“The distinction between the past, present and future is only a stubbornly persistent illusion” ― Albert Einstein

Universe: A Dream reigning in the veins

Thursday, 11 April 2019

First ever Image of a Black Hole captured by Astronomers: Finally Karl Schwarzschild's super idea has a visible form.

   
First Image of a Black Hole captured by Event Horizon Telescope
First Image of a Black Hole captured by Event Horizon Telescope


A dark core surrounded by a flame-orange halo of hot gas and plasma: thats what the first ever image of a black hole (BH) looked like when it was captured by the astronomers for the first time today on 10th April, 2019.  There was a great build up to the event during the last few days when a lot of speculations were floating in the air. Different types of opinions were given on this by different people. Some believed, some did not. It was finally announced during a simultaneous press conference in Brussels, Shanghai, Tokyo, Washington, Santiago and Taipei. The image is of a super-massive BH 50 million lightyears away in a galaxy named M87.

Black holes are star devouring monsters scattered throughout the universe. It is a highly compact object having immense gravitational pull such that even light cannot escape its gravity. According to American physicist John Archibald Wheeler "A black hole is a point in space where matter is so compressed so as to create a gravity field from where even light (with so much energy) cannot escape". These are formed as a final state of gravitational collapse of massive stars. This is the reason why it is very difficult to capture the image of a BH.

In fact the image that was recorded actually captured the surrounding mass (white hot gas and plasma) that it collected in an accretion procedure forming a luminous disc called the accretion disc. It did not record the interior of the black hole. In that sense it could only record the black hole shadow and not the black hole itself.


The image was recorded by the Event Horizon telescope installed specifically for this purpose.  Now it is the turn of Sagittarius A*, the black hole at the centre of our own galaxy, Milky way. Compared to M87, Sagittarius A* is just 26000 lightyears from Earth and is the next target of the Event Horizon telescope. Given its relatively shorter distance from Earth it is assumed that we will receive images of greater precision and clarity. In fact according to the reports the images already received from Sagittarius A* were blurred and lacked clarity due to its high activity. 

During the last two weeks eight telescopes positioned at Hawaii, Arizona, Spain, Mexico, Chile and the south pole zeroed in on M87 and Sagittarius A*. It was like a system of telescopes knit together to form a giant virtual observatory around 12000 kilometers across the globe. This image has been analyzed in six different studies by around 200 experts from 60 different institutions all over the world and was published in Astrophysical Journal Letters on 10th April, 2019.

There are obviously various technical procedures that had to be undertaken in this project. Actually what the telescopes recorded were astrophysical data which were simulated into the image of the black hole. In fact four different groups independently undertook this work of getting the image from the data and all the four finally produced the same image. The event marked the dream come true for many famous astrophysicists who never thought that they will be able to see the image of a black hole in their lifetime. 

Finally its another test passed by Einstein's General Relativity. This along with the discovery of Gravitational waves are the major advances in astronomy that we have made in the present decade and more importantly both upholds the flag of General Relativity.
Today is a time for celebration for astrophysicists and black hole lovers all over the world. Finally Karl Schwarzschild's super idea has a visible form.


Image Courtesy:  NASA

By Prabir Rudra
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Thursday, 4 April 2019

The Amazing Journey of E=mc2 : The Most Famous Equation of the World



More than a hundred years back a deceptively simple formula revealed a hidden unity buried deep in the fabric of the Universe. It connects energy with matter and the speed of light and was discovered by none other than the genius of Albert Einstein in 1905. When we think about E=mc2, we have this vision of an old white haired Einstein. But E=mc2 is not about an old Einstein. It is about a young, energetic and dynamic Einstein whose curiosity knew no bounds. 




The most famous equation of the World
The most famous equation of the World

Albert Einstein


                                                                          A young Albert Einstein


The half inch equation may seem to be so simple at the first look, but it is just a deception. Einstein in a stunning insight united the works of many who have come before him, scientists who fought and even died to form each sides of the equation. This is a story of those people who fought for the truth in spite of resistance and finally unveiled the secrets of nature. The story started long before Einstein with the discovery of E.


E is for Energy

London, England, early nineteenth century:

At that time scientists thought in terms of ‘Force’, ‘Pressure’, etc. They never had any idea about ‘Energy’ which could bring all these quantities under a single umbrella. Nobody knew that a lonely man’s quest for knowledge was going change the direction of science forever.

