
Erwin Schrodinger, the man behind the famous cat experiment that questioned reality
Until you look, the cat exists in a strange twilight: both alive and dead.advertisementIt is absurd, morbid, and yet -- utterly central to one of the most important debates in science.Outside the box, Erwin Schrodinger was not looking for a pet rescue mission but making a point: in the strange realm of quantum mechanics, reality itself may be undecided until you check.This was no cruel animal experiment in a lab. And Schrodinger never trapped a real cat. It was a thought experiment, dreamt up in 1935, in a Europe bracing for war and in a scientific community still grappling with the bizarre new rules of quantum theory.The image of Schrodinger's cat was so sharp, so unsettling, that it leapt from physics papers into cultural legend.To understand why a man would conjure such a morbid mental picture, you have to rewind to Vienna in the early 20th century. There lived a curious boy who would one day challenge how the universe itself is understood.FROM GIFTED CHILD TO WAVE MECHANICSErwin Schrodinger was born on August 12, 1887, in Vienna, the only child of a father who ran a small linoleum factory and a mother from an academic family. Their cultured, upper-middle-class home was filled with books, art, and scientific curiosity.Young Erwin excelled early, mastering advanced mathematics while classmates were still wrestling with basics. The coffee-houses and lecture halls of the city fed his fascination with science and philosophy.
1927 Solvay Conference (Photo: Wikimedia Commons) Row 1: A. Piccard, E. Henriot, P. Ehrenfest, Ed. Herzen, Th. De Donder, E. Schrdinger, E. Verschaffelt, W. Pauli, W. Heisenberg, R.H. Fowler, L. Brillouin, Row 2: P. Debye, M. Knudsen, W.L. Bragg, H.A. Kramers, P.A.M. Dirac, A.H. Compton, L. de Broglie, M. Born, N. Bohr, Row 3: I. Langmuir, M. Planck, M. Curie, H.A. Lorentz, A. Einstein, P. Langevin, w:Charles-Eugne Guye, C.T.R. Wilson, O.W. Richardson
He entered the University of Vienna in 1906, studying under the likes of Friedrich Hasenohrl, and earned his doctorate in 1910 (Maths History), before the world plunged into chaos with World War 1.advertisementSchrodinger served in the Austrian army as an artillery officer in the war. Even on the front lines, he carried notebooks filled with equations. The war ended with Austria's empire in ruins, and Vienna became a place of scarcity but also intellectual ferment.THE BREAKTHROUGH THAT WON HIM THE NOBELBy the mid-1920s, quantum mechanics was in its chaotic infancy. Werner Heisenberg had proposed 'matrix mechanics', a powerful but abstract method to describe the strange behaviour of subatomic particles. But Schrodinger took a different path.In 1926, while on a skiing holiday in the Swiss Alps resort of Arosa, he worked on the wave equation that would cement his place in history -- a mathematical description of how particles behaved not as fixed points, but as 'wave functions' spreading out in space and time.This not only matched Heisenberg's results, but offered a more intuitive picture of the quantum world. It was the bridge that connected the strange predictions of quantum theory with experiments in the real world.His wave mechanics explained phenomena like the hydrogen atom's energy levels with breath-taking accuracy, and won him the 1933 Nobel Prize in Physics, shared with Paul Dirac.It was this work, and not the cat, that made him a central architect of quantum theory.
