India’s first particle physics observatory is to be constructed in the district of Theni in Tamil Nadu at an expense of Rs. 1,200 crore (USD 250 million). Called the India-based Neutrino Observatory (INO), the entire experiment will be situated 1.3 km under a hill to keep other radiations and cosmic rays from interfering with the study. This is because the neutrinos that the detector will be studying rarely interact with matter and pass through it at the rate of three or four interactions per nearly 85 trillion trillion trillion. The gouging of a tunnel 7m wide and 1.9km long for accessing the cavern that will house the systems was commenced on October 14, Friday, and is expected to take a year.
Twenty-seven days ago, a startling discovery set off tremors across the scientific community when the Gran Sasso National Laboratory inItalyreported that certain fundamental particles called neutrinos had been observed moving faster than light. The reason this observation caused such dissonance and a flurry of excitement is that, according to the physics megagiant Albert Einstein, the Universe would allow nothing to travel faster than light.
Then again, conclusive proof was not presented by the physicists at the lab—at least, not anything that was within the infamous six-sigma accuracy tolerance limit: 99.99999 per cent. It was little surprise, then, that within a week of the report, engineers were working in full-swing atJapan's Kamioka reactor, at theUSA's dreaded Fermilab, at the Sudbury Neutrino Observatory inCanada, to recreate the conditions at Gran Sasso. Far away, in India, a country that had until then been the principle centre for processing second-hand information, a 22-year old plan was finally being mobilized.
With just a 29-year old history, the energy frontier of physics research was supposed to last at least until 2018—the year of the Super Large Hadron Collider. With such unprecedented discoveries, however, a shift away from high-energy research and toward ultra-rare processes has become conspicuous. For the INO, the timing couldn’t have been better.
The decision to locate the observatory at Theni was finalized after evaluating the local topography, seismic stability, environmental disturbance, rock quality, availability of electricity and water, and rain patterns. In order to further minimize the impact of the project’s logistical and infrastructural operations, an extant but little-used road is being re-laid for the trucks and earthmovers to use, instead of having them move through five villages.
Funded by the government of India and the Tata Institute of Fundamental Research (TIFR), and coordinated by the Institute of Mathematical Sciences (IMS), the INO will host a supersensitive static detector called the Iron Calorimeter (ICAL), incorporating a magnet exactly four times as large as the one in use at the Large Hadron Collider. Such an effort will involve the INO-industry interface in a big way, drawing heavily on available industrial infrastructure, in issues related to mechanical structure, electronics and detector-related technology.
The detector will consist of a stack of alternating plates of iron and borosilicate glass, each totally numbering 30,000 and measuring 12m to a side. The glass plates, in turn, will consist of glass sheets with a noble gas sandwiched in between—an arrangement referred to collectively as a resistive plate chamber (RPC). When a neutrino interacts with iron, it will knock out an electron from its orbit around an atom and send it into the RPC. Once there, the electron will be picked up by positively charged electrodes sewn into the glass, translated into a signal, and sent to the data processors.
The source of the neutrinos will be the sun, supernovae, cosmic rays and other intergalactic phenomena, and the output will correspond to the particle’s mass, position of interaction, velocity, type, degree of oscillation and charge.
There are two reasons the INO stands out from its peers: the first is that the ICAL is going to be devoted to studying neutrinos and neutrinos only, and the second is that the ICAL will study them continuously without stopping (except for scheduled maintenance). Because of such principled and technical dedication, physicists expect the detector to shine light on some of the more elusive characteristics of neutrinos, such as flavour oscillations and neutrino-neutrino interactions.
These are boom times for Indian science. The national spending on science and technology has gone up in the last five years and is inching towards two per cent ofIndia's GDP. Hordes of new institutes are coming up in the nook and corner of the country—30 new central universities, 5 new Indian Institutes of Science Education and Research, 8 new Indian Institutes of Technology and 20 new Indian Institutes of Information Technology are in various stages of conception and completion.
However, simply increasing the number of institutes will not lead to better scientific prowess. The education system needs a complete rethink in order to attract more students to science and produce world class scientists (the last home-grown scientist to win a Nobel Prize was Sir C. V. Raman in 1930). In this direction, the INO is a giant leap forward because of its capacity to sustain research in subjects at the energy and cosmic frontiers, because of the special and exotic experimentation environments it will support, and because of the invaluable access it will provide to the Indian scientific community to cutting-edge information.
