-Neutrino-
It's believed that modern physics nothing can travel faster than the speed of light. The astonishing results of the experiment seem to show that elementary particle Neutrinos, Can. It’s the most spread particles and the lightest. Neutrino is a hardly reacting with matter, It can travel right through the earth without interacting, As an example 70 billion Neutrinos per square second continue coming from the sun. These Neutrino parts traveled through the Earth Crust to the detection point and they synchronized between the 2 points to the nearest Nanno second (A billion of a second) in this distance, they discovered that the neutrino were 60 seconds ahead of what light takes to cover this distance. It's the first time we have an experimental evidence something faster than light and that will make a major change in physics as we know it now.
-Neutrino-
It's believed that modern physics nothing can travel faster than the speed of light. The astonishing results of the experiment seem to show that elementary particle Neutrinos, Can. It’s the most spread particles and the lightest. Neutrino is a hardly reacting with matter, It can travel right through the earth without interacting, As an example 70 billion Neutrinos per square second continue coming from the sun. These Neutrino parts traveled through the Earth Crust to the detection point and they synchronized between the 2 points to the nearest Nanno second (A billion of a second) in this distance, they discovered that the neutrino were 60 seconds ahead of what light takes to cover this distance. It's the first time we have an experimental evidence something faster than light and that will make a major change in physics as we know it now.
Kako smo videli nevidljivo - od crne rupe do Nobelove nagrade za fizikuMilan Milošević
Predavanje održano 27. septembra 2021. godine u okviru serije naučno-popularnih predavanja povodom obeležavanja 50 godina studija fizike, hemije i matematike na Univerzitetu u Nišu i dana Prirodno-matematičkog fakultetu u Nišu.
Astronomy - Stat eof the Art - CosmologyChris Impey
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the properties of the whole universe are covered, including Hubble expansion, the age and size, the big bang, and dark energy.
Discrete and broadband electron acceleration in Jupiter’s powerful auroraSérgio Sacani
The most intense auroral emissions from Earth’s polar regions,
called discrete for their sharply defined spatial configurations, are
generated by a process involving coherent acceleration of electrons
by slowly evolving, powerful electric fields directed along the
magnetic field lines that connect Earth’s space environment to its
polar regions1,2. In contrast, Earth’s less intense auroras are generally
caused by wave scattering of magnetically trapped populations of
hot electrons (in the case of diffuse aurora) or by the turbulent or
stochastic downward acceleration of electrons along magnetic field
lines by waves during transitory periods (in the case of broadband
or Alfvénic aurora)3,4. Jupiter’s relatively steady main aurora has a
power density that is so much larger than Earth’s that it has been
taken for granted that it must be generated primarily by the discrete
auroral process5–7. However, preliminary in situ measurements of
Jupiter’s auroral regions yielded no evidence of such a process8–10.
Here we report observations of distinct, high-energy, downward,
discrete electron acceleration in Jupiter’s auroral polar regions. We
also infer upward magnetic-field-aligned electric potentials of up to
400 kiloelectronvolts, an order of magnitude larger than the largest
potentials observed at Earth11. Despite the magnitude of these
upward electric potentials and the expectations from observations
at Earth, the downward energy flux from discrete acceleration is less
at Jupiter than that caused by broadband or stochastic processes,
with broadband and stochastic characteristics that are substantially
different from those at Earth.
The Fascinating World of Ghost Particles: Exploring Neutrinos and Their Role ...Hello879756
Do you know what ghost particles are? Although they could seem in a horror film, these entities are actually a fascinating and enigmatic shape that scientists have been researching for decades.
Neutrinos are also known as ghost particle, are exceedingly small subatomic particles with no electric charge. They are so tiny that they don't interact with anything as they go through matter, even our bodies and the entire Earth.Nothing can be written about these particles because it is impossible to find them. To study how neutrinos affect other particles and their surroundings, scientists have created sophisticated equipment and methods.
How can we identify these particles?
1. When a neutrinos are collide with other particles in a detector, then a light flash creates, which may be used to detect them. The Super-Kamiokande detector in Japan and the Icecube detector in Antarctica are only two examples of investigations that have employed this technique.