Schrodinger's Nobel Prize Diploma (Photo: Wikimedia Commons)
advertisementPOLITICS, IDEOLOGY, AND EXILESchrodinger's life was tangled up with the politics of his time. The cat came later, in a world shadowed by Nazi power.Schrodinger's politics were complex -- pacifist, humanist, and deeply opposed to totalitarianism. In 1933, as Hitler consolidated power, he resigned from his post in Berlin and left Germany, rejecting Nazi ideology.After brief academic posts in England and Austria, he eventually took up a role at the newly founded Institute for Advanced Studies in Dublin, helping shape it into a hub for theoretical physics.When he introduced the cat in a paper in 1935, Europe was already edging towards another catastrophic war.ENTER THE CAT, A QUANTUM PARADOXBy that time, Schrodinger was struggling with a puzzling idea in quantum mechanics: under Niels Bohr's Copenhagen interpretation, a particle existed in a 'superposition' or multiple states at once until someone observed it. Particles chose the state when we looked at them.advertisementTo show how bizarre that sounded when applied to normal life, he cooked up his most famous mental image:Imagine a cat locked in a boxInside the box is a device containing a single unstable atom -- the kind that can randomly 'decay,' or change into something else, at an unpredictable momentIf the atom decays, it triggers a chain reaction: a detector notices the change, releases a hammer, breaks open a vial of poison, and the cat diesIf the atom does not decay, the cat livesQuantum physics says that until we actually open the box, that atom is in a sort of limbo -- both decayed and not decayed.And if the atom is in both states, then the cat is, too: both dead and alive at the same time. Schrodinger's point wasn't that this scenario could actually happen to cats, but that the logic of quantum rules turns absurd when pulled out of the subatomic world and applied to everyday objects.The famous thought experiment was not meant to be solved; it was meant to unsettle. It was a challenge to scientists to question the Copenhagen interpretation, to probe its assumptions, and to think harder about what 'reality' really means.advertisementThe cat-in-a-box theory exposed the philosophical rift in quantum theory: Was reality determined only when observed, as the Copenhagen interpretation claimed, or was there some deeper, hidden truth?Schrodinger leaned towards the latter, uncomfortable with the idea that the universe only 'became real' when someone looked.A MIND THAT RANGED FAR BEYOND PHYSICSBeyond physics, Schrodinger strayed boldly into biology while in Ireland. His 1944 book What Is Life? suggested that the instructions for life or genetic information might be stored in a molecular 'code-script'.At the time, this was a leap of imagination, but it lit a spark in young scientists like James Watson, Francis Crick and Rosalind Franklin, who went on to reveal DNA's double helix, proving Schrodinger's hunch had been startlingly accurate.His curiosity didn't stop with science. Schrodinger, though an atheist, immersed himself in Eastern philosophy, reading deeply in Vedanta and Buddhist thought. He was drawn to their ideas of unity and interconnectedness -- that the boundaries between observer and observed are an illusion.He saw in these ideas parallels with quantum theory, and they quietly coloured his interpretation of quantum mechanics and his writings on the nature of reality. He also wrote on colour theory, and unified field theory.
Shrodinger's signature (Photo: Wikimedia Commons)
Even Schrodinger's personal life reflected his unconventional mind: while married, he also lived with a second partner -- a situation that baffled polite society but was tolerated in the academic circles he moved in.Returning to Vienna in 1956 after years abroad, he continued working until his death in 1961. He was buried in the small Austrian village of Alpbach. On his tombstone, instead of a cat, there's an engraving of the wave equation that changed physics forever.Today, his name echoes not only in physics textbooks but in quantum computer labs, philosophical debates, and the pages of science fiction.And that paradoxical cat -- imagined, never harmed -- still prowls the world's imagination, a reminder that reality may be stranger than we think, and never fully revealed until we observe.- Ends
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India Today
a day ago
- India Today
Erwin Schrodinger, the man behind the famous cat experiment that questioned reality
A cat is in a sealed box. It is both alive and dead, at least until you open the the sealed chamber also sits a vial of vial could be triggered to break by a tiny amount of radioactive material that may (or may not) release energy and change form over time. Until you look, the cat exists in a strange twilight: both alive and is absurd, morbid, and yet -- utterly central to one of the most important debates in the box, Erwin Schrodinger was not looking for a pet rescue mission but making a point: in the strange realm of quantum mechanics, reality itself may be undecided until you was no cruel animal experiment in a lab. And Schrodinger never trapped a real cat. It was a thought experiment, dreamt up in 1935, in a Europe bracing for war and in a scientific community still grappling with the bizarre new rules of quantum image of Schrodinger's cat was so sharp, so unsettling, that it leapt from physics papers into cultural understand why a man would conjure such a morbid mental picture, you have to rewind to Vienna in the early 20th century. There lived a curious boy who would one day challenge how the universe itself is GIFTED CHILD TO WAVE MECHANICSErwin Schrodinger was born on August 12, 1887, in Vienna, the only child of a father who ran a small linoleum factory and a mother from an academic family. Their cultured, upper-middle-class home was filled with books, art, and scientific Erwin excelled early, mastering advanced mathematics while classmates were still wrestling with basics. The coffee-houses and lecture halls of the city fed his fascination with science and philosophy. 