Michael Faraday was the son of a blacksmith who was lucky to work for a book binder as an apprentice. He never had the opportunity to acquire any elementary education. But he had an unending thirst for knowledge. He read all the books that reached him in the book binder’s shop. He wanted to escape from trade which he found vicious and selfish and wanted to become a servant of science, which he thought makes its pursuers amiable and liberal. He was determined to break free from his daily toil. 



Michael Faraday
19th century scientists were real celebrities of their time and getting a ticket to their lectures was very tough. Moreover at that time science was supposed to be a commodity of the so called gentleman, which Faraday was not. He got lucky when one of his customers got impressed with him and gave him a ticket to a lecture of the great chemist Sir Humphry Davy. Faraday never knew that this was going to change his life forever. 


Humphry Davy


                                                     Sir Humphry Davy



He was highly impressed with Davy’s lecture and became his ardent follower. His real opportunity came when Davy met with an accident while working in his laboratory, which severely damaged one of his eyes. In such a crisis, Davy appointed Faraday as one of his laboratory assistant. This opened the doors of knowledge to Faraday and he eagerly absorbed all that Davy deigned to impart. But who would have ever thought that in time the pupil would surpass the master.

Battery was newly invented at that time and as a result electricity was the order of the day. It was recorded by various scientists including Davy that a magnetic compass placed in the vicinity of a current carrying wire showed deflections.  How could electricity have any connection with magnetism, which were thought to be totally separate subjects at that time!!! Everybody was surprised and nobody could give any explanation to the observed phenomenon. Faraday speculated that perhaps some sort of electrical force is emanating outwards from the wire which was responsible for moving the magnet. This came as a shock to the scientific society nearly 300 years back because the prevailing concept at that time was that electricity flows through a wire and not sideways or out of it.

Electricity creating magnetism


Electricity creating magnetism






Lines of Forces
But Faraday was determined to reach the heart of the problem and unveil the truth. In a great leap of imagination he turned the problem in its head. Instead of an electrified wire moving a magnetic compass he wanted to know whether a static magnet could move a wire. This became the experiment of the century: The invention of the Electric motor. Although he did not understand at that time, he invented a new kind of physics. He had actually invented an over-arching principle. The chemicals in the battery had been transformed into electricity in the wire which would combine with a magnet to produce motion of the wire. Behind all these various forces there was a common ENERGY.




The set up of Electric Motor


The set up of Electric Motor

The achievements of the son of a blacksmith was opposed by many including his own master Davy. Davy was the elected president of the Royal society of London at that time. He accused Faraday of plagiarism (which was proved wrong)  and asked Faraday to put down his application seeking to be a member of the society. Faraday refused to do so and was soon elected a member of the Royal society on basis of his contributions to science. Davy died 5 years later, a victim of his many gaseous (specially laughing gas, N2O) inhalations. He was truly a great scientist of his time and had a few inventions to his name, but history will record his greatest invention as Michael Faraday.

With the passage of time Faraday’s world of invisible forces would lead to a whole new understanding of energy. He had actually shown that electricity and magnetism were not different entities (as it was thought to be at that time) but are forces that can be clubbed together into what is known as Electro-magnetism. He had started what Einstein would call the great revolution of unification.

Electromagnetic fields

Electromagnetic fields


M is for Mass

Paris, France, late eighteenth century:


King Louis XV was at the throne of France. But this was the era when the ancient absolute power of the monarchy was starting to be challenged by the common men. The French Revolution was lurking in the corner. It was the era of enlightenment which reflected that the development of humanity lies in science.

Antoine Lavoisier was an aristocratic wealthy young man who had a passion for science. He was not a scientist by profession. He was actually the head of tax enforcements in Paris. Lavoisier had an idea of building a great wall around the city and to tax every commodity that came in or went out through the wall. These political and economic activities enabled him to fund his scientific research. 

Antoine Lavoisier

Antoine Lavoisier



He was obsessed with matter and wanted to study and classify all its types. He had a great ambition to demonstrate that nature is a closed system: that in any transformation no amount of matter (mass) is ever gained or lost. He conducted an experiment where he heated water and produced its constituent hydrogen and oxygen gases. Then he combined the gases and got back water again. In the whole process he demonstrated that the total initial mass of the reactants was equal to the total final mass of all the products and successfully showed that no amount of matter was gained or lost during the transformation. 