2. Observing neutrinos interact with other particles like protons or electrons in a lab setting is another technique to examine them. The behaviour of neutrinos and their place in the cosmos can be better understood by using of these experiments.
So, why are scientists so interested in studying ghost particles?
These neutrino particles may hold crucial hints or details on the universe's creation and development. Nuclear processes like those in the Sun and significant cosmic occurrences like supernovae are responsible for their formation.Researchers are hoping to get greater insight into the processes that have built the cosmos over billions of years by examining neutrinos. In order to monitor nuclear reactors and other high-risk facilities, they want to develop new technologies and the applications for them, such as neutrino detectors.
FROM UNDERSTANDING BASIC PARTICLE PHYSICS —to exploring the Universe During the first half of 2013, a number of startling advances in astro-particle physics have been announced. In addition to this--the next ultra large cosmic ray experiment is being developed, regions of the world (including southwest Kansas) tested for their suitability to host such an experiment. In this talk you will get a brief introduction of the ideas of particle physics and how they are being transformed into astro-particle measurements to further understand the Universe and the forces within it.
Kako smo videli nevidljivo - od crne rupe do Nobelove nagrade za fizikuMilan Milošević
Predavanje održano 27. septembra 2021. godine u okviru serije naučno-popularnih predavanja povodom obeležavanja 50 godina studija fizike, hemije i matematike na Univerzitetu u Nišu i dana Prirodno-matematičkog fakultetu u Nišu.
Astronomy - Stat eof the Art - CosmologyChris Impey
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the properties of the whole universe are covered, including Hubble expansion, the age and size, the big bang, and dark energy.
Discrete and broadband electron acceleration in Jupiter’s powerful auroraSérgio Sacani
The most intense auroral emissions from Earth’s polar regions,
called discrete for their sharply defined spatial configurations, are
generated by a process involving coherent acceleration of electrons
by slowly evolving, powerful electric fields directed along the
magnetic field lines that connect Earth’s space environment to its
polar regions1,2. In contrast, Earth’s less intense auroras are generally
caused by wave scattering of magnetically trapped populations of
hot electrons (in the case of diffuse aurora) or by the turbulent or
stochastic downward acceleration of electrons along magnetic field
lines by waves during transitory periods (in the case of broadband
or Alfvénic aurora)3,4. Jupiter’s relatively steady main aurora has a
power density that is so much larger than Earth’s that it has been
taken for granted that it must be generated primarily by the discrete
auroral process5–7. However, preliminary in situ measurements of
Jupiter’s auroral regions yielded no evidence of such a process8–10.
Here we report observations of distinct, high-energy, downward,
discrete electron acceleration in Jupiter’s auroral polar regions. We
also infer upward magnetic-field-aligned electric potentials of up to
400 kiloelectronvolts, an order of magnitude larger than the largest
potentials observed at Earth11. Despite the magnitude of these
upward electric potentials and the expectations from observations
at Earth, the downward energy flux from discrete acceleration is less
at Jupiter than that caused by broadband or stochastic processes,
with broadband and stochastic characteristics that are substantially
different from those at Earth.
The Fascinating World of Ghost Particles: Exploring Neutrinos and Their Role ...Hello879756
Do you know what ghost particles are? Although they could seem in a horror film, these entities are actually a fascinating and enigmatic shape that scientists have been researching for decades.
Neutrinos are also known as ghost particle, are exceedingly small subatomic particles with no electric charge. They are so tiny that they don't interact with anything as they go through matter, even our bodies and the entire Earth.Nothing can be written about these particles because it is impossible to find them. To study how neutrinos affect other particles and their surroundings, scientists have created sophisticated equipment and methods.
How can we identify these particles?
1. When a neutrinos are collide with other particles in a detector, then a light flash creates, which may be used to detect them. The Super-Kamiokande detector in Japan and the Icecube detector in Antarctica are only two examples of investigations that have employed this technique.
2. Observing neutrinos interact with other particles like protons or electrons in a lab setting is another technique to examine them. The behaviour of neutrinos and their place in the cosmos can be better understood by using of these experiments.
