Environment-Clean-Generations

Environment-Clean-Generations
THE DEFINITIVE BLOG FOR EVERYTHING YOU NEED TO KNOW ABOUT THE ENVIRONMENT YOU LIVE IN, WITH REFERENCE TO LIFE, EARTH AND COSMIC SPACE SCIENCES, PRESENTED BY ENVIRONMENTAL ENGINEER DORU INDREI, ENVIRONMENTAL QUALITY AND ENERGY SPACIALIST
"Life is not about what we know, but what we don't know, craving the unthinkable makes it so amazing, that is worth dying for." Doru Indrei
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Showing posts with label protons. Show all posts
Showing posts with label protons. Show all posts

Racing to Create the Heaviest Element in the Universe


Two international teams are competing to create the heaviest element in the universe. Super-heavy elements are the elements at the bottom of the periodic table with an atomic number (the number of protons) above 104. The previous heaviest element, temporarily called ununoctium, was "discovered" in 2002, and the two teams are now attempting to produce elements 119 and 120.

Jon Petter Omtvedt, a professor of nuclear chemistry at University of Oslo, is working with scientists from Western Europe, Japan and the United States, running experiments at the German GSI Helmholtzzentrum für Schwerionenforschung. The other team is made up of Russian and American scientists working out of the Joint Institute for Nuclear Research in Dubna, Russia. "The competition is razor-sharp," said Omtvedt. "Super-heavy elements are highly unstable and very difficult to create. It is like finding something unknown in outer space."

Manufacturing a single atom of a new element is not sufficient to be credited with discovering a new element. The results need to be replicated. "No one will gain any recognition until another laboratory manages to recreate the experiment. In the worst case, it may take several decades before the experiment has been verified," said Omtvedt. The heavier a super-heavy element is, the longer it takes to produce, and the shorter it will remain intact. A single atom of element 106 could be created within one hour when it was first discovered, and that atom decayers into lighter elements in 20 seconds. An atom of element 118 could be created in one month, and its half-life (the time before half of it decayed) was a mere 1.8 milliseconds.

Two weeks ago, nuclear physicists at Oak Ridge National Laboratory in Oak Ridge, Tennessee, created 20 mg of the highly radioactive element berkelium. Each team vying to create element 119 was given 10 mg of berkelium. They will bombard a metal plate laced with berkelium atoms with a beam of titanium atoms. The teams are working on a tight schedule. Berkelium's half life is only 320 days, and once 320 days have passed, half of their sample will have decade into other elements. "It is extremely difficult to create intense titanium beams. To accomplish this, we have secrets that we will not share with others," said Omtvedt.

The basic principle of creating super-heavy atoms is simple: smash the atoms of one element into those of another and their protons will add up to create a new element. Titanium's 22 protons will join berkelium's 97 to create an atom with 119 protons, one atom of element 119. Most of the time, though, the atoms will collide and shatter or partially destroy each other. But rarely, "less than once a month," the protons will collide to create a complete atom. Detecting such a rare occurrence is a challenge. "You will have to detect this one atom on a metal plate where more than 100,000 superfluous events are occurring each second," Omtvedt said. The only way to detect the new atom is to observe the radioactive radiation it emits when it decays. There will be no evidence of the new element until it's already gone.
"We are working right at the cutting edge of what is experimentally possible," said Omtvedt. "In order to study the heaviest elements, we have to stretch the current technology to its utmost and even a little further."

Particles Faster Than Speed Of Light At CERN


Enormous underground detectors are needed to catch neutrinos, that are so elusive as to be dubbed "ghost particles".

A meeting at Cern, the world's largest physics lab, has addressed results that suggest subatomic particles have gone faster than the speed of light. 
The team presented its work so other scientists can determine if the approach contains any mistakes.

If it does not, one of the pillars of modern science will come tumbling down.

Antonio Ereditato added "words of caution" to his Cern presentation because of the "potentially great impact on physics" of the result.


The speed of light is widely held to be the Universe's ultimate speed limit, and much of modern physics - as laid out in part by Albert Einstein in his theory of special relativity - depends on the idea that nothing can exceed it.


Thousands of experiments have been undertaken to measure it ever more precisely, and no result has ever spotted a particle breaking the limit.


"We tried to find all possible explanations for this," the report's author Antonio Ereditato of the Opera collaboration told BBC News on Thursday evening.

"We wanted to find a mistake - trivial mistakes, more complicated mistakes, or nasty effects - and we didn't.

"When you don't find anything, then you say 'well, now I'm forced to go out and ask the community to scrutinise this'."


Friday's meeting was designed to begin this process, with hopes that other scientists will find inconsistencies in the measurements and, hopefully, repeat the experiment elsewhere.


"Despite the large [statistical] significance of this measurement that you have seen and the stability of the analysis, since it has a potentially great impact on physics, this motivates the continuation of our studies in order to find still-unknown systematic effects," Dr Ereditato told the meeting.

"We look forward to independent measurement from other experiments."
Neutrinos come in a number of types, and have recently been seen to switch spontaneously from one type to another.

The Cern team prepares a beam of just one type, muon neutrinos, and sends them through the Earth to an underground laboratory at Gran Sasso in Italy to see how many show up as a different type, tau neutrinos.

In the course of doing the experiments, the researchers noticed that the particles showed up 60 billionths of a second earlier than they would have done if they had travelled at the speed of light.


This is a tiny fractional change - just 20 parts in a million - but one that occurs consistently.

The team measured the travel times of neutrino bunches some 16,000 times, and have reached a level of statistical significance that in scientific circles would count as a formal discovery. 

But the group understands that what are known as "systematic errors" could easily make an erroneous result look like a breaking of the ultimate speed limit.

That has motivated them to publish their measurements.


"My dream would be that another, independent experiment finds the same thing - then I would be relieved," Dr Ereditato told BBC News.

But for now, he explained, "we are not claiming things, we want just to be helped by the community in understanding our crazy result - because it is crazy".



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Earth Surrounded By A "Ring of Antimatter"



Astrophysicists have found, using spacecraft Pamela, that in Earth's magnetosphere is manifested a flow of antiprotons resulting from nuclear interactions of cosmic rays (energetic charged particles such as protons, electrons and helium nuclei) and the Earth's atmosphere, antiprotons that accumulates in geomagnetic field at altitudes of several hundred kilometers.

                 When cosmic rays emanating from the sun and other sources in the universe, atoms bombard the Earth's upper atmosphere, the result is similar as collisions in particle accelerators manifested on the ground, that new particles are born.

                 For a while experts suspect that these collisions produce atmospheric antiprotons, just as in accelerators, but so far has only been speculated about their fate, once the scenarios are created. 

                Theoretically, these particles should be concentrated in the Earth's magnetic field, possibly in the region called the South Atlantic Magnetic Anomaly, that part of the Van Allen Belt is closest to the Earth and where energy charged particles tend to gather. 

                To solve the mystery, astronomers released in 2006 on orbit, PAMELA spacecraft , just with a mission to identify antiprotons in cosmic rays.  

                Now that they have carefully analyzed the data collected by the probe in 850 days orbiting the Earth, it was found that Pamela found, indeed, 28  antiprotons in the South Atlantic Magnetic Anomaly. The amount has exceeded any expectations of anyone trying to find some type of solar wind particles and achievement show that antiprotons are captured and stored in even one of Van Allen axes. 

                The discovery of a further belt of antiprotons has a major impact because the number is small compared to electrons and protons trapped in the same area. But confirmation of theoretical predictions is always interesting.


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