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Gravitational Waves - History, Causes, Types, Effects, LIGO, Interferometer, Significance And More

Last Updated on Oct 30, 2023
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Gravitational waves are the strength of gravity's waves produced by accelerating masses in an orbital binary system. These waves propagate outward from their source at the speed of light. Oliver Heaviside proposed gravitational waves in 1893, and Henri Poincaré suggested their existence in 1905, comparing them to electromagnetic waves but with a gravitational nature. The speed of gravitational waves is 186,000 miles per second.

Gravitational Waves are one of the most important topics for the UPSC IAS Examination. It covers a significant part of the Science & Technology subject of the General Studies Paper-3 syllabus and current events of national importance in UPSC prelims. 

In this article, we will discuss Gravitational Waves, the causes of their origin, how to detect such waves, the effects of Gravitational Waves, What LIGO is, India’s contribution to this path-breaking discovery, and what is the difference between Gravitational Waves and Gravity waves.

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What are Gravitational Waves?

Gravitational waves are distortions in space-time resulting from powerful and energetic events in the Universe. Albert Einstein first theorized the existence of gravitational waves in 1916 as part of his general theory of relativity. According to Einstein's Mathematics, massive accelerating objects, such as neutron stars or black holes orbiting each other, would generate waves of undulating space-time, propagating in all directions from the source. These cosmic ripples travel at the speed of light and carry information about their origins, providing insights into the nature of gravity itself.

History of Gravitational Waves

  • In the late 19th and early 20th centuries, Oliver Heaviside and Henri Poincaré proposed the existence of gravitational waves.
  • In 1916, Albert Einstein published his theory of general relativity. This predicted the existence of gravitational waves.
  • In 1936, Einstein and Nathan Rosen published a paper claiming that gravitational waves could not exist. However, this paper was later shown to be incorrect.
  • In 1974, Russell Hulse and Joseph Taylor discovered the first indirect evidence for the existence of gravitational waves. This was from the observed orbital decay of the Hulse–Taylor binary pulsar.
  • In 2015, the LIGO gravitational wave detectors made the first direct observation of gravitational waves from the merger of two black holes.

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Causes of Gravitational Waves

When objects travel at very high speeds, they produce the greatest strength. Several possibilities that could result in a gravitational wave include:

  • When a star erupts unevenly, it is called a supernova.
  • When two massive stars orbit one another
  • Whenever two black holes collide and fuse

However, the gravitational wave-producing objects of this type are far distant. Occasionally, these occurrences merely produce insignificant gravitational waves. When the waves finally reach Earth, they are incredibly weak. Due to this, gravitational waves are challenging to find.

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Importance of Gravitational Waves
  • Gravity waves are important because they open a new window into the cosmos. 
  • They can be used to study objects that are too faint or too distant to be seen with telescopes. 
  • They could help us understand the early moments of the universe. 
  • Gravity waves can also be used to test Einstein's theory of general relativity. They disprove Newton's theory of gravity and prove Einstein's theory of relativity.
  • They contributed to the discovery of the gravitational wave spectrum.
  • They could lead to the discovery of new devices and technologies.

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Types of Gravitational Waves
  • Continuous Gravitational Waves: These waves are produced by rotating asymmetric objects like neutron stars, and their frequency remains steady over time.
  • Compact Binary Inspirals: These waves occur when two compact objects, such as black holes or neutron stars, spiral closer together and eventually merge. It emits a characteristic chirp-like signal.
  • Burst Gravitational Waves: These waves are caused by sudden and violent events, like supernovae or cosmic collisions, producing short bursts of gravitational radiation.
  • Stochastic Gravitational Waves: These waves are background noise generated by numerous unresolved astrophysical sources and can be detected collectively but not individually.
  • Primordial Gravitational Waves: These waves originate from the early universe during inflation and can carry valuable information about the universe's early moments.

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How are Gravitational Waves detected?
  • In 2015, researchers used the Laser Interferometer Gravitational-Wave Observatory (LIGO), a discrete tool, to detect the first gravitational wave.
  •  When two black holes collided, the first gravitational waves were produced.
  • A 1.3 billion-year-old accident had occurred, and the ripples didn’t reach Earth until 2015.
  • A gravitational wave contracts and enlarges space as it passes through the Earth.
  • LIGO and two of the LIGO’s arms can detect this contracting and expansion, each measuring more than 4 km (2 miles).
  • It costs a billion dollars and includes two observatories in the shape of an L. One is in Washington State, and the other is in Louisiana.
  • The arms are moving gravitational waves, and their length varies very slightly.
  • The LIGO employs mirrors, lasers, and tiny detectors to find these minute modifications.
  • It wasn’t until 2015 that these waves were discovered on Earth, and it is one of the most important discoveries in modern physics.

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Effects of Gravitational Waves passing
  • Because a passing gravitational wave will interact with every particle it touches, it is more complex to identify the impacts of a gravitational wave.
  • In contrast to electromagnetics, uncharged particles can be used as a reference point to measure the relative velocity of charged particles.
  • It is consequently very difficult to designate a reference particle to measure gravitational waves.
  • Compared to radio waves and charged particles, gravitational waves barely interact with matter.
  • For instance, a supernova explosion within our galaxy would produce a lot of gravitational raiding. Yet, a 1-kilometre ring would only deform to the extent of an atomic nucleus’ size.
  • As of this, gravitational wave detection has proven to be incredibly difficult. However, modern detectors have already attained this sensitivity, and more advancements are planned.