So, why are scientists so interested in studying ghost particles?
These neutrino particles may hold crucial hints or details on the universe's creation and development. Nuclear processes like those in the Sun and significant cosmic occurrences like supernovae are responsible for their formation.Researchers are hoping to get greater insight into the processes that have built the cosmos over billions of years by examining neutrinos. In order to monitor nuclear reactors and other high-risk facilities, they want to develop new technologies and the applications for them, such as neutrino detectors.
FROM UNDERSTANDING BASIC PARTICLE PHYSICS —to exploring the Universe During the first half of 2013, a number of startling advances in astro-particle physics have been announced. In addition to this--the next ultra large cosmic ray experiment is being developed, regions of the world (including southwest Kansas) tested for their suitability to host such an experiment. In this talk you will get a brief introduction of the ideas of particle physics and how they are being transformed into astro-particle measurements to further understand the Universe and the forces within it.
El Británico Roger Penrose por sus desarrollos teóricos sobre agujeros negros. La Estadounidense Andrea Ghez y el Alemán Reinhald Genzel por el hallazgo de un objeto súper masivo y compacto en el centro de nuestra galaxia.
Por:
Herman J. Mosquera Cuesta
Ingeniero Mecánico UdeA.
PhD en Astrofísica.
Tres investigadores han sido galardonados con el premio Nobel de Física de este año por sus descubrimientos sobre estos fenómenos supermasivos. Roger Penrose por demostrar su existencia según la teoría de la relatividad general y Reinhard Genzel y Andrea Ghez por demostrar que los agujeros negros son capaces de interferir en las órbitas de estrellas cercanas.
Los astrónomos Roger Penrose, Reinhard Genzel y Andrea Ghez se han hecho con el premio Nobel de Física de 2020. El primero de los científicos ha obtenido la mitad del galardón por la demostración fáctica de la existencia de los agujeros negros, siguiendo los preceptos de la teoría de la relatividad de Einstein. Los otros dos investigadores han sido distinguidos por el descubrimiento de un objeto supermasivo en el centro de la Vía Láctea, a unos 26.000 años luz de nuestro planeta.
Reinhard Genzel y Andrea Ghez descubrieron un agujero negro en el centro de la Vía Láctea comprobando la velocidad de las órbitas de sus estrellas circundantes.
“Los descubrimientos de los galardonados de este año han abierto nuevos caminos en el estudio de objetos compactos y supermasivos. Pero estos objetos exóticos todavía plantean muchas preguntas que piden respuestas y plantean nuevos retos de investigación en el futuro, no solo sobre la estructura interna de estos objetos masivos, sino también sobre cómo usar la teoría de la relatividad general en condiciones extremas”, ha declarado David Haviland, presidente del Comité Nobel de Física.
Universe and the Solar System (Lesson 1).pptxJoenelRubino3
SHS Earth and Life Grade 11 Lesson 1. This lesson discusses the compos of the universe, the origin of the universe, different hypotheses of the origin of the universe
The slides are from the talk that I delivered on an INTERNATIONAL WEBINAR on Public Speaking skills called ''SPEAK UP'21'' organized by LEO club of Anna University CEG - Guindy, Chennai on an International collaboration with LEO CLUB of KAATSU International University (KIU) - Srilanka.
Instrumental Landing System - ILS - Airport EngineeringTheerumalai Ga
A short note on the Instrumental Landing system used for flight landing in Airport Engineering. Worked for an assignment. Hope it'll help you for a read to know about ILS
ITS - Intelligent Transport System - An OverviewTheerumalai Ga
A brief overview on the developing trends of Transportation Engineering. Intelligent Transport system uses TECHNOLOGY and existing INFRASTRUCTURAL facilities to provide maximum utility of transport facilities Sincere thanks to FABER MAUNSELL for the material reference and AECOM.COM
BRIHADEESWARAR TEMPLE - An Ancient Architectural marvelTheerumalai Ga
One Architectural marvel that has stood a millennium with violent natural disturbances and more violent human disturbances. One ancient TAMIL - DRAVIDIAN architecture with all it's structural intricacies and the SCIENCE which makes the modern day scientist to baffle. A SCIENTIFIC place than a SPIRITUAL place. One challenging structure analysed from the point of view of engineering details.
