New way to 'fish out' radioactive elements from nuclear waste

March 12, 2017

London, Mar 12: Scientists have found that the most toxic elements from radioactive nuclear waste may be 'fished out' using arsenic molecules - a breakthrough that could make the alternative energy industry safer and more effective. Researchers reported the first examples of thorium with multiple bonds to arsenic to exist under ambient conditions on multi-gram scales where before they had only been prepared on very small scales at temperatures approaching that of interstellar space.

nuclear

"Nuclear power could potentially produce far less carbon dioxide than fossil fuels, but the long-lived waste it produces is radioactive and needs to be handled appropriately," said Elizabeth Wildman, from University of Manchester in the UK. "In order to find ways of separating, recycling and reducing the volume of nuclear waste, research has focused on developing our understanding of how elements like thorium and uranium interact with elements from around the periodic table to potentially help improve nuclear waste clean-up," said Wildman.

"We need to reduce the volume of nuclear waste in order to make it easier to handle and process it to remove benign elements or separate the high level from low level waste," said Professor Steve Liddle, from The University of Manchester. The study looked at how the soft element arsenic interacts with thorium, because arsenic could in principle be used in organic molecules that bond to metal atoms and improve extraction processes.

"There is currently significant interest in using organic molecules to extract, selectively, metal ions from the 'soup' of nuclear waste and fish out the more radioactive and toxic ones and leave the rest behind," Liddle said. "This requires an understanding of chemical bonding and how the organic extractants bind to different metals. We can then exploit this knowledge to achieve separation by having them selectively bind to one type of metal and remove it from the soup," he said.

"There is mounting evidence that the molecules that are best at this contain soft donor atoms to the metals. Thus, we need to understand soft donor-to-metal binding better," he added. "Arsenic is a soft donor, so we have prepared model complexes with it to understand the nature of the bonding," said Liddle.

"Until now, complexes exhibiting multiple bonds between thorium and arsenic were limited to spectroscopic experiments carried out at temperatures close to that of interstellar space (3-10 Kelvin) where only a few molecules were made at a time," he said.

"We have made molecules in multi-gram quantities and they are stable under ambient conditions enabling us to study them more straightforwardly. We might be able to use this new knowledge and understanding in a real system in the future," he added. The finding is published in the journal Nature Communications.

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Agencies
June 24,2020

New Delhi, Jun 24: The Centre has made it mandatory for sellers to enter the 'Country of Origin' while registering all new products on government e-marketplace (GeM).

The e-marketplace is a special purpose vehicle (SPV) under the Ministry of Commerce and Industry which facilitates the entry of small local sellers in public procurement, while implementing 'Make in India' and MSE Purchase Preference Policies of the Centre.

Accordingly, the ministry said the move has been made to promote 'Make in India' and 'Atma Nirbhar Bharat'.

The provision has been enabled via the introduction of new features on GeM.

Besides the registration process, the new feature also reminds sellers who have already uploaded their products, to disclose their products' 'Country of Origin' details.

The ministry further said that failing to disclose the detail will lead to removal of the products from the e-marketplace.

"GeM has taken this significant step to promote 'Make in India' and 'Aatmanirbhar Bharat'," the ministry said in a statement.

"GeM has also enabled a provision for indication of the percentage of local content in products. With this new feature, now, the 'Country of Origin' as well as the local content percentage are visible in the marketplace for all items. More importantly, the 'Make in India' filter has now been enabled on the portal. Buyers can choose to buy only those products that meet the minimum 50 per cent local content criteria."

In case of bids, the ministry said that buyers can now reserve any bid for a "Class I Local suppliers. For those bids below Rs 200 crore, only Class I and Class II Local Suppliers are eligible to bid, with Class I supplier getting purchase preference".

In addition to this, the Department for Promotion of Industry and Internal Trade (DPIIT) has reportedly called for a meeting with all e-commerce companies such as Amazon and Flipkart to display the country of origin on the products sold on their platform, as well as the extent of value added in India.

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Agencies
June 8,2020

Washington DC, Jun 8: Astronomers acting on a hunch have likely resolved a mystery about young, still-forming stars and regions rich in organic molecules closely surrounding some of them.

