Skip to main content

Atoms promise as proton conducting membranes, for each of the thinner mineral green technologies.


Experiments by researchers at the University of Manchester have found that the atom is a type of common mineral found in each form of thin mic - soil, and is an excellent proton conductor, and this amazing result results in fuel cells and other hydrogen-related technologies, As such, it is important to use 2-D materials in applications.

Researchers have conducted many experiments before, with Manchester researchers led by Professor Andre Geim and Dr. Marcelo Lozada-Hidalgo finding that, like graphene, a one-atom thick material is highly permeable to the nuclei of protons, hydrogen atoms. However, researchers also found that there are many other 2-D substances, like molybdenum sulfide (MoS2), which had only three atoms thick, and are completely impermeable to protons.The results of the experiment by the same researchers suggested that any one-atom thick crystal can be permeable to protons.

Researchers, writing in Nature Nanotechnology, have shown that protons can allow very easily, through multiple layered micas, and are about 10 times thicker than graphene, because micas and graphite  Like, crystal layers stacked on top of each other, and can be moved down to one layer, the team of researchers separated one of these layers, and this  Or, that was 100 times more permeable to protons than Graphene proton.

The team of researchers said that at first, this result seemed impossible to come up with, because micas are too thick for protons, and this monolayers are much thicker than MoS2, and would be completely impermeable to protons. However, the researchers pierced the tubular channels in their experiment, and it was found that the mic can be thought of as a crystal slab, because the channels are not empty, but are filled with hydroxyl groups, because it  In water the protons of a one-dimensional chain operate, and these protons jump along these chains, and this makes the material an excellent proton conductor Switch to change. 

During the project, Lucas Mogg and a Ph.D. he said.We have found that the proton conductivity in the atom-thin mic is 10 to 100 times greater than that of graphene, and this is encouraging, as it was previously considered graphene to be a promising protecting material.Researchers' results show that mikes can be more promising because they are the least abundant and inexpensive.

Professor Andre Geim believes that this can also result in many other 2-D materials being turned into proton conductors. Professor Andre Geim states that our strategy is not limited to protons or micas only.And it is similar to mic with many 2-D crystal atomic-scale channels.Professor Andre Geim says that we can, that will bring many unexpected events, and fresh new applications in the field of protons and ionic conductors.

Researchers have also found in their experiment, mikes are highly conductive in temperature range, and are notorious for related technologies.Dr,Marcello Lozada-Hidalgo states that there is a shortage of proton-carrying materials, and that they can work reliably between 100 ° C and 500 ° C.  However, it is the sweet spot temperature range for optimal operation of many fuel cells and for, and each of the hydrogen technologies, and atmoli-thick mikes in this temperature range work correctly, and they draw attention from this point of view.

And in addition to all this, the researchers believe that they are now working on making a mica prototype membrane, and this is a large enough test for industrial conditions, the area of ​​two-dimensional ionic conductors, and the properties of each crystal  Promises more, and can be converted into other ionic and proton conductors.  

Comments

Popular posts from this blog

NASA/ESA Hubble Space Telescope Reveals New Details of the Orion Nebula’s Star Formation.

  This NASA/ESA Hubble Space Telescope image captures the Orion Nebula (Messier 42, M42), the nearest star-forming region to Earth, located about 1,500 light-years away. A captivating new image captured by the NASA/ESA Hubble Space Telescope offers an extraordinary look into the Orion Nebula, the nearest massive star-forming region to Earth. Located just 1,500 light-years away, this nebula is visible to the naked eye below the three stars forming Orion's "belt." The region is home to hundreds of newborn stars, including two protostars featured in the image: HOPS 150 and HOPS 153. Named after the Herschel Orion Protostar Survey, conducted with ESA’s Herschel Space Observatory, the protostars HOPS 150 and HOPS 153 provide key insights into the early stages of star formation. HOPS 150, visible in the upper-right corner of the image, is a binary star system, with two young stars orbiting one another. These protostars are surrounded by small dusty disks, where material from th...

New Method Detects Small Asteroids in Main Belt, Offering Insight for Planetary Defense.

  An international team of physicists, led by MIT researchers, has developed a groundbreaking method to detect small asteroids, as small as 10 meters in diameter, within the main asteroid belt. These space rocks, ranging from the size of a bus to several stadiums wide, were previously undetectable using traditional methods. The team's discovery, detailed in a paper published in Nature, could significantly improve tracking of potential asteroid impactors, aiding planetary defense efforts. The main asteroid belt, located between Mars and Jupiter, is home to millions of asteroids, but until now, scientists could only detect objects roughly a kilometer in diameter. The new detection technique, which utilizes the "shift and stack" method, is able to identify much smaller asteroids, even those far from Earth, enabling more precise orbital tracking. This breakthrough is crucial for planetary defense, allowing scientists to spot near-Earth objects that may pose a threat in the fu...

XSPECT Payload Successfully Validates Performance through Cas A Observation.

  The XSPECT instrument captures a detailed spectrum of the supernova remnant Cassiopeia A (Cas A), encompassing both the Galactic Cosmic Ray (GCR) background and the Cosmic X-ray Background (CXB). The flux observed above 8 keV predominantly results from the combined contributions of CXB and GCR. The presented spectrum, depicted in the figure, is derived from a cumulative integration time of 20 ksec, collected across multiple orbits, providing valuable insights into the X-ray emissions associated with Cas A. XPoSat, India's inaugural X-ray polarimetric mission, has achieved a significant as the XSPECT instrument captures its initial observations from the Cassiopeia A (Cas A) supernova remnant. Launched on January 1, 2024, XPoSat is equipped with two co-aligned instruments, namely the POLarimeter Instrument in X-rays (POLIX) and X-ray SPECtroscopy and Timing (XSPECT). This mission is designed to unravel the mysteries of cosmic X-ray sources. While POLIX focuses on examining X-ray po...