A prize winning presentation on "TENSEGRITY architecture" under the topic of "SMART STRUCTURES" for 8 minutes on "BUILDOFEST 2017"
Tensegrity, tensional integrity or floating compression is a structural principle based on the use of isolated components in compression inside a net of continuous tension, in such a way that the compressed members (usually bars or struts) do not touch each other and the prestressed tensioned members (usually cables or tendons) delineate the system spatially.
STEEL - As a Building material:
A 20-minute brief presentation on STEEL for a seminar session.
This presentation covers the areas of :
Origin of Steel, Discovery of STEEL, History of steel making, Classification of STEEL , Properties of steel, Mild Steel , Characteristic tension test curve, Medium Carbon Steel, High Carbon Steel, TOR Steel, Manufacturing processes.
Why STEEL is preferred to concrete?
Disadvantages of STEEL
Some Important Steel Structures
HIGG's BOSON - The 'GOD' Particle - Theerumalai GaTheerumalai Ga
A debut prize winning 5 minute presentation on the GOD particle 'Higg's Boson" at "CHENMAPH- 2K16". A brief description on what is Higg's Boson, it's properties, it's discovery, it's Nobel prize feat and it's importance. A short note on "L.H.C" - Large Hadron Collidor
NEUTRINO AND IT’S SOCIAL APPLICATIONS - Prize Winning 5 minute brief presentation - AnuYogin 2k16
Abstract : On Documents
Introduction:
For the past few decades , the area of “NEUTRINO” has always been a nostalgic area for almost all the nerd physicists around the world. TWENTY-EIGHT flashes of blue light may not seem like much to crow about. But for hundreds of scientists long in their pursuit, witnessing these faint flickers over the last two years has been a cause for celebration, because they mark the arrival of ghostly messengers called NEUTRINOS from the far—and incredibly violent—corners of the universe.
Higg's Boson - The GOD particle
An Abstract submitted for the prize winning presentation on "CHENMAPH - 2K17" for " PHYSICS PAPER PRESENTATION" on " The GOD particle - Higg's Boson"
HALL effect - SemiConductors - and it's Applications - Engineering PhysicsTheerumalai Ga
A 20 mins discussion on the "HALL EFFECT and it's applications" of Semiconductors and a brief explanation about Hall Sensors with a derivation and video attached. Engineering Physics - important area of discussion for Anna University examination- seminar
Seminar of U.V. Spectroscopy by SAMIR PANDASAMIR PANDA
Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
Ultraviolet-visible spectroscopy refers to absorption spectroscopy or reflect spectroscopy in the UV-VIS spectral region.
Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
Deep Behavioral Phenotyping in Systems Neuroscience for Functional Atlasing a...Ana Luísa Pinho
Functional Magnetic Resonance Imaging (fMRI) provides means to characterize brain activations in response to behavior. However, cognitive neuroscience has been limited to group-level effects referring to the performance of specific tasks. To obtain the functional profile of elementary cognitive mechanisms, the combination of brain responses to many tasks is required. Yet, to date, both structural atlases and parcellation-based activations do not fully account for cognitive function and still present several limitations. Further, they do not adapt overall to individual characteristics. In this talk, I will give an account of deep-behavioral phenotyping strategies, namely data-driven methods in large task-fMRI datasets, to optimize functional brain-data collection and improve inference of effects-of-interest related to mental processes. Key to this approach is the employment of fast multi-functional paradigms rich on features that can be well parametrized and, consequently, facilitate the creation of psycho-physiological constructs to be modelled with imaging data. Particular emphasis will be given to music stimuli when studying high-order cognitive mechanisms, due to their ecological nature and quality to enable complex behavior compounded by discrete entities. I will also discuss how deep-behavioral phenotyping and individualized models applied to neuroimaging data can better account for the subject-specific organization of domain-general cognitive systems in the human brain. Finally, the accumulation of functional brain signatures brings the possibility to clarify relationships among tasks and create a univocal link between brain systems and mental functions through: (1) the development of ontologies proposing an organization of cognitive processes; and (2) brain-network taxonomies describing functional specialization. To this end, tools to improve commensurability in cognitive science are necessary, such as public repositories, ontology-based platforms and automated meta-analysis tools. I will thus discuss some brain-atlasing resources currently under development, and their applicability in cognitive as well as clinical neuroscience.