Lavoisier's Experiment


Lavoisier's Experiment
To confirm this he conducted numerable other experiments which demanded accuracy. For this he had to commission very sensitive expensive apparatus which became possible only because of his position as a tax collector.  He became obsessed with accuracy. His experiments showed that forms of matter may change with transformations like solid, liquid or gas. Wood may become ash and smoke, metals may rust, solids may become liquid, but matter, the tiny atoms that make up all substances are never lost. This eventually laid the foundations of the law of conservation of mass.

On the other hand his methods of tax exactions was making the poor common people very angry. With the explosion of the French Revolution aristocrats like Lavoisier started losing their heads at the guillotine. After all, he was the despised tax collector who was always seen as an enemy of the common people. He was accused of tax fraud and adulteration of tobacco. Finally Lavoisier was denounced by a failed scientist turned radical journalist Jean-Paul Marat (whose scientific findings was once rejected by Lavoisier due to lack of proper scientific evidence) and was executed in front of the public at the guillotine on 8th May, 1794.


French Revolution
French Revolution
guillotine


Guillotine

Lavoisier was a great chemist of his time and is aptly known as the father of modern chemistry. His greatest accomplishment lies in changing science from a qualitative to a quantitative one. His findings with mass is central to the discovery of E= mc2.


C is for the speed of light


C stands for ‘Celeretas’ (latin word for swiftness). Since light travels with an incredible speed of 670 million miles per hour it was always considered as something which will be beyond the realm of human understanding. It was almost 100 years after Lavoisier that the world witnessed a young and energetic Einstein attending classes in the Zurich polytechnic, Switzerland. He was never an ideal student for his teachers. All he cared for in this world were Physics, Mathematics, Philosophy and his violin. All other things made absolutely no sense to him.

By that time everything that physically existed have been classified into two groups. One is matter, the building blocks of the universe and the other one is Energy, which excites matter. But nobody ever thought of any connection between the two entities. It was Einstein’s relentless pursuit of light that will bring about a revolution in science. With light he would re-invent the universe and find a hidden pathway that will unite energy and matter.

By the time Einstein arrived to the scene the speed of light have already been computed, but nobody actually knew what it was. One man whom we have already met was ready to make an educative guess on this. Michael Faraday became Professor Faraday after the death of Sir Humphry Davy. He became popular as a scientist and was known for his great experimentations. His concepts of invisible lines of forces that gave rise to electro-magnetism was still difficult for the people to digest. Now he was ready with another outrageous proposal. He proposed that light is actually one form of these vibrating lines of electro-magnetism. But as it happens everytime with science, nobody believed in him.

For 15 years Faraday struggled to convince the people that light was actually an electromagnetic wave but what he lacked was the knowledge of advanced mathematics that will back up his idea. Eventually a man by the name of James Clerk Maxwell came to his rescue. Maxwell not only believed in Faraday’s visions but also had the mathematical skills to prove Faraday right.



James Clerk Maxwell

James Clerk Maxwell
Maxwell in his calculations showed that the interlinking between electricity and magnetism can only happen at a particular speed, 670 million miles per hour. It was the speed of light. He had proved Faraday right. Electricity and magnetism woven together as electro-magnetism in its visible form was nothing but light itself.

Einstein with his never ending pursuit of light was slowly and unknowingly moving towards the link that would connect Energy with matter. He was studying rigorously the electro-magnetic theory of light that Maxwell had already proven. But one last mathematical ingredient that Einstein would need was the everyday process of squaring.




2 is for squared

Chateau Cirey, France, Early eighteenth century


For this we have go back more than a hundred years back, even before Lavoisier. At that time there was no idea how to quantify motion. All that existed was Galileo’s works and Isaac Newton’s Principia. Nobody ever thought that a crucial contribution to this subject will come from a very unusual source.

At that time King Louis XIV was at the throne of France. One of his courtyards had a daughter by the name of Emily Du Chatelet. She was a very intelligent young woman having an inclination towards science. In her tragic and short life she had a great impact on physics. She published many works of scientific research including a translation of Newton’s Principia in french which is still the standard text in France. She did all these at a time when science was considered to be a male commodity. She was ahead of any other woman of her time or even anyone upto hundred years later.

