Showing posts with label synchotron. Show all posts
Showing posts with label synchotron. Show all posts

Wednesday, August 15, 2018

Powerful beams of infrared light could probe cells, diagnose diseases



In tissue from a mouse's brain, seen at lower (left) and higher magnification (right), infrared spectroscopy can distinguish astrocytes (red) from neurons (green).
 
ARIS POLYZOS & LILA LOVERGNE
http://www.sciencemag.org/news/2018/08/powerful-beams-infrared-light-could-probe-cells-diagnose-diseases

By Mitch Leslie

To identify a cell, researchers often have to abuse it—rip it from its home, douse it with toxic fixatives, doctor its DNA, or coerce it into making exotic proteins that could upset its biochemistry. Even if the cell survives, it may never be the same again. But a strong yet gentle beam of light could one day allow researchers to classify cells while leaving them unharmed and alive for additional study.
A team led by biophysicist Cynthia McMurray and physicist Michael Martin of the Lawrence Berkeley National Laboratory (LBNL) in California has found that by scanning cells with an intense beam of infrared radiation produced by a synchrotron, a type of particle accelerator, they can capture a biochemical signature that reveals cells' identities.
The researchers presented early results from the method in June at a meeting in the United Kingdom, and they are now evaluating it with a 1-year pilot grant from the Chan Zuckerberg Initiative (CZI). If it works, the team's spectral phenotyping technique could provide a tool for another endeavor backed by CZI: the Human Cell Atlas, an international project that aims to chart the type and location of every cell in the body. And if the synchrotron-driven method can be adapted to more modest infrared instruments available to other labs and hospitals, spectral phenotyping might one day also help diagnose illnesses, probe the cellular changes that lead to disease, and delve into embryonic development. "The tools we are putting together will blow open this field," McMurray predicts.
Scientists who are familiar with the still unpublished results call the approach promising. "I'm looking forward to seeing the research that's going to come out," says spectroscopist Peter Gardner of The University of Manchester in the United Kingdom. Chemical physicist Hugh Byrne of the Dublin Institute of Technology is impressed by how thoroughly the group is testing its approach. "It's a concerted program to demonstrate the capabilities of the technique."
Martin and McMurray like to contrast their approach with a widely used cell-identification technique: fluorescent labeling. To spur cells of a specific type to produce a label such as green fluorescent protein (GFP), scientists have to equip them with the molecule's gene. The techniques for adding DNA can alter the cells, and because GFP is foreign to them—it's originally from a jellyfish—it could also modify their physiology. Moreover, McMurray notes, researchers typically have to zap fluorescent labels with a laser to induce them to light up, which can harm or kill cells. Other techniques are no less invasive. "If you are doing labeling or staining, you are changing the true chemistry" of cells, Martin says. "We want to explore what the chemistry is, not alter it to do the measurements."
That's where infrared spectroscopy comes in. "Infrared is not invasive, so it can be used on intact tissues and living cells," McMurray says. When a sample is exposed to different wavelengths of infrared radiation, how much light of each wavelength it absorbs indicates the kinds of chemical groups it contains. Unlike fluorescent labeling, the absorption pattern usually can't reveal whether a cell is producing a specific molecule—for example, the immune receptors CD4 or CD8, which are often used to define two classes of T cells. But a cell's infrared spectrum does reveal broad types of molecules—such as fats and proteins—providing a biochemical fingerprint. As a result, "You get a much more holistic picture of the cell," Byrne says.
Martin and McMurray say standard infrared sources don't provide the sensitivity they needed, so the team turned to LBNL's Advanced Light Source synchrotron, whose infrared beam is one of the brightest in the world. It "allows us to get better resolution and fidelity," Martin says. At the June SPEC2018 conference in Glasgow, U.K., McMurray and Martin revealed they could discriminate two types of brain cells—neurons and astrocytes—in slices of brain from mice. In brain tissue from rodents with a condition mimicking Huntington disease, they could also detect an increase in lipids that indicates degeneration. In the future, the researchers plan to automate cell identification by enlisting machine learning algorithms to pick out distinguishing features of each cell type.
McMurray and her colleagues still need to determine whether a cell's spectral signature remains constant or varies with its location in the body. For potential medical uses, they also want to find out whether a human cell's infrared signature changes when a person becomes ill. So far, however, the researchers have analyzed only mouse tissues. "We wanted to make sure the method is robust," McMurray says.
One limitation of the new technique is obvious—synchrotrons are huge, expensive, and rare, and often have monthslong waiting lists. "You aren't going to be taking your synchrotron into the hospital," Gardner says. But lab machines are rapidly approaching the infrared-generating power of particle accelerators, he notes. McMurray adds that after using the synchrotron to pinpoint distinctive spectral patterns for a variety of cell types, the researchers plan to publish a catalog that would allow other scientists to compare results from their own samples, even ones captured with less discerning lab devices.
Gardner expects the project to have an impact. "They have the tools, the expertise, and the personnel to accelerate this work," he says.