1927 Solvay Conference (Photo: Wikimedia Commons) Row 1: A. Piccard, E. Henriot, P. Ehrenfest, Ed. Herzen, Th. De Donder, E. Schrdinger, E. Verschaffelt, W. Pauli, W. Heisenberg, R.H. Fowler, L. Brillouin, Row 2: P. Debye, M. Knudsen, W.L. Bragg, H.A. Kramers, P.A.M. Dirac, A.H. Compton, L. de Broglie, M. Born, N. Bohr, Row 3: I. Langmuir, M. Planck, M. Curie, H.A. Lorentz, A. Einstein, P. Langevin, w:Charles-Eugne Guye, C.T.R. Wilson, O.W. Richardson He entered the University of Vienna in 1906, studying under the likes of Friedrich Hasenohrl, and earned his doctorate in 1910 (Maths History), before the world plunged into chaos with World War served in the Austrian army as an artillery officer in the war. Even on the front lines, he carried notebooks filled with equations. The war ended with Austria's empire in ruins, and Vienna became a place of scarcity but also intellectual BREAKTHROUGH THAT WON HIM THE NOBELBy the mid-1920s, quantum mechanics was in its chaotic infancy. Werner Heisenberg had proposed 'matrix mechanics', a powerful but abstract method to describe the strange behaviour of subatomic particles. But Schrodinger took a different 1926, while on a skiing holiday in the Swiss Alps resort of Arosa, he worked on the wave equation that would cement his place in history -- a mathematical description of how particles behaved not as fixed points, but as 'wave functions' spreading out in space and not only matched Heisenberg's results, but offered a more intuitive picture of the quantum world. It was the bridge that connected the strange predictions of quantum theory with experiments in the real wave mechanics explained phenomena like the hydrogen atom's energy levels with breath-taking accuracy, and won him the 1933 Nobel Prize in Physics, shared with Paul was this work, and not the cat, that made him a central architect of quantum theory. Schrodinger's Nobel Prize Diploma (Photo: Wikimedia Commons) advertisementPOLITICS, IDEOLOGY, AND EXILESchrodinger's life was tangled up with the politics of his time. The cat came later, in a world shadowed by Nazi politics were complex -- pacifist, humanist, and deeply opposed to totalitarianism. In 1933, as Hitler consolidated power, he resigned from his post in Berlin and left Germany, rejecting Nazi brief academic posts in England and Austria, he eventually took up a role at the newly founded Institute for Advanced Studies in Dublin, helping shape it into a hub for theoretical he introduced the cat in a paper in 1935, Europe was already edging towards another catastrophic THE CAT, A QUANTUM PARADOXBy that time, Schrodinger was struggling with a puzzling idea in quantum mechanics: under Niels Bohr's Copenhagen interpretation, a particle existed in a 'superposition' or multiple states at once until someone observed it. Particles chose the state when we looked at show how bizarre that sounded when applied to normal life, he cooked up his most famous mental image:Imagine a cat locked in a boxInside the box is a device containing a single unstable atom -- the kind that can randomly 'decay,' or change into something else, at an unpredictable momentIf the atom decays, it triggers a chain reaction: a detector notices the change, releases a hammer, breaks open a vial of poison, and the cat diesIf the atom does not decay, the cat livesQuantum physics says that until we actually open the box, that atom is in a sort of limbo -- both decayed and not if the atom is in both states, then the cat is, too: both dead and alive at the same time. Schrodinger's point wasn't that this scenario could actually happen to cats, but that the logic of quantum rules turns absurd when pulled out of the subatomic world and applied to everyday famous thought experiment was not meant to be solved; it was meant to unsettle. It was a challenge to scientists to question the Copenhagen interpretation, to probe its assumptions, and to think harder about what 'reality' really cat-in-a-box theory exposed the philosophical rift in quantum theory: Was reality determined only when observed, as the Copenhagen interpretation claimed, or was there some deeper, hidden truth?Schrodinger leaned towards the latter, uncomfortable with the idea that the universe only 'became real' when someone looked.A MIND THAT RANGED FAR BEYOND PHYSICSBeyond physics, Schrodinger strayed boldly into biology while in Ireland. His 1944 book What Is Life? suggested that the instructions for life or genetic information might be stored in a molecular 'code-script'.At the time, this was a leap of imagination, but it lit a spark in young scientists like James Watson, Francis Crick and Rosalind Franklin, who went on to reveal DNA's double helix, proving Schrodinger's hunch had been startlingly curiosity didn't stop with science. Schrodinger, though an atheist, immersed himself in Eastern philosophy, reading deeply in Vedanta and Buddhist thought. He was drawn to their ideas of unity and interconnectedness -- that the boundaries between observer and observed are an saw in these ideas parallels with quantum theory, and they quietly coloured his interpretation of quantum mechanics and his writings on the nature of reality. He also wrote on colour theory, and unified field theory. Shrodinger's signature (Photo: Wikimedia Commons) Even Schrodinger's personal life reflected his unconventional mind: while married, he also lived with a second partner -- a situation that baffled polite society but was tolerated in the academic circles he moved to Vienna in 1956 after years abroad, he continued working until his death in 1961. He was buried in the small Austrian village of Alpbach. On his tombstone, instead of a cat, there's an engraving of the wave equation that changed physics his name echoes not only in physics textbooks but in quantum computer labs, philosophical debates, and the pages of science that paradoxical cat -- imagined, never harmed -- still prowls the world's imagination, a reminder that reality may be stranger than we think, and never fully revealed until we observe.- Ends


