An Ongoing Meta-analysis of Gravitational Wave Signals may soon Prove that Space Remembers: permanent memory imprints in spacetime may soon be detected, which will be a validation of Nassim Haramein and our research team’s prediction that space has the property of memory, in which we described how the informational imprint of memory in space is what holographically generates time—that is to say that 4D spacetime is a holographic projection of a 3D voxel information network—as well as ordering properties underlying dynamics of organized matter. The gravitational wave memory effect is a prediction of general relativity, and physicists have devised a test of this interesting spacememory effect via a meta-analysis of gravitational wave detector data. The presence of memory effects in gravitational wave signals not only provides the chance to test an important aspect of general relativity, but also represents a potentially non-negligible contribution to the waveform for certain gravitational wave events. As well, memory properties of space will have far-reaching implications, from probing theories of quantum gravity and unified physics to potential applications in telecommunications technologies.
By: William Brown, scientist at the Resonance Science Foundation
Gravitational waves, oscillations or more colloquially “ripples” in the substantive medium of space-time, were first predicted by Albert Einstein's theory of general relativity over a century ago. These waves may be quite ubiquitous, what is known as the gravitational wave background (GWB), similar to the cosmic microwave background (CMB). The gravitational waves that have been detected to-date are generated by some of the most violent and energetic processes in the cosmos, such as the merging of black holes and neutron stars. However, a lesser-known phenomenon related to gravitational waves, termed the gravitational memory effect, has gained attention within the scientific community. This article delves into the intriguing concept of gravitational memory and its implications for our understanding of the fundamental forces of the universe.
Understanding Gravitational Waves
Gravitational waves are disturbances in the curvature of space-time, propagating as waves at the speed of light. They are generated when massive celestial objects accelerate asymmetrically, leading to oscillations in the gravitational field that radiate outwards. These ripples carry information about their origins and travel across the universe, allowing astronomers to probe the cosmos in a unique way.
The Gravitational Memory Effect
The gravitational memory effect is a manifestation of the persistent change in relative distances between test particles due to the passage of gravitational waves. Unlike the oscillatory nature of gravitational waves, the memory effect produces a permanent change in the separation of objects in its path. This phenomenon is a consequence of the non-linear nature of gravity in Einstein's theory of general relativity.
Types of Gravitational Memory
The gravitational memory effect can be classified into two types: positive and negative. A positive memory results in an increase in the separation of test particles, while a negative memory leads to a decrease. These changes occur along the direction of propagation of the gravitational wave.
History of Empirical Analysis of Gravitational Waves and Prediction of Memory Effect
Joseph Weber, an American physicist, claimed to have discovered gravitational radiation in the 1960s . He developed highly sensitive detectors known as Weber bars, which were designed to detect tiny vibrations caused by passing gravitational waves. His claim was based on the observations made using these detectors.
Weber's work garnered significant attention and excitement within the scientific community and the media. The potential discovery of gravitational radiation was groundbreaking, as it would have provided experimental confirmation of a fundamental prediction of Albert Einstein's theory of general relativity.
Weber's experiments involved aluminum cylinders, or "Weber bars," which were designed to resonate at specific frequencies when exposed to gravitational waves. Weber claimed to have detected gravitational waves emanating from various cosmic events, including supernova remnants and binary star systems.
However, over time, skepticism regarding the validity of Weber's results began to grow. Other researchers attempted to replicate his findings but faced challenges in reproducing the results with the same level of consistency and statistical significance. Physicists such as Yakov Zeldovich, a prominent Soviet theoretical physicist and cosmologist—who was instrumental in the formulation of how wave resonance can convert electromagnetic waves to gravitational waves—ran calculations that explicitly demonstrated how Weber’s bars would need to be 100 million times more sensitive than reported in order to detect even the largest theoretically possible gravitational wave sources, like from a super-dense highly-interacting cluster of stars.
However, the analysis utilized in proving Weber wrong led to a remarkable prediction. In the 1970’s in collaboration with his colleague Alexander Polnarev, Zeldovich predicted that passing gravitational waves should result in a permanent change in the relative separation of test particles, like a record or memory of the passing gravitational radiation. Their work laid the foundation for the theoretical understanding of the gravitational memory effect, emphasizing its potential significance in the study of gravitational waves and the implications for fundamental physics. Zeldovich and Polnarev's theoretical analysis provided a framework for subsequent researchers to explore this intriguing phenomenon in more detail.
Zeldovich's insights into the behavior of gravitational waves and their impact on spacetime were instrumental in advancing our understanding of how these waves can induce lasting alterations in the geometry of space. This pioneering work contributed to the development of experimental efforts to detect and study the gravitational memory effect.
While Zeldovich's role was primarily theoretical, his contributions have been fundamental in shaping our understanding of gravitational waves and their associated effects, including the gravitational memory. Subsequent experimental validations of the gravitational memory effect have further confirmed the accuracy of the predictions made by Zeldovich and Polnarev, solidifying their place in the history of gravitational wave research.
For Weber, several factors contributed to the doubts surrounding his claims:
As the years progressed, subsequent advancements in gravitational wave detection technologies, such as the Laser Interferometer Gravitational-Wave Observatory (LIGO), provided more accurate and reliable evidence for the existence of gravitational waves. LIGO's success in directly detecting gravitational waves in 2015 through the observation of merging black holes effectively discredited Weber's claims.