The use of Nauplii and metanauplii artemia in aquaculture (brine shrimp).pptxMAGOTI ERNEST
Although Artemia has been known to man for centuries, its use as a food for the culture of larval organisms apparently began only in the 1930s, when several investigators found that it made an excellent food for newly hatched fish larvae (Litvinenko et al., 2023). As aquaculture developed in the 1960s and ‘70s, the use of Artemia also became more widespread, due both to its convenience and to its nutritional value for larval organisms (Arenas-Pardo et al., 2024). The fact that Artemia dormant cysts can be stored for long periods in cans, and then used as an off-the-shelf food requiring only 24 h of incubation makes them the most convenient, least labor-intensive, live food available for aquaculture (Sorgeloos & Roubach, 2021). The nutritional value of Artemia, especially for marine organisms, is not constant, but varies both geographically and temporally. During the last decade, however, both the causes of Artemia nutritional variability and methods to improve poorquality Artemia have been identified (Loufi et al., 2024).
Brine shrimp (Artemia spp.) are used in marine aquaculture worldwide. Annually, more than 2,000 metric tons of dry cysts are used for cultivation of fish, crustacean, and shellfish larva. Brine shrimp are important to aquaculture because newly hatched brine shrimp nauplii (larvae) provide a food source for many fish fry (Mozanzadeh et al., 2021). Culture and harvesting of brine shrimp eggs represents another aspect of the aquaculture industry. Nauplii and metanauplii of Artemia, commonly known as brine shrimp, play a crucial role in aquaculture due to their nutritional value and suitability as live feed for many aquatic species, particularly in larval stages (Sorgeloos & Roubach, 2021).
Comparing Evolved Extractive Text Summary Scores of Bidirectional Encoder Rep...University of Maribor
Slides from:
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Track: Artificial Intelligence
https://www.etran.rs/2024/en/home-english/
DERIVATION OF MODIFIED BERNOULLI EQUATION WITH VISCOUS EFFECTS AND TERMINAL V...Wasswaderrick3
In this book, we use conservation of energy techniques on a fluid element to derive the Modified Bernoulli equation of flow with viscous or friction effects. We derive the general equation of flow/ velocity and then from this we derive the Pouiselle flow equation, the transition flow equation and the turbulent flow equation. In the situations where there are no viscous effects , the equation reduces to the Bernoulli equation. From experimental results, we are able to include other terms in the Bernoulli equation. We also look at cases where pressure gradients exist. We use the Modified Bernoulli equation to derive equations of flow rate for pipes of different cross sectional areas connected together. We also extend our techniques of energy conservation to a sphere falling in a viscous medium under the effect of gravity. We demonstrate Stokes equation of terminal velocity and turbulent flow equation. We look at a way of calculating the time taken for a body to fall in a viscous medium. We also look at the general equation of terminal velocity.
The ability to recreate computational results with minimal effort and actionable metrics provides a solid foundation for scientific research and software development. When people can replicate an analysis at the touch of a button using open-source software, open data, and methods to assess and compare proposals, it significantly eases verification of results, engagement with a diverse range of contributors, and progress. However, we have yet to fully achieve this; there are still many sociotechnical frictions.
Inspired by David Donoho's vision, this talk aims to revisit the three crucial pillars of frictionless reproducibility (data sharing, code sharing, and competitive challenges) with the perspective of deep software variability.
Our observation is that multiple layers — hardware, operating systems, third-party libraries, software versions, input data, compile-time options, and parameters — are subject to variability that exacerbates frictions but is also essential for achieving robust, generalizable results and fostering innovation. I will first review the literature, providing evidence of how the complex variability interactions across these layers affect qualitative and quantitative software properties, thereby complicating the reproduction and replication of scientific studies in various fields.