Emily Du Chatelet


                                                      Emily Du Chatelet





She was married to a general in the French army at the age nineteen and had three children. She ran a busy household and simultaneously pursued her passion for science. Emily took lessons from one of the greatest mathematicians of that time Pierre de Maupertuis, who was expert on Newton. She also had an affair with Voltaire, who was France’s greatest poet and a fierce critic of the king and the church. 



Voltaire was in prison twice and was exiled to England where he learned a lot about Newton. When he came back to France, he again got into problems with the king. At that time Emily hid him in her country home in Chateau. Far from Paris Emily and Voltaire turned her house into a centre of learning and culture along with the support of her husband (who mostly remained away busy with his duties at the army). 


Voltaire


 Voltaire




Newton stated that the the energy (force with which masses collide) is very simply mass of the object times its velocity. On the other hand a German scientist, Gottfried Wilhelm Leibniz had a different view to this. He believed that a moving object has a kind of inner spirit (which he called ‘vis viva’, latin word for living force). In his theory Leibniz was convinced that the energy of a moving body must be its mass times its velocity squared

But defying Newton and convincing the people against Newton’s theory in those days was almost an impossible task. This was where Emily came into the picture. She was highly convinced that Leibniz’s theory was correct, but the support for Newton was overwhelming. What she needed was proof in favour of Leibniz. 

Gottfried Wilhelm Leibniz

Gottfried Wilhelm Leibniz 

Finally she came across the experiments of a Dutch scientist, Willem’s Gravesande which showed that the observations indeed favour Leibniz. Gravesande’s experiment comprised of simply dropping lead balls into a pan of clay from a certain calculated height. 

His experiments showed that when we double the speed of the drop by increasing the height then the ball goes four times more deep into the clay rather than twice, thus giving evidence in favour of squaring the speed. Emily published the result in her famous book ‘Institutions De Physique’.  It is quite understandable that the work was not at all acceptable for the academy at that time.

All her life Emily tried to rise above the limitations placed on her gender. In the end it was an affair with a young soldier that brought about her demise. She conceived at an advanced age of forty-three which was considered to be dangerous in the 18th century. Finally she died six days after giving birth to her fourth child. 

Emily Du Chatelet’s conviction in the idea that the energy of an object is the function of the square of its velocity sent shockwaves through the academic society. It took hundred years after her death for the idea to be completely accepted, probably just in time for Einstein.


Einstein and his BIG idea 


By the time Einstein arrived in the scene it was all set for him to provide the final thrust towards framing the equation. All the quantities of the equation were already developed by the people who came before him. The timing was so perfect for him that it seemed to be God’s wish. Now all he had to do was to find a way to unify the physical quantities to produce the equation.

Einstein was not the so called good obedient student in the class as it was stated earlier. He had the least interest in attending classes which he said was boring. All he was interested in was light. As a result of this his professors in Zurich polytechnic did not like him at all and neither did they give him any recommendations for an academic position. He married his classmate Mileva Maric and had a child. 

Bern, Switzerland, 1905: 


After passing out of the Zurich Polytechnic in 1900, Einstein had to take a low paying job as a clerk in a patent office in Bern, Switzerland in order to run his house. After completing his daily work he had enough time at the office to think about science. He was relentlessly pursuing his question of light which he had now been thinking for ten years. Light became his obsession. His wife started complaining because his low wage made it difficult to run the house. His friends advised him to find a better job so that he could provide more comfort to his family. But Einstein had no effect of these on him. He wanted to know how God created the universe.

In a stunning insight he turned everything upside down. He changed the way how people thought about the universe. In Einstein’s universe one true constant was the speed of light and the other quantities can be bent so as to match the constant speed. In his amazing world neither space nor time were absolute quantities. This idea produced his paper on the Special Theory of Relativity

Some time earlier that same year he had already published his paper on Photoelectric effect which later won him the Nobel prize. He had also published a work on the structure of atom that same year (known as his miracle year). But he was not done yet. In one last great 1905 paper he would propose an even deeper unity. As his ten year journey with light was drawing to an end he noticed another strange connection between energy, mass and light.

He finds out that energy and mass are not at all separate entities but different forms of the same thing. As a result they can be converted into one another. Mass can be transformed into energy and vice versa. In fact all the matter that we see around us are huge reservoirs of nothing but energy. These masses are formed by the condensation of huge amounts of energy. So when these are annihilated, they give rise to huge amount of energy. With this clear idea in his mind Einstein calculated his way through to the most famous equation of the world, E=mc2. 