Thursday, May 28, 2015

Abstract-Observing microscopic structures of a relativistic object using a time-stretch strategy

http://www.nature.com/srep/2015/150528/srep10330/full/srep10330.html



Emission of light by a single electron moving on a curved trajectory (synchrotron radiation) is one of the most well-known fundamental radiation phenomena. However experimental situations are more complex as they involve many electrons, each being exposed to the radiation of its neighbors. This interaction has dramatic consequences, one of the most spectacular being the spontaneous formation of spatial structures inside electrons bunches. This fundamental effect is actively studied as it represents one of the most fundamental limitations in electron accelerators, and at the same time a source of intense terahertz radiation (Coherent Synchrotron Radiation, or CSR). Here we demonstrate the possibility to directly observe the electron bunch microstructures with subpicosecond resolution, in a storage ring accelerator. The principle is to monitor the terahertz pulses emitted by the structures, using a strategy from photonics, time-stretch, consisting in slowing-down the phenomena before recording. This opens the way to unpreceeded possibilities for analyzing and mastering new generation high power coherent synchrotron sources.

Thursday, May 8, 2014

Berkeley Lab Develops Nanoscope to Probe Chemistry on the Molecular Scale


http://newscenter.lbl.gov/news-releases/2014/05/07/berkeley-lab-develops-nanoscope-to-probe-chemistry-on-the-molecular-scale/?fb_action_ids=10202078686957296&fb_action_types=og.likes

New technique uses infrared synchrotron light and atomic force microscopy to study batteries, cell membranes, stardust, and other complex systems on the nanoscale