Showing posts with label Fermilab. Show all posts
Showing posts with label Fermilab. Show all posts
Wednesday, 19 October 2011
Star of the Orient
India’s first particle physics observatory is to be constructed in the district of Theni in Tamil Nadu at an expense of Rs. 1,200 crore (USD 250 million). Called the India-based Neutrino Observatory (INO), the entire experiment will be situated 1.3 km under a hill to keep other radiations and cosmic rays from interfering with the study. This is because the neutrinos that the detector will be studying rarely interact with matter and pass through it at the rate of three or four interactions per nearly 85 trillion trillion trillion. The gouging of a tunnel 7m wide and 1.9km long for accessing the cavern that will house the systems was commenced on October 14, Friday, and is expected to take a year.
Twenty-seven days ago, a startling discovery set off tremors across the scientific community when the Gran Sasso National Laboratory inItalyreported that certain fundamental particles called neutrinos had been observed moving faster than light. The reason this observation caused such dissonance and a flurry of excitement is that, according to the physics megagiant Albert Einstein, the Universe would allow nothing to travel faster than light.
Then again, conclusive proof was not presented by the physicists at the lab—at least, not anything that was within the infamous six-sigma accuracy tolerance limit: 99.99999 per cent. It was little surprise, then, that within a week of the report, engineers were working in full-swing atJapan's Kamioka reactor, at theUSA's dreaded Fermilab, at the Sudbury Neutrino Observatory inCanada, to recreate the conditions at Gran Sasso. Far away, in India, a country that had until then been the principle centre for processing second-hand information, a 22-year old plan was finally being mobilized.
With just a 29-year old history, the energy frontier of physics research was supposed to last at least until 2018—the year of the Super Large Hadron Collider. With such unprecedented discoveries, however, a shift away from high-energy research and toward ultra-rare processes has become conspicuous. For the INO, the timing couldn’t have been better.
The decision to locate the observatory at Theni was finalized after evaluating the local topography, seismic stability, environmental disturbance, rock quality, availability of electricity and water, and rain patterns. In order to further minimize the impact of the project’s logistical and infrastructural operations, an extant but little-used road is being re-laid for the trucks and earthmovers to use, instead of having them move through five villages.
Funded by the government of India and the Tata Institute of Fundamental Research (TIFR), and coordinated by the Institute of Mathematical Sciences (IMS), the INO will host a supersensitive static detector called the Iron Calorimeter (ICAL), incorporating a magnet exactly four times as large as the one in use at the Large Hadron Collider. Such an effort will involve the INO-industry interface in a big way, drawing heavily on available industrial infrastructure, in issues related to mechanical structure, electronics and detector-related technology.
The detector will consist of a stack of alternating plates of iron and borosilicate glass, each totally numbering 30,000 and measuring 12m to a side. The glass plates, in turn, will consist of glass sheets with a noble gas sandwiched in between—an arrangement referred to collectively as a resistive plate chamber (RPC). When a neutrino interacts with iron, it will knock out an electron from its orbit around an atom and send it into the RPC. Once there, the electron will be picked up by positively charged electrodes sewn into the glass, translated into a signal, and sent to the data processors.
The source of the neutrinos will be the sun, supernovae, cosmic rays and other intergalactic phenomena, and the output will correspond to the particle’s mass, position of interaction, velocity, type, degree of oscillation and charge.
There are two reasons the INO stands out from its peers: the first is that the ICAL is going to be devoted to studying neutrinos and neutrinos only, and the second is that the ICAL will study them continuously without stopping (except for scheduled maintenance). Because of such principled and technical dedication, physicists expect the detector to shine light on some of the more elusive characteristics of neutrinos, such as flavour oscillations and neutrino-neutrino interactions.
These are boom times for Indian science. The national spending on science and technology has gone up in the last five years and is inching towards two per cent ofIndia's GDP. Hordes of new institutes are coming up in the nook and corner of the country—30 new central universities, 5 new Indian Institutes of Science Education and Research, 8 new Indian Institutes of Technology and 20 new Indian Institutes of Information Technology are in various stages of conception and completion.
However, simply increasing the number of institutes will not lead to better scientific prowess. The education system needs a complete rethink in order to attract more students to science and produce world class scientists (the last home-grown scientist to win a Nobel Prize was Sir C. V. Raman in 1930). In this direction, the INO is a giant leap forward because of its capacity to sustain research in subjects at the energy and cosmic frontiers, because of the special and exotic experimentation environments it will support, and because of the invaluable access it will provide to the Indian scientific community to cutting-edge information.
Twenty-seven days ago, a startling discovery set off tremors across the scientific community when the Gran Sasso National Laboratory inItalyreported that certain fundamental particles called neutrinos had been observed moving faster than light. The reason this observation caused such dissonance and a flurry of excitement is that, according to the physics megagiant Albert Einstein, the Universe would allow nothing to travel faster than light.