Time of India
4 days ago
- Time of India
Seven superclouds: Giant gas neighbours of our solar system discovered
Source: ScienceNews In a stunning breakthrough, astronomers have discovered seven massive structures of gas known as superclouds just beyond our solar system. These immense clouds, stretching thousands of light-years across, are likely the birthplaces of stars and may have formed from material stripped from the spiral arms of the Milky Way . While two of them, including the well-known Radcliffe Wave, had been identified earlier, five are brand new discoveries. Lying nearly parallel to each other and undulating in wave-like patterns, these superclouds are our largest local neighbours in space and are rewriting what we know about interstellar structure and star formation . A hidden interstellar structure revealed by modern mapping Thanks to advanced space mapping using data from the Gaia spacecraft, a team of astronomers led by Lilly Kormann from the University of Vienna has charted a detailed 3D map of interstellar dust and hydrogen within 50 million square light-years around the Sun. What they initially saw were patches of high-density dust, but a closer analysis revealed that many of these dense zones were linked together in long, coherent structures. By connecting the dots, the team identified seven vast superclouds, including the Radcliffe Wave and a previously known one called the Split, lying close to the solar system in an almost parallel arrangement. Colossal dimensions and mass by Taboola by Taboola Sponsored Links Sponsored Links Promoted Links Promoted Links You May Like Jamaica: New Container Houses (Prices May Surprise You) Container House | Search Ads Undo Each of the seven superclouds stretches between 3,000 and 8,000 light-years in length and holds gas weighing 800,000 to 3.5 million times the mass of the Sun. These massive forms are not only among the largest known local structures in our galaxy, but researchers believe they might be even larger than measured, as parts likely extend beyond the edges of the current dust map. Positioned along the Milky Way's disc, these superclouds form a sort of galactic framework that may shape the way stars and star systems, including ours, are created and distributed across space. Star nurseries within the superclouds What makes this discovery especially important is that most known stellar nurseries, regions where new stars are born, are located inside these superclouds, particularly along their central spines. This pattern strongly suggests that superclouds play a foundational role in star formation, acting as the 'mothers' to smaller, denser gas clouds that collapse under gravity to form stars. Scientists now believe these superclouds represent an early stage in the hierarchy of star-making, offering insight into how vast structures break down into smaller ones, eventually producing stars, solar systems, and perhaps even planets like Earth. The mystery of the waves Most of the superclouds show a distinct wave-like form, rising and falling in an undulating pattern above and below the flat disc of the Milky Way. Only one, the Split, remains relatively straight. The fact that so many of these gas clouds zigzag in unison suggests there's a common physical mechanism shaping them, possibly linked to galactic gravity, spiral arm dynamics, or even external galactic forces. Even more intriguing is how their average densities remain strikingly similar, despite differences in the amount of material packed into each section. This hints at a larger, still-unknown system regulating their structure and behaviour. What this means for astronomy This discovery marks a turning point in our understanding of the local interstellar medium , the cloud-like environment that surrounds our solar system. As astrophysicist Bruce Elmegreen put it, we are only now beginning to "see what is very local to us," after decades of struggling to separate nearby structures from distant background noise. The identification of these seven superclouds gives scientists a valuable new framework to study star formation, interstellar physics, and the evolution of our galaxy on a large scale. It also opens new questions about what other structures might still be hidden in the cosmic dust. Also read | New Hubble photo shows cotton candy-like nebula in a nearby dwarf galaxy
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First Post
6 days ago
- First Post
Did you know that the Eiffel Tower gets bigger in the summer? Here's why
