantum entanglement asymmetries and coherences between separately bounded quantum informational reference frames sufficient to be construed as a form of measurement. These conditional relationships are the precursor of the reiterating nested architecture of the N-space-derived information fields that characterize life and account for biological order. Accordingly, biotic measurement and biological N-space partitioning are exaptations of preexisting information processes within abiotic systems. Abiotic and biotic states thereby reconcile as differing forms of measurement of fundamental universal information. The essential difference between abiotic and biotic states lies within the attributes of the specific observer/detectors, thereby clarifying several contentious aspects of self-referential consciousness.
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Hannam M, Hoy C, Thompson JE, Fairhurst S, Raymond V, Colleoni M, Davis D, Estellés H, Haster CJ, Helmling-Cornell A, Husa S, Keitel D, Massinger TJ, Menéndez-Vázquez A, Mogushi K, Ossokine S, Payne E, Pratten G, Romero-Shaw I, Sadiq J, Schmidt P, Tenorio R, Udall R, Veitch J, Williams D, Yelikar AB, Zimmerman A. General-relativistic precession in a black-hole binary. Nature 2022; 610:652-655. [PMID: 36224390 DOI: 10.1038/s41586-022-05212-z] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/19/2022] [Accepted: 08/09/2022] [Indexed: 11/09/2022]
Abstract
The general-relativistic phenomenon of spin-induced orbital precession has not yet been observed in strong-field gravity. Gravitational-wave observations of binary black holes (BBHs) are prime candidates, as we expect the astrophysical binary population to contain precessing binaries1,2. Imprints of precession have been investigated in several signals3-5, but no definitive identification of orbital precession has been reported in any of the 84 BBH observations so far5-7 by the Advanced LIGO and Virgo detectors8,9. Here we report the measurement of strong-field precession in the LIGO-Virgo-Kagra gravitational-wave signal GW200129. The binary's orbit precesses at a rate ten orders of magnitude faster than previous weak-field measurements from binary pulsars10-13. We also find that the primary black hole is probably highly spinning. According to current binary population estimates, a GW200129-like signal is extremely unlikely, and therefore presents a direct challenge to many current binary-formation models.
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Affiliation(s)
- Mark Hannam
- Gravity Exploration Institute, Cardiff University, Cardiff, UK.
| | - Charlie Hoy
- Gravity Exploration Institute, Cardiff University, Cardiff, UK
| | | | | | - Vivien Raymond
- Gravity Exploration Institute, Cardiff University, Cardiff, UK
| | - Marta Colleoni
- Departament de Física, Universitat de les Illes Balears, Palma, Spain
| | - Derek Davis
- LIGO Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - Héctor Estellés
- Departament de Física, Universitat de les Illes Balears, Palma, Spain
| | - Carl-Johan Haster
- LIGO Laboratory, Massachusetts Institute of Technology, Cambirdge, MA, USA
| | | | - Sascha Husa
- Departament de Física, Universitat de les Illes Balears, Palma, Spain
| | - David Keitel
- Departament de Física, Universitat de les Illes Balears, Palma, Spain
| | - T J Massinger
- LIGO Laboratory, Massachusetts Institute of Technology, Cambirdge, MA, USA
| | - Alexis Menéndez-Vázquez
- Institut de Fìsica d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Barcelona, Spain
| | - Kentaro Mogushi
- Missouri University of Science and Technology, Rolla, MO, USA
| | - Serguei Ossokine
- Max Planck Institute for Gravitational Physics, Potsdam, Germany
| | - Ethan Payne
- LIGO Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - Geraint Pratten
- Institute for Gravitational Wave Astronomy and School of Physics and Astronomy, University of Birmingham, Birmingham, UK
| | - Isobel Romero-Shaw
- School of Physics and Astronomy, Monash University, Clayton, Victoria, Australia.,OzGrav: The ARC Centre of Excellence for Gravitational Wave Discovery, Clayton, Victoria, Australia.,Department of Applied Mathematics and Theoretical Physics, Cambridge, UK
| | - Jam Sadiq
- Instituto Galego de Fisica de Altas Enerxias, Universidade de Santiago de Compostela, Santiago de Compostela, Spain
| | - Patricia Schmidt
- Institute for Gravitational Wave Astronomy and School of Physics and Astronomy, University of Birmingham, Birmingham, UK
| | - Rodrigo Tenorio
- Departament de Física, Universitat de les Illes Balears, Palma, Spain
| | - Richard Udall
- LIGO Laboratory, California Institute of Technology, Pasadena, CA, USA
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Krishnan VV, Bailes M, van Straten W, Wex N, Freire PCC, Keane EF, Tauris TM, Rosado PA, Bhat NDR, Flynn C, Jameson A, Osłowski S. Lense-Thirring frame dragging induced by a fast-rotating white dwarf in a binary pulsar system. Science 2020; 367:577-580. [PMID: 32001656 DOI: 10.1126/science.aax7007] [Citation(s) in RCA: 31] [Impact Index Per Article: 6.2] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/10/2019] [Accepted: 12/03/2019] [Indexed: 11/03/2022]
Abstract
Radio pulsars in short-period eccentric binary orbits can be used to study both gravitational dynamics and binary evolution. The binary system containing PSR J1141-6545 includes a massive white dwarf (WD) companion that formed before the gravitationally bound young radio pulsar. We observed a temporal evolution of the orbital inclination of this pulsar that we infer is caused by a combination of a Newtonian quadrupole moment and Lense-Thirring (LT) precession of the orbit resulting from rapid rotation of the WD. LT precession, an effect of relativistic frame dragging, is a prediction of general relativity. This detection is consistent with an evolutionary scenario in which the WD accreted matter from the pulsar progenitor, spinning up the WD to a period of <200 seconds.
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Affiliation(s)
- V Venkatraman Krishnan
- Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne, Victoria 3122, Australia. .,Max-Planck-Institut für Radioastronomie, D-53121 Bonn, Germany
| | - M Bailes
- Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne, Victoria 3122, Australia.,Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav), Swinburne University of Technology, Melbourne, Victoria 3122, Australia
| | - W van Straten
- Institute for Radio Astronomy and Space Research, Auckland University of Technology, Auckland 1142, New Zealand
| | - N Wex
- Max-Planck-Institut für Radioastronomie, D-53121 Bonn, Germany
| | - P C C Freire
- Max-Planck-Institut für Radioastronomie, D-53121 Bonn, Germany
| | - E F Keane
- Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne, Victoria 3122, Australia.,Square Kilometer Array Organisation, Jodrell Bank Observatory, Macclesfield SK11 9DL, UK
| | - T M Tauris
- Aarhus Institute of Advanced Studies, Aarhus University, 8000 Aarhus C, Denmark.,Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark.,Max-Planck-Institut für Radioastronomie, D-53121 Bonn, Germany
| | - P A Rosado
- Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne, Victoria 3122, Australia
| | - N D R Bhat
- International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia 6102, Australia
| | - C Flynn
- Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne, Victoria 3122, Australia
| | - A Jameson
- Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne, Victoria 3122, Australia
| | - S Osłowski
- Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne, Victoria 3122, Australia
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