Then again, conclusive proof was not presented by the physicists at the lab—at least, not anything that was within the infamous six-sigma accuracy tolerance limit: 99.99999 per cent. It was little surprise, then, that within a week of the report, engineers were working in full-swing atJapan's Kamioka reactor, at theUSA's dreaded Fermilab, at the Sudbury Neutrino Observatory inCanada, to recreate the conditions at Gran Sasso. Far away, in India, a country that had until then been the principle centre for processing second-hand information, a 22-year old plan was finally being mobilized.
With just a 29-year old history, the energy frontier of physics research was supposed to last at least until 2018—the year of the Super Large Hadron Collider. With such unprecedented discoveries, however, a shift away from high-energy research and toward ultra-rare processes has become conspicuous. For the INO, the timing couldn’t have been better.
The decision to locate the observatory at Theni was finalized after evaluating the local topography, seismic stability, environmental disturbance, rock quality, availability of electricity and water, and rain patterns. In order to further minimize the impact of the project’s logistical and infrastructural operations, an extant but little-used road is being re-laid for the trucks and earthmovers to use, instead of having them move through five villages.
Funded by the government of India and the Tata Institute of Fundamental Research (TIFR), and coordinated by the Institute of Mathematical Sciences (IMS), the INO will host a supersensitive static detector called the Iron Calorimeter (ICAL), incorporating a magnet exactly four times as large as the one in use at the Large Hadron Collider. Such an effort will involve the INO-industry interface in a big way, drawing heavily on available industrial infrastructure, in issues related to mechanical structure, electronics and detector-related technology.
The detector will consist of a stack of alternating plates of iron and borosilicate glass, each totally numbering 30,000 and measuring 12m to a side. The glass plates, in turn, will consist of glass sheets with a noble gas sandwiched in between—an arrangement referred to collectively as a resistive plate chamber (RPC). When a neutrino interacts with iron, it will knock out an electron from its orbit around an atom and send it into the RPC. Once there, the electron will be picked up by positively charged electrodes sewn into the glass, translated into a signal, and sent to the data processors.
The source of the neutrinos will be the sun, supernovae, cosmic rays and other intergalactic phenomena, and the output will correspond to the particle’s mass, position of interaction, velocity, type, degree of oscillation and charge.
There are two reasons the INO stands out from its peers: the first is that the ICAL is going to be devoted to studying neutrinos and neutrinos only, and the second is that the ICAL will study them continuously without stopping (except for scheduled maintenance). Because of such principled and technical dedication, physicists expect the detector to shine light on some of the more elusive characteristics of neutrinos, such as flavour oscillations and neutrino-neutrino interactions.
These are boom times for Indian science. The national spending on science and technology has gone up in the last five years and is inching towards two per cent ofIndia's GDP. Hordes of new institutes are coming up in the nook and corner of the country—30 new central universities, 5 new Indian Institutes of Science Education and Research, 8 new Indian Institutes of Technology and 20 new Indian Institutes of Information Technology are in various stages of conception and completion.
However, simply increasing the number of institutes will not lead to better scientific prowess. The education system needs a complete rethink in order to attract more students to science and produce world class scientists (the last home-grown scientist to win a Nobel Prize was Sir C. V. Raman in 1930). In this direction, the INO is a giant leap forward because of its capacity to sustain research in subjects at the energy and cosmic frontiers, because of the special and exotic experimentation environments it will support, and because of the invaluable access it will provide to the Indian scientific community to cutting-edge information.
Monday, 26 September 2011
My kingdom for a neutrino
In 1982, when the construction for CERN’s Large Hadron Collider (LHC) experiment was given the go-ahead, physics entered a very exciting period. It promised them the answers to their biggest questions and, in the event that that didn’t happen, it promised them ample evidence to come to a conclusion of their own.
Two decades later, with the device in full operation, results are emerging, some more improbable than the rest. The project was put in place to attempt to create the conditions of the Big Bang so physicists could detect the Higgs boson. However, nobody anticipated such a thing as evidence of super-luminary travel by neutrinos.
The existence of neutrinos was first proposed by Austrian physicist Wolfgang Pauli in 1930 to account for the excess mass and energy left behind after a neutron disintegrated into a proton and an electron. The first direct observation was to be made only in the 1970s, more than 40 years later. The neutrino is one of the many indivisible particles of this Universe, and is of neutral charge and very little mass. In fact, amongst all the particles that have any mass, a neutrino is the lightest. This means that according to Albert Einstein’s theory of relativity, the mass of the particle will hit infinity only when it travels at speeds terribly close to that of light. And by terribly close, I’m talking 99.9999% close.