The Eiffel Tower, erected during the 1889 World's Fair, expands up to 15 cm in the summer due to thermal expansion of iron. This natural process can lead it to grow taller and lean away from the sun read more As temperatures rise during the summer months, the Eiffel Tower grows even taller than its original design. File image/AP The structure known today as the Eiffel Tower was originally dubbed the Tour de 300 mètres, the 300-metre tower. The name was proposed by engineers Maurice Koechlin and Émile Nougier to Gustave Eiffel, who oversaw the tower's construction. It hinted at the desire to build something extraordinary, a technological feat that would set a new height record. However, as temperatures rise during the summer months, the Eiffel Tower grows even taller than its original design. STORY CONTINUES BELOW THIS AD A lightweight iron structure The Eiffel Tower was erected at the 1889 World's Fair to commemorate the centenary of the French Revolution. Eiffel chose puddled iron for its construction, a material he knew well and had used in previous projects with good results. This ferrous material can withstand high levels of stress, which allowed for the construction of a large, very light tower that would be safe from horizontal wind forces. To give an idea of how light the tower is, its weight of 7,300 tonnes is close to the weight of the volume of air contained within it – around 6,300 tonnes. The Eiffel Tower was intended to be a prime observation point, as well as a base for radio broadcasting. The tower itself is a gigantic triangular lattice structure, much like the Garabit Viaduct (also designed by Eiffel's office) and the Forth Bridge in Scotland, both from the same period. All of these structures grow when the temperature of the material increases. However, unlike bridges, which behave in a more complex manner, the Eiffel Tower experiences mainly vertical growth and shrinkage due to changes in temperature. This phenomenon is known as thermal expansion. Materials that grow and shrink We know that most solids expand when the temperature rises and contract when it falls. This is because an increase in temperature causes greater agitation in the atoms, which leads to an increase in the average distance between them. Depending on the nature of the bond, different kinds of solids experience greater or lesser growth, which engineers have to record with great care. Ceramics and glasses, with stronger bonds, expand less than metals, which in turn expand less than polymers. The Eiffel Tower under construction. Wikimedia Commons So, how can we estimate the amount of movement in a solid? When the elements are straight – as is the case in most public works and architecture, where beams and bars predominate – the movement is proportional to three parameters: the length of the element, the change in its temperature, and the material's coefficient of expansion. STORY CONTINUES BELOW THIS AD A hair's breadth Many ceramic materials typically have expansion coefficients ranging from 0.5x10⁻⁶ to 1.5x10⁻⁶ (degree Celsius) ⁻¹, while metals range between 5x10⁻⁶ and 30x10⁻⁶ (degree Celsius)⁻¹, and polymers between 50x10⁻⁶ and 300x10⁻⁶ (degree Celsius)⁻¹. These (perhaps strange-looking) numbers indicate the growth of a standard-length unit when the temperature rises by one degree Celsius. The most expandable materials are polymers, which expand about ten times more than metals, and metals expand ten times more than ceramics. The puddled iron used in the Eiffel Tower, and its steel components, have a coefficient of around 12x10⁻⁶ (degree Celsius)⁻¹, meaning that a one-metre-long iron bar expands by 12x10⁻⁶ metres when the temperature rises by one degree. That is just a dozen microns, less than the thickness of a human hair. So does heat have any noticeable effect on buildings? Yes, if we take into account that there are two other parameters to consider: the length of the element and the temperature range where it is located. The length can be very great. The Eiffel Tower is 300 m high, but the Garabit Viaduct is 565m long, and the Forth Bridge is over 2.5km long. Today, there are many larger linear structures, and thermal expansion also affects the railway tracks that many bridges are built to carry. STORY CONTINUES BELOW THIS AD Historical temperature ranges must also be analysed. Paris has been recording temperatures for more than two centuries, with winter minimums below -20 degrees Celsius and summer maximums of around 40 degrees Celsius. We should also take into account the effect of solar radiation – metals can reach much higher temperatures in direct sunlight, often exceeding 60 degrees Celsius or 70 degrees Celsius. Leaning away from the sun Now, let's do the maths. We'll estimate how much a simple 100-metre-long metal bar expands when the temperature fluctuates by 100 degrees Celsius – the approximate range experienced by the Eiffel Tower. The calculation is simple. If a one-metre bar expands by 0.000012 metres when the temperature rises by one degree, a 100-metre bar expands by 0.12 metres when the temperature rises by 100 degrees. And a 300-metre bar would expand three times as much: 0.36 metres. That is, 36 cm. This is a noticeable difference. The most expandable materials are polymers, which expand about ten times more than metals, and metals expand ten times more than ceramics. AP Clearly, a simple bar does not behave the same as a tower made of more than 18,000 pieces of riveted iron oriented in all directions. Furthermore, the sun always shines on one of its sides. This means one of its faces grows more than the others, causing a slight curve in the tower, as if it were leaning away from the sun. STORY CONTINUES BELOW THIS AD Specialists have estimated that the Eiffel Tower actually grows between 12 and 15 centimetres when comparing its size on cold winter days with the hottest days of summer. This means that, in addition to being a landmark, a communications tower and a symbol of Paris itself, the Eiffel Tower is also, in effect, a giant thermometer. Federico de Isidro Gordejuela, Profesor adjunto de Construcciones Arquitectónicas, Universidad CEU San Pablo This article is republished from The Conversation under a Creative Commons license. Read the original article.