With four familiar notes in the scale of nature this patent clerk had composed a totally fresh melody- the culmination of his ten year journey into light. Irrespective of how far we reach in our scientific quest in the time to come, Einstein and his E=mc2 will keep whispering through the ages.


By Prabir Rudra






























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Sunday, 31 March 2019

Launch of PSLV-C45/EMISAT Mission (ISRO) on April 1, 2019 at 9.30 hours (IST) from Sriharikota, India



The Indian Space Research Organization (ISRO) is all set to launch the Polar Satellite Launch vehicle (PSLV) C45 on 1st April, 2019. The launch will take place from the rocket port at Sriharikota, Andhra Pradesh at 9.30 hours. The event will be live telecasted on Doordarshan and webcasted on the ISRO website from 9.00 hours. This mission from the Indian space agency is going to be the first of its nature because the satellites is going to be placed in three different orbits.

The PSLV-C45 rocket is going to carry a total of 29 satellites in it. Out of these there are 28 international satellites and 1 indian satellite. Out of the 28 international satellites 2 are from Lithuania, 1 each from Switzerland and Spain and 24 from United States. The most important satellite that the rocket will carry is india's electronic intelligence satellite (EMISAT), which weighs around 436 kgs. This satellite will help the Defence Research and Development Organization (DRDO) in research and development.

The triple orbit launch will take around 3 hours and weather conditions does play a big role int this. In fact, the launch was supposed to take place on 21st March, 2019 which was postponed to 1st April, 2019. The countdown has already begun. Its going to be yet another achievement for the Indian space agency. Watch it live on Doordarshan or ISRO website from 9 hours onwards.

Rocket Satellite Launch
Rocket Launch


By Prabir Rudra
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Thursday, 21 March 2019

LIGO will come back online on 1st April, 2019 after a big upgrade



LIGO (Laser Interferometer Gravitational wave observatory) is a facility that was responsible for the first Gravitational wave detection back in February, 2016. Gravitational waves are ripples in the fabric of space-time caused by highly explosive events like black hole mergers, collision of stellar remnants (white dwarfs, neutron stars, etc.), supernova, etc. Einstein predicted this almost 100 years back as a possible test of his theory of General Relativity. The 2017 Nobel prize in Physics went to three distinguished scientists Kip Thorne, Barry Barish and Rainer Weiss for their ground breaking work in designing and setting up LIGO

There are two set-ups one located at Hanford, Washington and the other at Livingstone, Louisiana. Last year both the facilities of LIGO was taken down so that its detectors could undergo some serious hardware upgrades. 

The set-ups basically consists of two perpendicular concrete pipes joined in the shape of a giant 'L' each extending to around two miles (3.2 kilometres). Inside these these pipes two powerful Laser beams are bounced off a series of mirrors. Since the two pipes are of the same length the two beams remain in phase with each other. But whenever a gravitational wave passes through the facility it extends one of the pipes and contracts the other one thus creating a difference in length. This distortion in space gets the beams off balance and they become out of phase. This is what is measured with extreme precision. 

Till date 11 such events have been recorded by the facilities. Out of these, 10 events were due to merging of black holes and 1 event arose from the collision of two neutron stars.

LIGO has recently announced that these upgrades are almost complete and the observatories will be up and working from 1st April, 2019. We hope that better technology will give us better observations and we will soon make serious breakthrough into gravitational wave astronomy.


LIGO facility, Virgo
LIGO facility


For more on LIGO visit  https://www.ligo.caltech.edu/




Image courtesy:  https://www.ligo.caltech.edu/images

By Prabir Rudra

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Live webcast of the super worm moon and the vernal Equinox



Slooh.com is an online observatory that is going to live webcast the Super worm moon and the vernal equinox today (20th March, 2019) at 2 p.m. EDT (1800 GMT) . The observations will be conducted via the Canary island telescopes. Two Slooh Astronomers Paul Cox and Dr. Paige Godfrey will discuss the dynamics involved between Earth and Sun during an Equinox. You can watch it directly at  https://www.slooh.com/shows/event-details/621



Equinox


By Prabir Rudra
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Thursday, 14 March 2019

Relativity for All Contd.!! (The General theory of Relativity)



On the 140th birth anniversary of Albert Einstein it is our great pleasure to revisit one of his greatest masterpiece, the General theory of Relativity (GR) (arguably the best theory of Einstein). Today we discuss GR in his memory and ponder over the extraordinary genius of the man who redefined Physics in the 20th century.