Such neutrinos were generated by the LHC over the course of some of its experiments and sent to the Gran Sasso National Laboratory in Italy for study. Located 730 km south of the LHC and almost a kilometre under Mt. Gran Sasso, the laboratory receives the particles in a massive tank of ultra-pure water.
Once a neutrino comes in contact with a proton of a water molecule, they react to form a neutron and a positron. The positron collides with an electron, its anti-particle, to annihilate each other, releasing two gamma rays. The neutron is captured by another nucleus to release a third gamma ray. Therefore, the signature of a neutrino capture is the release of three gamma rays.
[caption id="attachment_20371" align="aligncenter" width="439" caption="The Super-KamiokaNDE experiment in Japan contains a tank of 50,000 litres of water, fit with an array of tens of thousands of photo-multiplier tubes (as above) to detect the release of energy in case of a neutrino capture. The cylindrical container has other systems in place to detect the position of a capture, too."]
[/caption]
At the laboratory, as scientists waited for the neutrinos to arrive and set off the reactions, they were hardly prepared when the release of the gamma rays was detected precisely 60 nanoseconds before it was due. While such a small difference might seem trivial, the implication is that the neutrinos arrived before any other kind of electromagnetic radiation did. Since electromagnetic radiations possess the fastest speed attainable in this Universe according to Einstein, the speeding neutrinos have possibly defied the greatest physicist of the last century.
Where does that leave the world of physics?
Centuries of hypothesizing and experimenting by scientists have ingrained the importance of reasoned scepticism in their minds. While the Gran Sasso National Laboratory has claimed that 16,000 such instances have been recorded and documented, they haven’t ruled out any errors. For now, physicists the world over await similar conclusions, and so confirmations, from the two other colliders capable of replicating such conditions.
One of them is the J-PARC in Japan. Located along the coast of the Tohoku prefecture, the device was damaged and unable to operate for the next 12 months, at least, by the earthquake in March 2011 in nearby Fukushima. The other collider is the Fermilab Tevatron, an atom-smasher of considerable reputation, in the USA. After close to three decades of operation, the facility is scheduled to shut down permanently on September 30, 2011.
Collaboration rather than competition seems to be the emerging mantra. The shadow of CERN is beginning to loom large on most particle physics labs, and they’re finding it difficult to compete with CERN and its flagship project. Further, in these days of ballooning fiscal deficits and bond rating downgrades in the US, funding is hard to come by for such "creamy" projects.
Unsurprisingly, physicists are prepared to wait. Why won’t they when the speed of light – a form of electromagnetic radiation – has been the definitive cornerstone of some of the most important foundations of our understanding of this Universe? By defying that limit, neutrinos have brought upon them the scrutiny of the entire scientific community.
For one, by being faster than light, neutrinos speeding toward Earth from distant stars get here before the image of the star does, making it possible for astrophysicists to peek farther back into history. Second, the particle that carries electromagnetic energy, the photon, was thought to be massless so it wouldn’t violate the theory of relativity. However, the neutrino has mass, and that means all of Einstein’s works will have to be disrobed and studied. The larger consequence of this is that almost all high-energy installations on this planet, ranging from nuclear power plants (NPPs) that power cities to radio-telescopes searching for extra-terrestrial life, become available for changes as much as at the design level.
(In an NPP, the flow of single-phase coolants in pressurized water reactors is assumed to flow not faster than the speed of light. Even if the fluid dynamics of single-phase coolants has already been modelled on luminary principles, how could there be any changes at the design level?
If the speed of the coolants can be increased even higher, then the critical discharge, i.e., the maximum flow rate permissible, will also go higher. This translates into enhanced cooling, and this obviously means that fuel rods can be made even thicker and more power could be generated.*)
Similarly, the way the world works also is not going to change since the neutrino has always been working the same way for billions of years irrespective of how we thought it worked. But what is going to change is the way we understand electromagnetic concepts. The Standard Model of particle physics, the Big Daddy of all the theories of physics, won’t have to be tweaked so much as twisted around to accommodate this yet-unsubstantiated phenomenon.
Physicists will wait, and while they wait, they’ll debate. They’ll conduct more experiments, record more data, hypothesize more, refute more, argue more, all the while hoping that the Tevatron will be fired up for one last battle, that the J-PARC will be resuscitated for a one-of-a-kind challenge. In my opinion, no overbearing modifications will have to be made to the pool of knowledge we possess regarding physics as such. Even if the neutrinos did travel at super-luminary speeds - which I highly doubt and attribute to minute measurement errors adding up to cause the spike - it won't be long before the concept of the phenomenon is quickly subsumed by the search for other even greater truths. Yes, our perspectives are going to change, but more than anything, the discovery's original role as a tool with which to discover more about nature will not.
