Einstein must be wrong: How general relativity fails to explain the universe

Could Einstein Be Wrong? Theory of Gravity May Have Shortcomings in Explaining the UniverseKendra Stacy

Nov 15, 2023
While the popular theory of gravity, or general relativity, of Einstein boasts of success that has lasted for over a century, it does have its own theoretical shortcoming when it comes to explaining the Universe.

The theory of gravity has only been tested in gravity that is weak. This is unlike other physical theories that describe the three other fundamental physics forces, namely, the strong, weak, and electromagnetic nuclear interactions.

General relativity's gravity deviations are not tested nor excluded anywhere in the Universe. Theoretical physicists think that deviation is necessary.

held that the Universe started with the Big Bang. There are other singularities that can be found within black holes. Within these massive cosmic mysteries, time and space become meaningless, while pressure and energy density end up becoming infinite. These show that the theory of Einstein fails there and that a more fundamental theory should replace it.
Quantum mechanics should be able to resolve singularities in spacetime. Quantum physics typically depends on two ideas, namely, the Heinsenberg uncertainty principle that holds that no one can know a certain quantity pair's value with absolute accuracy and that point particles do not have sense.

This is sufficient enough to understand that such pathologies should not be present in a theory that embraces quantum physics and general relativity. However, Einstein's theory ends up with deviations when attempts are made to mix quantum physics and general relativity.

This means that the general theory of relativity proposed by Einstein cannot be the utmost theory of gravity. Interestingly, Arthur Eddington began looking for alternatives shortly after Einstein's theory was introduced. Eddington is known for verifying the theory during the solar eclipse in 1919.

The theory of Einstein has lived through all the tests. The question now is where the general relativity deviations could be.

See: Breakthrough Physics Discovery: Gravity Can Actually Create Light, Study Says
With a century's worth of research, scientists have been gifted with the Λ-Cold Dark Matter (ΛCDM) model. The symbol Λ refers to the cosmological constant of Einstein or a similar dark energy, which was introduced to explain cosmic expansion and acceleration. Though the model was found to fit cosmological data, it was found to be unsatisfactory and incomplete from a theoretical stance.

The model has also seen various observational tensions throughout the past five years. The constant of the Hubble, which notes the scale of distance and age across the Universe, can be gauged in the early Universe via cosmic microwave background. It can also be assessed in the late Universe via supernovae.

Both measurements offer results that are not compatible. The ΛCDM components also largely remain mysterious.

From an observational perspective, the most convincing reason for modified gravity would be the Universe's acceleration. The ΛCDM model postulates dark energy that is remarkably exotic and that has negative pressure that permeates through the Universe. However, the issue lies in the lack of physical justification of dark energy. The proposed dark energy alternative is the Λ cosmological constant, which calculations show should be huge. However, the constant Λ should be fine tuned into a small value for it to align with cosmic observations.

The idea of troubles surfacing from wrongly fitting cosmological data into the theory is an idea that has been gaining great popularity. This comes as the camp for dark energy stays vigorous.

This can be told by how the deviations of Einstein's theory are constrained by experiments in the solar systems.

Literature pertaining to alternative gravity theories are widely present and have shown dramatic growth. In the last decades, theorists have been trying to see the physical consequences that result from other theories.

Recent gravitational wave detections have offered an approach to manage the physical class modifications that were allowed by Einstein gravity. However, there is a need to conduct further work and research.

See: https://www.sciencetimes.com/articles/47123/20231115/einstein-wrong-theory-gravity-shortcomings-explaining-universe.htm
Einstein's Theory Of General Relativity has been under assault for the better part of a century. No one can really prove it wrong but it's commonly assumed to be wrong.

Sergei Kopeikin, associate professor of physics and astronomy at University of Missouri-Columbia, has spent the last five years defending Einstein's prediction that gravity moves at the speed of light - they want to prove Einstein right and they say they can measure the speed of propagation of tiny ripples of space-time known as gravitational waves.

He says his paper, "Gravimagnetism, causality, and aberration of gravity in the gravitational light-ray deflection experiments" published along with Edward Fomalont from the National Radio Astronomical Observatory, arrives at a consensus in the continuing debate that has divided the scientific community.

The experiment conducted by Kopeikin and Edward Fomalont five years ago found that the gravity force of Jupiter and light travel at the same speed, which validates Einstein's suggestion that gravity and electromagnetic field properties, are governed by the same principle of special relativity with a single fundamental speed.

In observing the gravitational deflection of light caused by motion of Jupiter in space, Kopeikin concluded that mass currents cause non-stationary gravimagnetic fields to form in accordance with Einstein's point of view.