I will then present some software engineering and AI techniques that can support the strategic exploration of variability spaces. These include the use of abstractions and models (e.g., feature models), sampling strategies (e.g., uniform, random), cost-effective measurements (e.g., incremental build of software configurations), and dimensionality reduction methods (e.g., transfer learning, feature selection, software debloating).
I will finally argue that deep variability is both the problem and solution of frictionless reproducibility, calling the software science community to develop new methods and tools to manage variability and foster reproducibility in software systems.
Exposé invité Journées Nationales du GDR GPL 2024
Nutraceutical market, scope and growth: Herbal drug technologyLokesh Patil
As consumer awareness of health and wellness rises, the nutraceutical market—which includes goods like functional meals, drinks, and dietary supplements that provide health advantages beyond basic nutrition—is growing significantly. As healthcare expenses rise, the population ages, and people want natural and preventative health solutions more and more, this industry is increasing quickly. Further driving market expansion are product formulation innovations and the use of cutting-edge technology for customized nutrition. With its worldwide reach, the nutraceutical industry is expected to keep growing and provide significant chances for research and investment in a number of categories, including vitamins, minerals, probiotics, and herbal supplements.
This presentation explores a brief idea about the structural and functional attributes of nucleotides, the structure and function of genetic materials along with the impact of UV rays and pH upon them.
1. Created by Theerumalai Ga , 1st
Year Civil Engg, GCE Tirunelveli
1 NEUTRINO and it’s Social Applications
NEUTRINO AND IT’S
SOCIAL APPLICATIONS
-Theerumalai Ga
Introduction:
For the past few decades , the area of “NEUTRINO” has always been a nostalgic
area for almost all the nerd physicists around the world. TWENTY-
EIGHT flashes of blue light may not seem like much to crow about. But for
hundreds of scientists long in their pursuit, witnessing these faint flickers over the
last two years has been a cause for celebration, because they mark the arrival of
ghostly messengers called NEUTRINOS from the far—and incredibly violent—
corners of the universe.
A pic from NOVA detector Source: Physics Today
What’s a neutrino…?
A neutrino is a lepton, an elementary particle with half-integer spin, that
interacts only via the weak subatomic force and gravity. The mass of the neutrino
is tiny compared to other subatomic particles. Neutrinos are the only identified
candidate for dark matter, specifically hot dark matter.
Neutrinos come in three flavours electron neutrinos (νe), muon neutrinos (νμ),
and tau neutrinos(ντ). Each flavor is also associated with an antiparticle, called
2. Created by Theerumalai Ga , 1st
Year Civil Engg, GCE Tirunelveli
2 NEUTRINO and it’s Social Applications
an "antineutrino", which also has no electric charge and half-integer spin.
Neutrinos are produced in a way that conserves lepton number; i.e., for every
electron neutrino produced, a positron (anti-electron) is produced, and for every
electron antineutrino produced, an electron is produced as well.
Neutrinos, named as such because they are electrically neutral, are leptons, and
so are not affected by the strong force either. The weak force is a very short-range
interaction, and gravity is extremely weak on thesubatomic scale. Thus, neutrinos
typically pass through normal matter unimpeded and undetected.
Source: Wikipedia
The first use of Hydrogen Bubble chamber to detect Neutrinos at 1930 by Pauli
What’s the BIG DEAL with the neutrino…?
A typical neutrino can traverse the Earth, or even a light-year’s worth of lead,
without bumping into an atom. Their severe reluctance to mingle makes neutrinos
hard to pin down, so scientists have to build mammoth (and expensive) detectors
like IceCube to trap just a few. In fact, neutrinos, a type of elementary particle
with no electric charge and very little mass, are all around us. Many trillions of
them, produced in the sun’s nuclear core, zip right through our bodies every
second of day and night. Luckily, they do no harm and leave no trace.