Let's not get carried away, though. After all, disproving the greatest minds of physics in history requires a future of its own.
Two decades later, with the device in full operation, results are emerging, some more improbable than the rest. The project was put in place to attempt to create the conditions of the Big Bang so physicists could detect the Higgs boson. However, nobody anticipated such a thing as evidence of super-luminary travel by neutrinos.
The existence of neutrinos was first proposed by Austrian physicist Wolfgang Pauli in 1930 to account for the excess mass and energy left behind after a neutron disintegrated into a proton and an electron. The first direct observation was to be made only in the 1970s, more than 40 years later. The neutrino is one of the many indivisible particles of this Universe, and is of neutral charge and very little mass. In fact, amongst all the particles that have any mass, a neutrino is the lightest. This means that according to Albert Einstein’s theory of relativity, the mass of the particle will hit infinity only when it travels at speeds terribly close to that of light. And by terribly close, I’m talking 99.9999% close.
Such neutrinos were generated by the LHC over the course of some of its experiments and sent to the Gran Sasso National Laboratory in Italy for study. Located 730 km south of the LHC and almost a kilometre under Mt. Gran Sasso, the laboratory receives the particles in a massive tank of ultra-pure water.
Once a neutrino comes in contact with a proton of a water molecule, they react to form a neutron and a positron. The positron collides with an electron, its anti-particle, to annihilate each other, releasing two gamma rays. The neutron is captured by another nucleus to release a third gamma ray. Therefore, the signature of a neutrino capture is the release of three gamma rays.
[caption id="attachment_20371" align="aligncenter" width="439" caption="The Super-KamiokaNDE experiment in Japan contains a tank of 50,000 litres of water, fit with an array of tens of thousands of photo-multiplier tubes (as above) to detect the release of energy in case of a neutrino capture. The cylindrical container has other systems in place to detect the position of a capture, too."]
[/caption]At the laboratory, as scientists waited for the neutrinos to arrive and set off the reactions, they were hardly prepared when the release of the gamma rays was detected precisely 60 nanoseconds before it was due. While such a small difference might seem trivial, the implication is that the neutrinos arrived before any other kind of electromagnetic radiation did. Since electromagnetic radiations possess the fastest speed attainable in this Universe according to Einstein, the speeding neutrinos have possibly defied the greatest physicist of the last century.
Where does that leave the world of physics?
Centuries of hypothesizing and experimenting by scientists have ingrained the importance of reasoned scepticism in their minds. While the Gran Sasso National Laboratory has claimed that 16,000 such instances have been recorded and documented, they haven’t ruled out any errors. For now, physicists the world over await similar conclusions, and so confirmations, from the two other colliders capable of replicating such conditions.
One of them is the J-PARC in Japan. Located along the coast of the Tohoku prefecture, the device was damaged and unable to operate for the next 12 months, at least, by the earthquake in March 2011 in nearby Fukushima. The other collider is the Fermilab Tevatron, an atom-smasher of considerable reputation, in the USA. After close to three decades of operation, the facility is scheduled to shut down permanently on September 30, 2011.
Collaboration rather than competition seems to be the emerging mantra. The shadow of CERN is beginning to loom large on most particle physics labs, and they’re finding it difficult to compete with CERN and its flagship project. Further, in these days of ballooning fiscal deficits and bond rating downgrades in the US, funding is hard to come by for such "creamy" projects.
Unsurprisingly, physicists are prepared to wait. Why won’t they when the speed of light – a form of electromagnetic radiation – has been the definitive cornerstone of some of the most important foundations of our understanding of this Universe? By defying that limit, neutrinos have brought upon them the scrutiny of the entire scientific community.
For one, by being faster than light, neutrinos speeding toward Earth from distant stars get here before the image of the star does, making it possible for astrophysicists to peek farther back into history. Second, the particle that carries electromagnetic energy, the photon, was thought to be massless so it wouldn’t violate the theory of relativity. However, the neutrino has mass, and that means all of Einstein’s works will have to be disrobed and studied. The larger consequence of this is that almost all high-energy installations on this planet, ranging from nuclear power plants (NPPs) that power cities to radio-telescopes searching for extra-terrestrial life, become available for changes as much as at the design level.