Einstein believed that in order to measure any property of gravity, one has to use test particles. “By observing the motion of the particles under influence of the gravity force, one can then extract properties of the gravitational field,” Kopeikin said. “Particles without mass – such as photons – are particularly useful because they always propagate with constant speed of light irrespectively of the reference frame used for observations.”

The property of gravity tested in the experiment with Jupiter also is called causality. Causality denotes the relationship between one event (cause) and another event (effect), which is the consequence (result) of the first. In the case of the speed of gravity experiment, the cause is the event of the gravitational perturbation of photon by Jupiter, and the effect is the event of detection of this gravitational perturbation by an observer. The two events are separated by a certain interval of time which can be measured as Jupiter moves, and compared with an independently-measured interval of time taken by photon to propagate from Jupiter to the observer. The experiment found that two intervals of time for gravity and light coincide up to 20 percent. Therefore, the gravitational field cannot act faster than light propagates.”

Other physicists argue that the Fomalont-Kopeikin experiment measured nothing else but the speed of light. “This point of view stems from the belief that the time-dependent perturbation of the gravitational field of a uniformly moving Jupiter is too small to detect,” Kopeikin said.

“However, our research article clearly demonstrates that this belief is based on insufficient mathematical exploration of the rich nature of the Einstein field equations and a misunderstanding of the physical laws of interaction of light and gravity in curved space-time.”

- University of Missouri-Columbia

See: https://www.science20.com/news_account/defending_einstein_finding_a_consensus_in_physics
Scientists used a half-century of lunar laser ranging data to confirm with 100 times greater precision that all properties of mass are equivalent. This finding significantly bolsters Einstein’s equivalence principle, a cornerstone of relativity theory.
One of the most basic assumptions of fundamental physics is that the different properties of mass – weight, inertia, and gravitation – always remain the same in relation to each other. Without this equivalence, Einstein’s theory of relativity would be contradicted and our current physics textbooks would have to be rewritten. Although all measurements to date confirm the equivalence principle, quantum theory postulates that there should be a violation. This inconsistency between Einstein’s gravitational theory and modern quantum theory is the reason why ever more precise tests of the equivalence principle are particularly important.

A team from the Center of Applied Space Technology and Microgravity (ZARM) at University of Bremen, in collaboration with the Institute of Geodesy (IfE) at Leibniz University Hannover, has now succeeded in proving with 100 times greater accuracy

How close the measured value conforms to the correct value.

Inertial mass resists acceleration. For example, it causes you to be pushed backward into your seat when the car starts. Passive gravitational mass reacts on gravity and results in our weight on Earth. Active gravitational mass refers to the force of gravitation exerted by an object, or more precisely, the size of its gravitational field. The equivalence of these properties is fundamental to general relativity. Therefore, both the equivalence of inertial and passive gravitational mass and the equivalence of passive and active gravitational mass are being tested with increasing precision.

https://scitechdaily.com/images/Vishwa-Vijay-Singh-400x400.jpgFirst Author of the Publication, Vishwa Vijay Singh. Credit: Singh
What was the study about?
If we assume that passive and active gravitational mass are not equal – that their ratio depends on the material – then objects made of different materials with a different center of mass would accelerate themselves. Since the Moon consists of an aluminum shell and an iron core, with centers of mass offset against each other, the Moon should accelerate. This hypothetical change in speed could be measured with high precision, via “Lunar Laser Ranging.” This involves pointing lasers from Earth at reflectors on the Moon placed there by the Apollo missions and the Soviet Luna program. Since then, round trip travel times of laser beams are recorded. The research team analyzed “Lunar Laser Ranging” data collected over a period of 50 years, from 1970 to 2022, and investigated such mass difference effects. Since no effect was found, this means that the passive and active gravitational masses are equal to approximately 14 decimal places. This estimate is a hundred times more accurate than the best previous study, dating back to 1986.

LUH’s Institute of Geodesy – one of only four centers worldwide analyzing laser distance measurements to the Moon – has unique expertise in assessing the data, particularly for testing general relativity. In the current study, the institute analyzed the Lunar Laser Ranging measurements, including error analysis and interpretation of the results.

Vishwa Vijay Singh, Jürgen Müller and Liliane Biskupek from the Institute of Geodesy at Leibniz University Hannover, as well as Eva Hackmann and Claus Lämmerzahl from the Center of Applied Space Technology and Microgravity (ZARM) at the University of Bremen published their findings in the journal Physical Review Letters, where the paper was highlighted in the category “editors’ suggestion.”