Albert Einstein
Albert Einstein


Background



After his miraculous year in 1905, when he laid the foundation of 4 groundbreaking theories of nature (Photoelectric effect, Brownian motion, special theory of relativity and “the world’s most famous equation, E= mc2”), Einstein came to the limelight. 

World’s most famous equation
World’s most famous equation


From a patent clerk in Bern, Switzerland Einstein became a lecturer in the University of Bern in 1908. The following year he was appointed as an associate professor of theoretical physics in the university of Zurich. Einstein became a full professor in the Charles-Ferdinand university in Prague in April, 1911. In 1912 he returned to Zurich as a professor of theoretical physics in ETH, Zurich. He decided to move to Germany and on 1st April, 1914, he joined the Berlin University.



During all these switch overs from one institute to the other Einstein kept nourishing his original idea of generalizing the theory of relativity that he proposed back in 1905. It was as situation of crisis to humanity. First world war was about to break out. But all these seemed to have minimal effect on the genius. A sense of incompleteness kept haunting him through days and nights.

General theory of Relativity


                                       The Problem 


If we recall our last discussion of Special theory of Relativity we will note that the theory was valid only for inertial (non-accelerated) frames of references. But in reality almost all frames are accelerated . A moving car needs to accelerate or de-accelerate. Similarly a cyclist has to use brakes while cycling. A football rolling on the ground de-accelerates due to friction. All these are non-inertial (accelerated) frames of references where special theory of relativity is not applicable. 

So we need a general theory of relativity that will be applicable to all frames of references (both inertial and non-inertial frames).



Why a theory of Gravity?


In the attempt to generalize his theory of relativity, Einstein knew that he has to incorporate acceleration in his theory. Now acceleration comes from force. In a great insight Einstein understood two things which he stated as the Principle of Equivalence.

1)  The equivalence of inertial and gravitational mass.    

2)  The gravitational force experienced locally while standing on a massive body like Earth is the same as the pseudo force experienced by an observer in a non-inertial frame of reference.


He had the feeling that this can really be a theory of gravity. He started to consider the problem of gravity seriously. He consulted Max Planck (who laid the foundations of Quantum mechanics in 1900) and told him about his intentions to work out the gravity problem. 

The legend says that Planck told him “There are two possibilities: (1) The gravity problem is so difficult that probably you will never succeed.  (2) Even if you are able to find a solution to the problem nobody will believe you.”




Max Planck

Max Planck

The weak link of the prevailing Newton’s theory of Gravitation


The first comprehensive theory of gravitation was stated by Isaac Newton in the 17th century. It stated that:

Any two masses separated by a certain distance will attract each other by a force directly proportional to the product of the masses and inversely proportional to the square of the distance between them.



The theory seemed to be fine at that time with no flaws and was universally accepted. Newton became the God and very few people had the guts to question his intellect. Moreover the problem of gravity was very difficult to address and so only a few showed any further interest and believed in Newton.

Isaac Newton
Isaac Newton


But some natural questions arise:

What is the source or the origin of the force?

What is creating it?

Why is it present at all?

Newton was silent to these questions. He did not have any logical answer to it. 

The Theory that answered the above questions


Einstein’s theory of General Relativity is a geometric theory of gravitation that answered the prevailing questions of the critics.

Einstein argued that space-time (space and time together) is like a stretched fabric.  Now when we put a mass on such a fabric naturally it will create a curvature around itself. This is warping (curving, bending or twisting) of space-time that gives rise to a gravity well around the mass. Now when a second mass comes within the curvature quite naturally it moves towards the first body due to the gravity well produced. 


Curvature in space-time
Curvature in space-time




Einstein argued this is what gravitation is!! It is not a force at all as Newton had proposed almost 250 years back. It is a phenomenon that is created by the geometry or curvature of the space-time.


Curvature in space-time
Greater the mass greater the curvature on the space-time fabric




What a masterstroke indeed!! What a beautiful insight!! The common mind can only bewilder and get lost in its aura!! Such was the extraordinary genius of a curious mind.   

The Race to Glory


Einstein had developed the physics of the theory back in 1912, but he did not have any clue about the Mathematics. He needed sufficient knowledge about the geometry of curved space-time (Non-Euclidean geometry) before he could proceed towards developing any meaningful mathematics of the theory. 