(In an NPP, the flow of single-phase coolants in pressurized water reactors is assumed to flow not faster than the speed of light. Even if the fluid dynamics of single-phase coolants has already been modelled on luminary principles, how could there be any changes at the design level?
If the speed of the coolants can be increased even higher, then the critical discharge, i.e., the maximum flow rate permissible, will also go higher. This translates into enhanced cooling, and this obviously means that fuel rods can be made even thicker and more power could be generated.*)
Similarly, the way the world works also is not going to change since the neutrino has always been working the same way for billions of years irrespective of how we thought it worked. But what is going to change is the way we understand electromagnetic concepts. The Standard Model of particle physics, the Big Daddy of all the theories of physics, won’t have to be tweaked so much as twisted around to accommodate this yet-unsubstantiated phenomenon.
Physicists will wait, and while they wait, they’ll debate. They’ll conduct more experiments, record more data, hypothesize more, refute more, argue more, all the while hoping that the Tevatron will be fired up for one last battle, that the J-PARC will be resuscitated for a one-of-a-kind challenge. In my opinion, no overbearing modifications will have to be made to the pool of knowledge we possess regarding physics as such. Even if the neutrinos did travel at super-luminary speeds - which I highly doubt and attribute to minute measurement errors adding up to cause the spike - it won't be long before the concept of the phenomenon is quickly subsumed by the search for other even greater truths. Yes, our perspectives are going to change, but more than anything, the discovery's original role as a tool with which to discover more about nature will not.
Let's not get carried away, though. After all, disproving the greatest minds of physics in history requires a future of its own.
*On the other hand, for example, the speed at which the gravitational force acts on any body is limited to the speed of electromagnetic radiations, but that doesn't mean discovery of a higher speed in this Universe is going to change anything. It's only a role reversal at the most (although the massiveness of the neutrino is going to make a difference) because the practically achievable velocity is going to remain the same.
My kingdom for a neutrino
In 1982, when the construction for CERN’s Large Hadron Collider (LHC) experiment was given the go-ahead, physics entered a very exciting period. It promised them the answers to their biggest questions and, in the event that that didn’t happen, it promised them ample evidence to come to a conclusion of their own.
Two decades later, with the device in full operation, results are emerging, some more improbable than the rest. The project was put in place to attempt to create the conditions of the Big Bang so physicists could detect the Higgs boson. However, nobody anticipated such a thing as evidence of super-luminary travel by neutrinos.
The existence of neutrinos was first proposed by Austrian physicist Wolfgang Pauli in 1930 to account for the excess mass and energy left behind after a neutron disintegrated into a proton and an electron. The first direct observation was to be made only in the 1970s, more than 40 years later. The neutrino is one of the many indivisible particles of this Universe, and is of neutral charge and very little mass. In fact, amongst all the particles that have any mass, a neutrino is the lightest. This means that according to Albert Einstein’s theory of relativity, the mass of the particle will hit infinity only when it travels at speeds terribly close to that of light. And by terribly close, I’m talking 99.9999% close.
Such neutrinos were generated by the LHC over the course of some of its experiments and sent to the Gran Sasso National Laboratory in Italy for study. Located 730 km south of the LHC and almost a kilometre under Mt. Gran Sasso, the laboratory receives the particles in a massive tank of ultra-pure water.
Once a neutrino comes in contact with a proton of a water molecule, they react to form a neutron and a positron. The positron collides with an electron, its anti-particle, to annihilate each other, releasing two gamma rays. The neutron is captured by another nucleus to release a third gamma ray. Therefore, the signature of a neutrino capture is the release of three gamma rays.
[caption id="attachment_20371" align="aligncenter" width="439" caption="The Super-KamiokaNDE experiment in Japan contains a tank of 50,000 litres of water, fit with an array of tens of thousands of photo-multiplier tubes (as above) to detect the release of energy in case of a neutrino capture. The cylindrical container has other systems in place to detect the position of a capture, too."][/caption]
At the laboratory, as scientists waited for the neutrinos to arrive and set off the reactions, they were hardly prepared when the release of the gamma rays was detected precisely 60 nanoseconds before it was due. While such a small difference might seem trivial, the implication is that the neutrinos arrived before any other kind of electromagnetic radiation did. Since electromagnetic radiations possess the fastest speed attainable in this Universe according to Einstein, the speeding neutrinos have possibly defied the greatest physicist of the last century.
Where does that leave the world of physics?
Centuries of hypothesizing and experimenting by scientists have ingrained the importance of reasoned scepticism in their minds. While the Gran Sasso National Laboratory has claimed that 16,000 such instances have been recorded and documented, they haven’t ruled out any errors. For now, physicists the world over await similar conclusions, and so confirmations, from the two other colliders capable of replicating such conditions.