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Contribution of the Indian Scientific Community
  • Over the past two decades, the Indian scientific community has achieved important advances in gravitational-wave physics.
  • The theoretical calculations needed to represent gravitational-wave signals from circling black holes were developed by Indians.
  • The Bangalore team is led by B.R. Iyer (At the International Centre for Theoretical Sciences (ICTS)-TIFR) in collaboration with French researchers.
  • Under the auspices of the Indian Initiative in Gravitational-Wave Observations (IndIGO), Indian scientists from different institutions participated in the LIGO.
  • The gravitational-wave physics group INDIGO comprises researchers from India and was founded in Maharashtra’s Hingoli district.
  • These are Chennai Mathematical Institute, ICTS-TIFR Bangalore, IISER and IITs, Institute for Plasma Research Gandhinagar, IUCAA Pune, Raja Ramanna Centre for Advanced Technology Indore, and TIFR Mumbai.
  • Estimates of the black hole’s mass, spin, energy, and peak power were all made possible by the direct efforts of the ICTS-TIFR group.
  • The team has also contributed to the astrophysics analysis of the merger of two black holes.
  • One of the general relativity tests that demonstrated the current observation is perfectly consistent with a binary black hole collision in Einstein’s theory was planned and carried out by the ICTS-TIFR group.
  • The Inter-University Centre for Astronomy and Astrophysics (IUCAA) team in Pune worked on developing the data-analysis methods needed to find these weak signals.

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What is LIGO?

LIGO stands for Laser Interferometer Gravitational-Wave Observatory (LIGO). It is a remarkable gravitational wave observatory, showcasing meticulous engineering and being the largest of its kind globally. The primary objective is to utilize gravitational-wave observations for astronomical research.

Interferometer and LIGO

  • Interferometers are investigative instruments used in a wide range of scientific and technical disciplines.
  • As they combine two or more light sources to produce an interference pattern that can be monitored and analyzed, they are also known as interferometers.
  • Interferometers produce interference patterns that reveal details about the object or activity being researched.
  • They are frequently utilized to take incredibly small measurements that are impossible to take in any other manner.
  • The LIGO interferometers are so effective at detecting gravitational waves that they can measure a distance that is 1/10,000th the width of a proton.
  •  LIGO interferometers have an L-shape. and the mirrors at the ends of the arms reflect light to produce fringes, which are interference patterns.

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Difference between Gravitational Waves and Gravity waves

Gravitational waves are rippling effects of cosmic occurrences in space-time. The merging of two enormous black holes 1.3 billion light-years away shocked LIGO since it was an unlikely event. Gravity waves, on the other hand, are much less explosive. They are produced by atmospheric and gravitational interactions rather than catastrophic cosmic events.

Let us see the difference between Gravitational Waves and Gravity waves in the table below;

Differences

Gravity Waves

Gravitational waves

Fundamental Nature

These are mechanical waves

These are not mechanical waves

Speed

The maximal speed may be around 100 ms-1, albeit speed varies.

Has a speed equal to that of light.

Medium for propagation

Given that they are mechanical waves, they don’t require a medium for transmission. They develop in fluids and spread there as well.

Since these waves are not mechanical waves, they do not require a medium for propagation.

Explanation Via

These waves can be explained using fluid dynamics.

These waves are expected to exist and form according to general relativity theory.

Energy Associated

These waves move energy across the material world.

These waves move energy through empty space or matter.

Detection

While some types of gravity waves, like ocean tides, can be observed with the naked eye, there are other types that can be identified and mapped using satellite data or other tools.

With the aid of signals captured by LIGO, physicists were able to identify gravitational waves on September 14, 2015, for the first time.

Importance of Detection

This wave detection is crucial for weather forecasting and catastrophe preparedness.

These waves, according to physicists, can break through any cosmic barrier and unveil the secrets of the cosmos.

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Significance of the Discovery
  • Space-time around other bodies, including the Earth, can be distorted by gravitational waves.
  • It might be possible for us to “see” the formation of stars and black holes if we could properly detect the waves.
  • We could comprehend the universe’s origins, creation, and many of its most enigmatic features.
  • The discovery of gravitational waves also provides further evidence for the existence of black holes.
  • The discovery will pave the way for countless other discoveries.
  • The latest discovery supports one of Einstein’s most bizarre hypotheses, made as part of his general theory of relativity 100 years ago.

Conclusion

Many things about the evolution of our universe can be learned through the detection of gravitational waves. It provides details on the cosmological objects’ motion. We can observe further into the past of the universe due to gravitational waves. It benefits the development of Einstein’s theory of relativity. These waves assist in locating the source of dark matter and brand-new celestial objects. It offers a wealth of information for astronomers and scientists looking to discover new wonders.

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Gravitational Waves - FAQs

Gravitational Waves are an invisible ripple in space that moves at the speed of light. As they pass, these waves compress and stretch everything in their path. These waves are produced when two objects are in a planar orbit.

Several possibilities are: When a star erupts in an uneven manner which is called a supernova. Or when two massive stars orbit one another or whenever two black holes collide and fuse, there are chances that gravitational waves are formed.

Compared to the compression you experience when you jump up and land on the ground,. Like ripples on a pond, gravitational waves become weaker as they move farther. So, humans cannot feel the gravitational waves.

Even after a gravitational wave has passed, the gravitational potential changes due to the energy it carries, and this change in potential causes space-time to change. Thus, Gravitational waves affect time.

Gravitational waves are rippling effects of cosmic occurrences in space-time. Whereas, Gravity waves are much less explosive. They are produced by atmospheric and gravitational interactions rather than catastrophic cosmic events.

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