Kate Greene 510-486-4404  kgreene@lbl.gov
 0 

 
News Release


For years, scientists have had an itch they couldn’t scratch. Even with the best microscopes and spectrometers, it’s been difficult to study and identify molecules at the so-called mesoscale, a region of matter that ranges from 10 to 1000 nanometers in size. Now, with the help of broadband infrared light from the Advanced Light Source (ALS) synchrotron at the U.S. Department of Energy’s Lawrence Berkeley National Laboratory (Berkeley Lab), researchers have developed a broadband imaging technique that looks inside this realm with unprecedented sensitivity and range.
This peptoid nanosheet, produced by Gloria Olivier and Ron Zuckerman at Berkeley Lab, is less than 8 nanometers thick at points. SINS makes it possible to acquire spectroscopic images of these ultra-thin nanosheets for the first time.
This peptoid nanosheet, produced by Gloria Olivier and Ron Zuckerman at Berkeley Lab, is less than 8 nanometers thick at points. SINS makes it possible to acquire spectroscopic images of these ultra-thin nanosheets for the first time.
By combining atomic force microscopy with infrared synchrotron light, researchers from Berkeley Lab and the University of Colorado have improved the spatial resolution of infrared spectroscopy by orders of magnitude, while simultaneously covering its full spectroscopic range, enabling the investigation of variety of nanoscale, mesoscale, and surface phenomena that were previously difficult to study.
The new technique, called Synchrotron Infrared Nano-Spectroscopy or SINS, will enable in-depth study of complex molecular systems, including liquid batteries, living cells, novel electronic materials and stardust.
“The big thing is that we’re getting full broadband infrared spectroscopy at 100 to 1000 times smaller scale,” says Hans Bechtel, principal scientific engineering associate at Berkeley Lab. “This is not an incremental achievement. It’s really revolutionary.”
In a Proceedings of the National Academy of Sciences paper published May 6 onlinetitled “Ultra-broadband infrared nano-spectroscopic imaging,” Berkeley Lab’s Bechtel and Michael Martin, a Berkeley Lab staff scientist, and colleagues from Markus Raschke’s group at the University of Colorado at Boulder describe SINS. They demonstrate the nanoscope’s ability to capture broadband spectroscopic data over a variety of samples, including a semiconductor-insulator system, a mollusk shell, proteins, and a peptoid nanosheet. Martin says these demonstrations just “scratch the surface” of the potential of the new technique.
Synchronizing Scopes
SINS combines two pre-existing infrared technologies: a newer technique called infrared scattering-scanning near-field optical microscopy (IR s-SNOM) and an old laboratory standby, known even to college chemistry students, called Fourier Transform Infrared Spectroscopy (FTIR). A clever melding of these two tools, combined with the intense infrared light of the synchrotron at Berkeley Lab gives the researchers the ability to identify clusters of molecules sized as small as 20 to 40 nanometers.
Experimental setup for SINS that includes the synchrotron light source, an atomic force microscope, a rapid-scan Fourier transform infrared spectrometer, a beamsplitter, mirrors and a detector.
Experimental setup for SINS that includes the synchrotron light source, an atomic force microscope, a rapid-scan Fourier transform infrared spectrometer, a beamsplitter, mirrors and a detector.
The new approach overcomes long-standing barriers with pre-existing microscopy techniques that often involve demanding technical and sample preparation requirements. Infrared spectroscopy uses low-energy light, is minimally invasive, and is applicable under ambient conditions, making it an excellent tool for chemical and molecular identifications in systems that are static as well as those that are living and dynamic. The technique works by shining low-energy infrared light onto a molecular sample. Molecules can be thought of as systems of balls (atoms) and springs (bonds between atoms) that vibrate with characteristic wiggles; they absorb infrared radiation at frequencies that correspond to their natural vibrating modes. The output from this absorption is a spectrum, often called a fingerprint, which shows distinctive peaks and dips, depending on the bonds and atoms present in the sample.
But infrared spectroscopy has its challenges too. While it works well for bulk samples, traditional infrared spectroscopy can’t resolve molecular composition below about 2000 nanometers. The major hurdle is the diffraction limit of light, which is the fundamental barrier that determines the smallest focus spot of light and is particularly troublesome for the large wavelengths of infrared light. In recent years, though, the diffraction limit has been overcome by a technique called scattering-scanning near-field optical microscopy, or s-SNOM, which involves shining light onto a metallic tip. The tip acts as an antenna for the light, directing it to a tiny region at its apex just tens of nanometers wide.
This trick is what’s used in IR s-SNOM, where infrared light is coupled to a metallic tip. The challenge with IR s-SNOM, however, is that researchers have been relying on infrared light produced by lasers. Lasers emit a large number of photons needed for the technique, but because they operate in a narrow wavelength band, they can only probe a narrow range of molecular vibrations. In other words, laser light simply can’t give you the flexibility to explore a spectrum of mixed molecules.