One of them is the J-PARC in Japan. Located along the coast of the Tohoku prefecture, the device was damaged and unable to operate for the next 12 months, at least, by the earthquake in March 2011 in nearby Fukushima. The other collider is the Fermilab Tevatron, an atom-smasher of considerable reputation, in the USA. After close to three decades of operation, the facility is scheduled to shut down permanently on September 30, 2011.
Collaboration rather than competition seems to be the emerging mantra. The shadow of CERN is beginning to loom large on most particle physics labs, and they’re finding it difficult to compete with CERN and its flagship project. Further, in these days of ballooning fiscal deficits and bond rating downgrades in the US, funding is hard to come by for such "creamy" projects.
Unsurprisingly, physicists are prepared to wait. Why won’t they when the speed of light – a form of electromagnetic radiation – has been the definitive cornerstone of some of the most important foundations of our understanding of this Universe? By defying that limit, neutrinos have brought upon them the scrutiny of the entire scientific community.
For one, by being faster than light, neutrinos speeding toward Earth from distant stars get here before the image of the star does, making it possible for astrophysicists to peek farther back into history. Second, the particle that carries electromagnetic energy, the photon, was thought to be massless so it wouldn’t violate the theory of relativity. However, the neutrino has mass, and that means all of Einstein’s works will have to be disrobed and studied. The larger consequence of this is that almost all high-energy installations on this planet, ranging from nuclear power plants (NPPs) that power cities to radio-telescopes searching for extra-terrestrial life, become available for changes as much as at the design level.
(In an NPP, the flow of single-phase coolants in pressurized water reactors is assumed to flow not faster than the speed of light. Even if the fluid dynamics of single-phase coolants has already been modelled on luminary principles, how could there be any changes at the design level?
If the speed of the coolants can be increased even higher, then the critical discharge, i.e., the maximum flow rate permissible, will also go higher. This translates into enhanced cooling, and this obviously means that fuel rods can be made even thicker and more power could be generated.*)
Similarly, the way the world works also is not going to change since the neutrino has always been working the same way for billions of years irrespective of how we thought it worked. But what is going to change is the way we understand electromagnetic concepts. The Standard Model of particle physics, the Big Daddy of all the theories of physics, won’t have to be tweaked so much as twisted around to accommodate this yet-unsubstantiated phenomenon.
Physicists will wait, and while they wait, they’ll debate. They’ll conduct more experiments, record more data, hypothesize more, refute more, argue more, all the while hoping that the Tevatron will be fired up for one last battle, that the J-PARC will be resuscitated for a one-of-a-kind challenge. In my opinion, no overbearing modifications will have to be made to the pool of knowledge we possess regarding physics as such. Even if the neutrinos did travel at super-luminary speeds - which I highly doubt and attribute to minute measurement errors adding up to cause the spike - it won't be long before the concept of the phenomenon is quickly subsumed by the search for other even greater truths. Yes, our perspectives are going to change, but more than anything, the discovery's original role as a tool with which to discover more about nature will not.
Let's not get carried away, though. After all, disproving the greatest minds of physics in history requires a future of its own.
Two decades later, with the device in full operation, results are emerging, some more improbable than the rest. The project was put in place to attempt to create the conditions of the Big Bang so physicists could detect the Higgs boson. However, nobody anticipated such a thing as evidence of super-luminary travel by neutrinos.
The existence of neutrinos was first proposed by Austrian physicist Wolfgang Pauli in 1930 to account for the excess mass and energy left behind after a neutron disintegrated into a proton and an electron. The first direct observation was to be made only in the 1970s, more than 40 years later. The neutrino is one of the many indivisible particles of this Universe, and is of neutral charge and very little mass. In fact, amongst all the particles that have any mass, a neutrino is the lightest. This means that according to Albert Einstein’s theory of relativity, the mass of the particle will hit infinity only when it travels at speeds terribly close to that of light. And by terribly close, I’m talking 99.9999% close.
Such neutrinos were generated by the LHC over the course of some of its experiments and sent to the Gran Sasso National Laboratory in Italy for study. Located 730 km south of the LHC and almost a kilometre under Mt. Gran Sasso, the laboratory receives the particles in a massive tank of ultra-pure water.
Once a neutrino comes in contact with a proton of a water molecule, they react to form a neutron and a positron. The positron collides with an electron, its anti-particle, to annihilate each other, releasing two gamma rays. The neutron is captured by another nucleus to release a third gamma ray. Therefore, the signature of a neutrino capture is the release of three gamma rays.