Neutrinos, produced in nuclear reactions and traveling at nearly the speed of light,
zip away with little impediment, bringing scientists valuable information from
the place of their birth. Neutrinos have already taught physicists a great deal about
the subatomic realm, and given astronomers a way to test their calculations of the
reactions at the scorching heart of the sun. Back in 1987, neutrinos were the first
harbingers of the dramatic demise of a massive, bloated star in a satellite galaxy
of the Milky Way. Soon, with more detections and better statistics, the IceCube
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Year Civil Engg, GCE Tirunelveli
3 NEUTRINO and it’s Social Applications
researchers expect to pinpoint the cosmic particle accelerators, likely powered by
black holes or dying stars, that propel energetic neutrinos like the 28 they have
already nabbed.
That may be just the beginning. Some have suggested, with varying degrees of
seriousness, that neutrinos could be used not only to probe the extremes of space
but for more pragmatic, down-to-earth purposes. Their proposed schemes range
from the perfectly sensible to the rather outlandish, and some require much better
technology for producing and detecting neutrinos than is currently available.
The ICE-CUBE apparatus at Antarctica Source : The BUSINESS Insider
The Discovery of Neutrinos:
Wolfgang Pauli first postulated NEUTRINO in 1930 which was later confirmed
with its discovery in 1956 by Clyde Cowan and Freidrick Reinnes. It was the
electron neutrino. Whereas the muon neutrino was discovered by Leon
Lederman, Melvin Schwartz and Jack Steinberger in1962. And the Tau neutrino
was discovered by the DONUT collaboration in 2000.
Sources of Neutrinos:
Researchers reported in Science that IceCube, a novel observatory made of some
5,000 sensory orbs strung on 86 steel cables and buried more than a mile deep in
the Antarctic ice, has been registering about one energetic neutrino originating
from beyond our galaxy each month.
4. Created by Theerumalai Ga , 1st
Year Civil Engg, GCE Tirunelveli
4 NEUTRINO and it’s Social Applications
The main sources are
Artificial
i. Reactor neutrinos
ii. Accelerator neutrinos
iii. Nuclear bombs
Geologic
Atmospheric
Solar
Supernovae
BIG BANG
Future Application of Neutrinos:
Find exploding stars in the far reaches of our galaxy
It has been over four centuries since astronomers have seen a
supernova in the Milky Way. If a star explodes in the far side of the galaxy,
interstellar dust would obscure our view—but the neutrinos would come
through unhindered, with modern detectors giving us an unprecedented
peek at the action.
Figure out what keeps the Earth’s interior warm
Part of our planet’s internal heat comes from the decay of radioactive
elements—but we don’t know exactly what fraction. Since radioactivity also
releases neutrinos, measuring them could tell us how much uranium and
thorium are in the Earth’s crust and mantle.
Expose rogue nuclear reactors and covert bomb tests
Nuclear reactors and nuclear bombs release staggering numbers of
neutrinos, so international monitors could rely on them for surveillance and
help prevent proliferation.
5. Created by Theerumalai Ga , 1st
Year Civil Engg, GCE Tirunelveli
5 NEUTRINO and it’s Social Applications
Understand how matter won over antimatter
There should have been equal amounts of matter and antimatter right
after the Big Bang. But today’s universe consists overwhelmingly of matter.
Physicists believe the behavior of neutrinos could reveal why.
Scan Earth’s crust for mineral or oil deposits
Some scientists have proposed that intense beams of neutrinos could
be used to probe the Earth’s crust, sort of like how dentists use X-rays to scan
teeth for cavities.
Use neutrino signals for equity trading
One researcher has suggested linking the world’s financial centers
using encoded neutrino beams that take shortcuts through the Earth, giving
high-frequency traders a time advantage of up to tens of milliseconds.
Communicate with aliens
Since neutrinos travel freely through space, proponents argue that
they would make terrific messengers between advanced civilizations across
the galaxy.
Conclusion:
But if these visionaries turn out to be right, the esoteric and cagey neutrinos might
be of interest not just for physicists chasing Nobel Prizes but also for nuclear
monitors, mineral prospectors, and maybe even traders looking to make an
extremely fast buck.
References:
Wikipedia
The Business Insider – Ray Jayawardena’s article on Neutrino Hunters
Boston Globe – Ray Jayawardena
Physics Today – Philip McClain
The ICECUBE official website.
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6 NEUTRINO and it’s Social Applications