Einstein was far from being an expert in such a geometry. But one man by the name of David Hilbert was. He was a mathematical giant of that era. Hilbert took up the problem and started developing the mathematics, which came as a terror to Einstein. His theory was in danger of being credited to somebody else. He had to act and act fast.

David Hilbert
David Hilbert


Einstein’s friend Marcel Grossmann (a great mathematician) came to his rescue. With his help Einstein learnt the concepts of Riemannian (Non-Euclidean) geometry and started developing the mathematics of his theory. Hilbert on the other hand continued his effort silently but swiftly. 

As the race to glory became more and more intense the scientific community watched the battle of the two scientific giants (one physicist, the other mathematician) and waited eagerly for a result.


By the grace of God, it so happened that both these great minds reached their destination independently and almost simultaneously. By 1915 both had their own versions of the mathematics of GR ready. On careful scrutiny it was found that both were correct.

Hilbert accepted that the contributions to the theory was far more loaded in favour of Einstein and the theory of general relativity must go by the name of Einstein. This ended all confusions if at all there was any. Finally in 1916, Einstein published his theory of general relativity in the Annals of Physics.



It is difficult to contemplate the feelings of the great man. During his quest, at some point he must have felt that he was losing the battle. After all Hilbert was a great mathematician and matching him was a herculean task. Therefore after the publication, it could have felt like winning a battle once thought to be lost. But it should be remembered that the physical basis of the theory was solely laid by Einstein and probably that’s enough to retain the credit. 

The Equations of General Relativity

This is a relation between mass and spacetime geometry.


Equation of GR
Equation of GR



The Reaction from the scientific community


Accepting this theory was not at all easy for the scientific community. The theory will shake the very foundations of physics. Shock-waves were abundant and far reaching. Scientists had many years of scientific career jeopardized. Isaac Newton’s theory of gravitation was in danger. So it happened as Max Planck had predicted some years back. Everybody demanded a proof for the theory.

The radical nature of the theory was criticized by many great minds. Some even thought that GR is not a theory of physics, but the whims and fantasies of Einstein, who is living in a fantasy world.

Experimental physicists like Philipp Lenard (Nobel Laureate, 1905) went into direct confrontations with Einstein and mocked him publicly. He said that physics is a subject of experiments and observations. We believe what we see. There is no place for dreamers like Einstein in the scientific community. Science got really ugly!!



Einstein retaliated but he understood that he had to give a proof to save his theory from being demolished by the critics (specially nazi).

The Proof of General Relativity


The paper was published. The theory was complete. But it didn’t matter to anybody because nobody believed it. Now the genius of Einstein faced a bigger challenge. How will he provide a proof for the theory for which he fought for over a decade. Moreover he was not an expert in experimentation at all. It was an uphill task for him.

But again his extraordinary genius came out with an extraordinary idea. He proposed the bending of starlight around the solar limb (gravitational lensing) as a possible proof for general relativity. 

He argued that the light from the distant stars that pass by the sun before reaching us on Earth will bend while their journey near the sun. The sun being a massive mass will create a huge curvature in the space-time around it. The starlight while passing by the sun will follow this curvature and get bent. As a result multiple images of the star will be formed in the sky. This is in complete compliance with general relativity.



So if Einstein’s theory is correct starlight will bend around the sun and if it is not then the light will pass unaffected. Einstein requested the astronomers all over the world to go and check it.

Many astronomers including Arthur Eddington, a renowned British astronomer took up the challenge. Watching the faint starlight in the presence of powerful sunlight was always going to be difficult. So they chose total solar eclipse for their observations.

In 1919, Eddington’s observations of a total solar eclipse provided concrete proofs in favour of Einstein’s general theory of relativity. 


A British proof to a German theory provided a thrust towards world peace in the post first world war era. Einstein dreamt of a peaceful world without any wars. Even his greatest scientific theory advocated his humane feelings.

In 1921, Einstein was awarded the Nobel prize, not for his general theory of relativity, but for his discovery of the photoelectric effect (may be to his disappointment).

General theory of relativity has been termed as ‘the most beautiful theory of physics’ ever. Till date it remains arguably the best theory of nature not to win a Nobel prize.

Einstein receives 1921 Nobel prize for physics



I am not a genius. I am just curious...I ask many questions and when the answer is simple, then God is answering.     

         --Albert Einstein.


By Prabir Rudra




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