In retrospect, while Joseph Weber's work was influential in laying the groundwork for gravitational wave detection, subsequent advancements in technology and the success of more precise experiments have reshaped our understanding of gravitational waves and reinforced the accuracy of Einstein's general theory of relativity.
Black hole Memory Effect
The investigation of Weber’s claim of gravitational wave detection and subsequent elucidation and prediction of gravitational wave memory effects by Yakov Zeldovich and Alexander Polnarev led them to another related prediction of a similar effect occurring in the spacetime geometry of black hole’s event horizons—a “black hole memory effect”. This effect is a consequence of the non-linear nature of general relativity and arises when gravitational waves pass through a region of space near a black hole causes a distortion in the geometry of spacetime. This distortion leads to a change in the orbits and dynamics of particles in the vicinity of the black hole. Even after the gravitational waves have passed, this change persists, creating a lasting memory in the structure of spacetime.
In more technical terms, the black hole memory effect is related to the so-called "asymptotic symmetries" of gravity. These are transformations that affect the geometry of spacetime at infinity and can leave a permanent mark on the space surrounding a black hole. It is an important area of study in gravitational wave physics, helping researchers understand the lasting impact of gravitational waves on the fabric of the universe and its implications for astrophysics and fundamental physics.
Detecting the Non-linear Gravitational Memory Effect
By combining data from the gravitational wave detectors—large highly sensitive laser interferometers—LIGO, the Virgo detector in Italy, and the Kamioka detector in Japan it may be possible to tease out a tell-tale signal of gravitational wave memory effects from the meta-analysis of data . Such analysis is underway, with new observations rolling in every week, pushing the current total to over 100 and counting. At this rate, experimentalists hope they will detect gravitational memory within a few years. There is as well recent proposals to detect the gravitational memory effect in LISA using triggers from ground-based detectors, which will obviate the signal-to-noise (SNR) problem that arises because the memory effect is one or two orders below the detector noise background level , and to use the TianQin proposed space-based gravitational wave observatory designed to detect and study gravitational waves with high precision and sensitivity .
TianQin is conceived as a space-based gravitational wave observatory that aims to observe gravitational waves with lower frequencies (millihertz to hertz range). This complements ground-based observatories like LIGO and Virgo, which detect higher-frequency gravitational waves. The TianQin observatory relies on a constellation of three spacecraft forming an equilateral triangle in space. These spacecraft will be equipped with highly sensitive lasers and accelerometers to measure the tiny displacements caused by passing gravitational waves. TianQin's lower frequency range allows it to detect gravitational waves from different sources, such as massive binary systems (e.g., merging supermassive black holes), extreme mass ratio inspirals (e.g., a small compact object orbiting a massive black hole), and other astrophysical events.
TianQin is a proposed space-based gravitational wave detector, like the Laser Interferometer Space Antenna (LISA) pictured above in Artist's impression. Credit: ESA
Being in space, TianQin is free from the seismic noise and other disturbances that can affect ground-based detectors. This enables it to detect lower frequency gravitational waves with greater sensitivity and accuracy. During its five years of operation, for the gravitational wave signals that could be detected by TianQin, about 0.5–2.0 signals may contain displacement memory effect with SNR ratios greater than 3. This suggests that the chance for TianQin to detect the displacement memory effect directly is low but not fully negligible.
Implications and Application
Studying the gravitational memory effect allows physicists to probe the fundamental nature of gravity and its behavior in extreme conditions. This phenomenon holds promise in enhancing our understanding of the intricate interplay between gravity and other fundamental forces in the universe.
Gravitational waves, including their memory effect, provide a powerful tool for studying astrophysical phenomena. They offer insights into the dynamics of compact binary systems, the properties of merging black holes, neutron stars, and the early universe. Gravitational memory can be a valuable addition to our observational toolkit for understanding cosmic events.
The near-undetectable perturbation effect of gravitational wave memory is a relatively subtle indication of the memory attribute of space arising from the vacuum’s substantive properties as a physical medium, but it is not the only mechanism by which the memory properties of space can potentially be manifest. For example, gravitational interaction is proposed to mediate such quintessentially quantum mechanical behavior as entanglement, such as in the ERb=EPR holographic correspondence conjecture by Susskind and Maldacena . As such, the entanglement nexus of spacememory may be integral in encoding naturally occurring qubit memory states of interacting systems all around us .
In terms of what investigating gravitational waves can help us to learn about astrophysics, cosmology, and quantum gravity, it is important to note that within our unified physics approach gravitational waves are not just being generated by massively high-energy events like black hole mergers. We predict that gravitational waves will be a quite ubiquitous phenomenon occurring at many scales. Gravitational waves probably emanate from fundamental particles like the proton and are even generated at the Planck scale. The role of such oscillatory radiation of spacetime itself will form a significant contribution to the energy dynamics of material systems, and the complex interplay of many-bodied radiative sources generating constructive and destructive interference wave forms and wave resonance may very well be a significant factor in the holographic memory properties of space.
The gravitational memory effect, a consequence of gravitational waves, remains a fascinating and relatively unexplored aspect of general relativity. As gravitational wave detection technology advances, scientists are eager to unravel the mysteries surrounding this phenomenon. Unveiling the gravitational memory effect not only expands our understanding of the fundamental forces shaping the cosmos but also holds promise for a deeper comprehension of the intricate dance of the universe.
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