Discover how scientists are constraining the dynamics of rotating black holes using gauge symmetry principles to better understand their evolution and behaviour in space.
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Mysterious Dynamics of Rotating Black Holes
Unlocking the secrets of Kerr black holes: Scientists from Uppsala University, Oxford and Mons propose a theoretical framework based on large, high-spin particles and symmetry measurements to explain the evolution of black holes. This study, published in Physical Review Letters, aims to constrain the Compton scattering amplitude, paving the way for a better understanding of the behaviour of Kerr black and its potential use in future experiments such as the Einstein Telescope, LISA and the Cosmic Explorer. TO DO.
In 2015, the LIGO/Virgo experiment, a large research project based on two American observatories, made the first direct observation of gravitational waves. This important moment led scientists around the world to develop a new explanation for the changes occurring in the black hole, based on data collected by the LIGO/Virgo collaboration. Researchers from the University of Uppsala, Oxford and Mons recently set out to explain the dynamics of Kerr black holes, a theoretical hypothesis that black holes rotate at a constant speed, using the theory of massive objects.
Their paper, published in Physical Review Letters, specifically states that the power of rotating black holes is limited by the principle of gauge symmetry. This shows that some changes in the body are not measurable. Henrik Johansson, author of the paper, told Phys.org: “We found a link between rotating Kerr black holes and higher spin mass. “In other words, we modelled a black hole as a fundamental connection, similar to the way electrons are treated in quantum electrodynamics.
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The link between Kerr black holes and overthinking was first discovered in two separate papers published in 2019. The first study was led by Alfredo Guevara of the Perimeter Institute for Theoretical Physics and his colleagues in Europe, and the second was led by Ming-Zhi Chung of the National Taiwan University and his colleagues of the National University of Seoul.
Previous studies have shown that the well-known Kerr measurement can be performed in an infinite range of higher amplitudes. The amplitudes were first obtained by physicists Nima Arkani-Hamed, Tzu-Chen Huang and Yu-tin Huang in previous research. “These previous results are surprising, but they are still not enough to explain the energy of the Kerr black hole, considering future experiments such as the Einstein Telescope, LISA and Space Explorers,” Johansson said. “Some important missing information is contained in the amplitude of the Compton black hole burst, which is currently generally unknown.”
In this paper, Johansson and colleagues show that the symmetry principle can be used to predict the effects of black hole evolution. Scientists have shown that the magnitude of large-scale rotation, known from the machine first described by Ernst Stueckelberg and later invented by Yurii Zinoviev, can be used to create the magnitudes of Kerr cracks reported in the previous article.
“We also found that the unknown Compton scattering amplitude is severely limited, although additional techniques are needed to achieve this specification,” Johansson said. “High-spin quantum field theories (QFTs) are known for their complexity. Low-spin QFTs, such as the spin-1 case of the Standard Model and the spin-2 case of relativity, are difficult. The process is based on the measurement of symmetry and heterogeneity. These two symmetries can be thought of as the two lowest rungs of an infinite ladder called higher spin gauge symmetries. “
Although the symmetry test is not necessary to describe the strength of large objects, it has proven to be a useful tool for showing relationships. One of the known aspects of this scale is the so-called Higgs mechanism. Johansson explained that “using the large-scale measurement system for the black hole allowed us to ensure that the degree of freedom was fixed continuously and recorded the Lagrangian quality,” Johansson explained. “Lagrangians both provide a useful description of Kerr black holes. “The behaviour is not essential for classical black holes, but it gives us confidence that the theory will explain some quantum processes.”
Johansson and his colleagues were the first to use a higher-resolution index for black holes. The results of the first calculations are promising and will soon pave the way for further research.
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“We anticipate that it will take some time before we understand the theory of black hole evolution, but we believe that the more important the measurement equation is in its structure, the more gauge symmetries and heteromorphic symmetries have taken on theory. “do.” Johansson said “The framework of 20th century physics,” Johansson said. “The total Compton scattering amplitude for the Kerr black hole remains a mystery, but we hope to be able to constrain it completely in the future. This must be understood both by arbitrary rotational orders and by higher orders of Newton’s constant.”
Fully constraining the diffusion of Kerr black holes requires collaboration between theoretical researchers studying large, highly rotating particles and those trying to solve the Teukolsky equation, which relies on comparison. Recent partnerships between these different research communities suggest that progress may be imminent.
“In our next research, we want to find a continuum between black holes and quantum energy reminiscent of fundamental particles,” Johansson added.
Source: by Ingrid Fadelli , Phys.org
Conclusion
The current study by scientists from Uppsala University, the University of Oxford and the University of Mons sheds light on the fascinating dynamics of Kerr black holes. Using a theoretical framework based on massive high-spin particles and the principle of gauge symmetry, the researchers wish to explain the evolution of these rotating black holes. Their study, published in Physical Review Letters, addresses the challenge of understanding the unknown domain of Compton scattering, which is crucial to a comprehensive understanding of the behaviour of black holes.
Kerr’s groundbreaking link proposed between black holes and high-spin theories builds on previous research in 2019. This link opens up opportunities to explore the complex dynamics of rotating black holes. It provides valuable insights that may be important for future experiments such as the Einstein Telescope, LISA, and space probes.
The use of symmetries, based on the theories of Stockelberg and Zinoviev, provides a promising method for predicting the effects of black hole growth. The study does not present a new approach only by modelling the black hole as basic particles but also contributes to the continuous dialogue between theoretical physicists, who study large particles of high rotation and which is Tukolski who works in the accuracy of the equation. General relativity.
By realizing the complexity of the highest field principles in the highest region, researchers express their confidence in their ability to completely limit the computing offer to compete for the black hole in Kiir. These developments, combined with collaborations between diverse research communities, send optimistic signals for future progress in understanding the quantum processes involved in black hole dynamics.
In the future, scientists expect further exploration of the continuum between quantum energies such as black holes and elementary particles. The research community is ready to embark on the journey to uncover the secrets of Kerr black holes, with the hope that continued collaboration and theoretical advances will lead to a comprehensive and comprehensive understanding of these fascinating astronomical objects. Masu.
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