[caption id="attachment_20371" align="aligncenter" width="439" caption="The Super-KamiokaNDE experiment in Japan contains a tank of 50,000 litres of water, fit with an array of tens of thousands of photo-multiplier tubes (as above) to detect the release of energy in case of a neutrino capture. The cylindrical container has other systems in place to detect the position of a capture, too."]
[/caption]At the laboratory, as scientists waited for the neutrinos to arrive and set off the reactions, they were hardly prepared when the release of the gamma rays was detected precisely 60 nanoseconds before it was due. While such a small difference might seem trivial, the implication is that the neutrinos arrived before any other kind of electromagnetic radiation did. Since electromagnetic radiations possess the fastest speed attainable in this Universe according to Einstein, the speeding neutrinos have possibly defied the greatest physicist of the last century.
Where does that leave the world of physics?
Centuries of hypothesizing and experimenting by scientists have ingrained the importance of reasoned scepticism in their minds. While the Gran Sasso National Laboratory has claimed that 16,000 such instances have been recorded and documented, they haven’t ruled out any errors. For now, physicists the world over await similar conclusions, and so confirmations, from the two other colliders capable of replicating such conditions.
One of them is the J-PARC in Japan. Located along the coast of the Tohoku prefecture, the device was damaged and unable to operate for the next 12 months, at least, by the earthquake in March 2011 in nearby Fukushima. The other collider is the Fermilab Tevatron, an atom-smasher of considerable reputation, in the USA. After close to three decades of operation, the facility is scheduled to shut down permanently on September 30, 2011.
Collaboration rather than competition seems to be the emerging mantra. The shadow of CERN is beginning to loom large on most particle physics labs, and they’re finding it difficult to compete with CERN and its flagship project. Further, in these days of ballooning fiscal deficits and bond rating downgrades in the US, funding is hard to come by for such "creamy" projects.
Unsurprisingly, physicists are prepared to wait. Why won’t they when the speed of light – a form of electromagnetic radiation – has been the definitive cornerstone of some of the most important foundations of our understanding of this Universe? By defying that limit, neutrinos have brought upon them the scrutiny of the entire scientific community.
For one, by being faster than light, neutrinos speeding toward Earth from distant stars get here before the image of the star does, making it possible for astrophysicists to peek farther back into history. Second, the particle that carries electromagnetic energy, the photon, was thought to be massless so it wouldn’t violate the theory of relativity. However, the neutrino has mass, and that means all of Einstein’s works will have to be disrobed and studied. The larger consequence of this is that almost all high-energy installations on this planet, ranging from nuclear power plants (NPPs) that power cities to radio-telescopes searching for extra-terrestrial life, become available for changes as much as at the design level.
(In an NPP, the flow of single-phase coolants in pressurized water reactors is assumed to flow not faster than the speed of light. Even if the fluid dynamics of single-phase coolants has already been modelled on luminary principles, how could there be any changes at the design level?
If the speed of the coolants can be increased even higher, then the critical discharge, i.e., the maximum flow rate permissible, will also go higher. This translates into enhanced cooling, and this obviously means that fuel rods can be made even thicker and more power could be generated.*)
Similarly, the way the world works also is not going to change since the neutrino has always been working the same way for billions of years irrespective of how we thought it worked. But what is going to change is the way we understand electromagnetic concepts. The Standard Model of particle physics, the Big Daddy of all the theories of physics, won’t have to be tweaked so much as twisted around to accommodate this yet-unsubstantiated phenomenon.
Physicists will wait, and while they wait, they’ll debate. They’ll conduct more experiments, record more data, hypothesize more, refute more, argue more, all the while hoping that the Tevatron will be fired up for one last battle, that the J-PARC will be resuscitated for a one-of-a-kind challenge. In my opinion, no overbearing modifications will have to be made to the pool of knowledge we possess regarding physics as such. Even if the neutrinos did travel at super-luminary speeds - which I highly doubt and attribute to minute measurement errors adding up to cause the spike - it won't be long before the concept of the phenomenon is quickly subsumed by the search for other even greater truths. Yes, our perspectives are going to change, but more than anything, the discovery's original role as a tool with which to discover more about nature will not.
Let's not get carried away, though. After all, disproving the greatest minds of physics in history requires a future of its own.
*On the other hand, for example, the speed at which the gravitational force acts on any body is limited to the speed of electromagnetic radiations, but that doesn't mean discovery of a higher speed in this Universe is going to change anything. It's only a role reversal at the most (although the massiveness of the neutrino is going to make a difference) because the practically achievable velocity is going to remain the same.
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