Reference: “Equivalence of Active and Passive Gravitational Mass Tested with Lunar Laser Ranging” by Vishwa Vijay Singh, Jürgen Müller, Liliane Biskupek, Eva Hackmann and Claus Lämmerzahl, 13 July 2023, Physical Review Letters.
DOI: 10.1103/PhysRevLett.131.021401
See: https://scitechdaily.com/gravity-still-holds-einsteins-relativity-theory-stands-strong-after-quantum-challenge/
Albert Einstein published his full theory of general relativity in 1915, followed by a flurry of research papers by Einstein and others exploring the predictions of the theory. In general relativity (GR), concentrations of mass and energy curve the structure of spacetime, affecting the motion of anything passing near — including light. The theory explained the anomalous orbit of Mercury, but the first major triumph came in 1919 when Arthur Eddington and his colleagues measured the influence of the Sun’s gravity on light from stars during a total solar eclipse.

Physicists made many exotic predictions using general relativity. The bending of light around the Sun is small, but researchers realized the effect would be much larger for galaxies, to the point where gravity would form images of more distant objects — the phenomenon now called gravitational lensing. GR also predicted the existence of black holes: objects with gravity so intense that nothing getting too close can escape again, not even light.

General relativity showed that gravitation has a speed, which is the same as the speed of light. Catastrophic events like collisions between black holes or neutron stars produce gravitational waves. Researchers finally detected these waves in 2015 using the Laser Interferometer Gravitational Observatory (LIGO), a sensitive laboratory that took decades to develop.

For many aspects of astronomy — the motion of planets around stars, the structure of galaxies, etc. — researchers don’t need to use general relativity. However, in places where gravity is strong, and to describe the structure of the universe itself, GR is necessary. For that reason, researchers continue to use GR and probe its limits.
Black holes are extremely common in the universe. Stellar-mass black holes, the remnants of massive stars that exploded, are sometimes the source of powerful X-ray emissions when they are in binary systems with stars. In addition, nearly every galaxy harbors a supermassive black hole at its center, some of which produce powerful jets of matter visible from across the universe. GR is essential to understanding how these objects become so bright, as well as studying how black holes form and grow. The Event Horizon Telescope (EHT) is a world-spanning array of observatories that captured the first image of a supermassive black hole, providing a new arena for testing GR’s predictions.
Gravitational waves are a new branch of astronomy, providing a complementary way to study astrophysical systems to the standard light-based observations. Researchers use GR to provide “templates” of many possible gravitational wave signals, which is how they identify the source and its properties. Gravitational wave astronomy combines with light-based astronomy to characterize some of the most extreme events in the cosmos: collisions of black holes and neutron stars.
Astronomers use gravitational lensing to locate some of the earliest galaxies in the universe, which are too faint to be seen without the magnification provided by gravity. In addition, the distortion created by lensing allows researchers to study dark matter, and map the structure of the universe on the largest scales.
Not long after Einstein published GR, researchers realized the theory predicts that the universe changes in time. Observations in the 1920s found that prediction was true: the universe is expanding, with galaxies moving away from each other. Using GR, cosmologists found the cosmos had a beginning, and was once hotter and denser than it is today. GR provides the mathematical framework for describing the structure and evolution of the universe from its beginnings 13.8 billion years ago, and into the future.See: https://pweb.cfa.harvard.edu/research/science-field/einsteins-theory-gravitation
General relativity explains how the universe can obey physical laws that apply to any form of motion. It’s at the heart of identifying and investigating key questions about space and time, existence and reality. Its implications are not limited to esoteric concerns on cosmic scales — it has its down-to-Earth impacts as well. Without general relativity, for instance, GPS devices would be worthless. Satellite signals designed to keep your car on the right road would be off by miles if not corrected for the effects predicted by Einstein’s math.

Special relativity showed that the laws of nature don’t depend on how you are moving, as long as it’s uniform motion — constant speed in a straight line. But in real life, objects and people move in all sorts of nonuniform ways. Even some “simple” motions, like the rotation of a sphere or orbit of a planet, are nonuniform, as they constantly change direction and are therefore accelerating. Einstein wanted to extend relativity to all forms of accelerated motions. But he didn’t know how.

Today, Einstein’s cosmological constant has been revived. Rather than preventing the universe from collapse, the vacuum energy it describes can explain why the universe now expands at an accelerating pace. General relativity, cosmological constant and all, today forms the core science for analyzing the history of the universe and forecasting its future.

After Einstein died in 1955, general relativity came to life. About that time Wheeler, at Princeton University, began a program to explore its implications and train students to pursue them. By the early 1960s, new astronomical phenomena demanded explanations that Newtonian physics could not provide, and general relativity was poised for its renaissance. In the decades that followed, general relativity proved crucial for describing all sorts of celestial phenomena. At the same time, physicists devised ever more precise tests of its predictions, and Einstein passed them all. As Will has noted, “It is remarkable that this theory, born 100 years ago out of almost pure thought, has managed to survive every test.”

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