They used the National Science Foundation's Karl G Jansky Very Large Array (VLA) to reveal one such region that previously had eluded detection and that revelation answered a longstanding question.

The regions around the young protostars contain complex organic molecules which can further combine into prebiotic molecules that are the first steps on the road to life.

The regions, dubbed "hot corinos" by astronomers, are typically about the size of our solar system and are much warmer than their surroundings, though still quite cold by terrestrial standards.

The first hot corino was discovered in 2003 and only about a dozen have been found so far. Most of these are in binary systems, with two protostars forming simultaneously.

Astronomers have been puzzled by the fact that, in some of these binary systems, they found evidence for a hot corino around one of the protostars but not the other.

"Since the two stars are forming from the same molecular cloud and at the same time, it seemed strange that one would be surrounded by a dense region of complex organic molecules and the other wouldn't," said Cecilia Ceccarelli, of the Institute for Planetary Sciences and Astrophysics at the University of Grenoble (IPAG) in France.

The complex organic molecules were found by detecting specific radio frequencies, called spectral lines, emitted by the molecules. Those characteristic radio frequencies serve as "fingerprints" to identify the chemicals.

The astronomers noted that all the chemicals found in hot corinos had been found by detecting these "fingerprints" at radio frequencies corresponding to wavelengths of only a few millimetres.

"We know that dust blocks those wavelengths, so we decided to look for evidence of these chemicals at longer wavelengths that can easily pass through dust," said Claire Chandler of the National Radio Astronomy Observatory, and principal investigator on the project.

"It struck us that dust might be what was preventing us from detecting the molecules in one of the twin protostars," added Chandler.

The astronomers used the VLA to observe a pair of protostars called IRAS 4A, in a star-forming region about 1,000 light-years from Earth. They observed the pair at wavelengths of centimetres.

At those wavelengths, they sought radio emissions from methanol, CH3OH (wood alcohol, not for drinking). This was a pair in which one protostar clearly had a hot corino and the other did not, as seen using the much shorter wavelengths.

The result confirmed their hunch. "With the VLA, both protostars showed strong evidence of methanol surrounding them. This means that both protostars have hot corinos. The reason we did not see the one at shorter wavelengths was because of dust," said Marta de Simone, a graduate student at IPAG who led the data analysis for this object.

The astronomers cautioned that while both hot corinos now are known to contain methanol, there still may be some chemical differences between them. That, they said, can be settled by looking for other molecules at wavelengths not obscured by dust.

"This result tells us that using centimetre radio wavelengths is necessary to properly study hot corinos," Claudio Codella of Arcetri Astrophysical Observatory in Florence, Italy, said.

"In the future, planned new telescopes such as the next-generation VLA and SKA, will be very important to understanding these objects," added Codella.

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Agencies
March 10,2020

New Delhi, Mar 10: Crisis-hit Yes Bank on Tuesday said that it has enabled inward IMPS and NEFT services.

The move allows people to send money from other bank accounts to their Yes Bank account through IMPS (Immediate Payment Service) and NEFT (National Electronic Funds Transfer) mode.

In a tweet, the bank also said that Yes Bank customers can pay their credit card dues and loan obligations from other bank accounts.

"Inward IMPS/NEFT services have now been enabled. You can make payments towards YES BANK Credit Card dues and loan obligations from other bank accounts. Thank you for your co-operation. @RBIA @FinMinIndia," said tweet.

Last week Yes Bank was placed under moratorium and a withdrawal cap of Rs 50,000 was imposed till April 3.

The administrator of Yes Bank, Prashant Kumar and Rajnish Kumar, the Chairman of the State Bank of India are hopeful that moratorium would be lifted within a week.

As per the Reserve Bank of India (RBI) draft reconstruction scheme for the crisis-hit private lender, the SBI will take up 49 per cent in the bank by investing Rs 2,450 crore.

The new board of directors will stand constituted from the appointed date. It will comprise a CEO and MD, non-executive chairman and non-executive directors. The SBI will have nominee directors appointed on the board of the reconstructed bank.

The RBI may appoint additional directors to the board, who shall continue in office for one year, or until an alternate board is constituted by Yes Bank.

The SBI will not reduce its holding below 26 per cent before completion of three years from the date of infusion of the capital.

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