A spectral-linescan of a blue mussel shell, which transitions from calcite to aragonite, illustrates the spatial resolution and spectroscopic range capabilities of the SINS technique. The image shows two simultaneously acquired vibrational modes across the transition region.
A spectral-linescan of a blue mussel shell, which transitions from calcite to aragonite, illustrates the spatial resolution and spectroscopic range capabilities of the SINS technique. The image shows two simultaneously acquired vibrational modes across the transition region.
Bechtel, Martin and Raschke’s team saw the opportunity to use Berkeley Lab’s ALS to overcome the laser limitation. The lab’s synchrotron produces broadband infrared light with a high-photon count that can be focused to the diffraction limit. The researchers coupled the synchrotron light to a metallic tip with an apex of about 20 nanometers, focusing the infrared beam onto the samples. The resulting spectrum is analyzed with a modified FTIR instrument.
“This is actually one of very few examples where synchrotron light has been coupled to scanning probe microscopy,” says Raschke. “Moreover, the implementation of the technique at the synchrotron brings chemical nano-spectroscopy and -imaging out of the lab of a few laser science experts and makes it available for a broader scientific community at a user facility.”
From mollusks to moon rocks
The team demonstrated the technique by confirming the spectroscopic signature of silicon dioxide on silicon and by illustrating the sharp chemical transition that occurs within the shells of the blue mussel (M. edulis). Additionally, the researchers looked at proteins and a peptoid nanosheet, an engineered, ultra-thin film of proteins with medical and pharmacological applications.
Martin is excited for the potential of SINS, which is available for researchers from any institution to use. In particular he’s interested in a closer look at battery systems, with the hope that understanding battery chemistry on the mesoscale could provide insight into better performance. Further out, he expects SINS to be useful for a range of biochemistry as well. “This hints at a dream I’ve had in my mind, to look at the surface of a cell, inside the bi-layer membrane, the channels, and receptors,” says Martin. “If we could put a SINS tip on a living cell, we could watch biochemistry happen in real time.”
Berkeley Lab's Michael Martin
Berkeley Lab's Michael Martin
Bechtel, for his part, is intrigued by the possibility of using SINS for the study of lunar rocks, meteorites and stardust. These extraterrestrial materials have a molecular diversity that is difficult to resolve on the nanoscale, particularly in a non-destructive manner for these rare samples. A better understanding of the makeup of moon rocks and dust from space could provide clues to the formation of the planets and solar system.
Raschke is using the technique to study the processes that limit the performance of organic solar cells. He is looking to further improve the flexibility of the technique such that it can be applied under variable and controlled atmospheric and low-temperature conditions. Among other tweaks, he plans to increase the sensitivity of the technique with the ultimate goal of performing singe-molecule chemical spectroscopy.
This research was supported by the DOE Office of Science.
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Lawrence Berkeley National Laboratory addresses the world’s most urgent scientific challenges by advancing sustainable energy, protecting human health, creating new materials, and revealing the origin and fate of the universe. Founded in 1931, Berkeley Lab’s scientific expertise has been recognized with 13 Nobel prizes. The University of California manages Berkeley Lab for the U.S. Department of Energy’s Office of Science. For more, visit www.lbl.gov.
The Advanced Light Source is a third-generation synchrotron light source producing light in the x-ray region of the spectrum that is a billion times brighter than the sun. A DOE national user facility, the ALS attracts scientists from around the world and supports its users in doing outstanding science in a safe environment. For more information visit www-als.lbl.gov.
DOE’s Office of Science is the single largest supporter of basic research in the physical sciences in the United States and is working to address some of the most pressing challenges of our time. For more information, please visit the Office of Science website atscience.energy.gov/.

Tuesday, December 10, 2013

Abstract-Extragalactic Millimeter-wave Point-source Catalog, Number Counts and Statistics from 771 deg2 of the SPT-SZ Survey


L. M. Mocanu1,2, T. M. Crawford1,2, J. D. Vieira3, K. A. Aird4, M. Aravena5,6, J. E. Austermann7, B. A. Benson1,8, M. Béthermin9, L. E. Bleem1,10, M. Bothwell11, J. E. Carlstrom1,2,8,10,12, C. L. Chang1,8,12, S. Chapman13,14, H.-M. Cho15, A. T. Crites1,2, T. de Haan16, M. A. Dobbs16, W. B. Everett7, E. M. George17, N. W. Halverson7, N. Harrington17, Y. Hezaveh16, G. P. Holder16, W. L. Holzapfel17, S. Hoover1,10, J. D. Hrubes4, R. Keisler1,10, L. Knox18, A. T. Lee17,19, E. M. Leitch1,2, M. Lueker3, D. Luong-Van4, D. P. Marrone20, J. J. McMahon21, J. Mehl1,12, S. S. Meyer1,2,8,10, J. J. Mohr22,23,24, T. E. Montroy25, T. Natoli1,10, S. Padin1,2,3, T. Plagge1,2, C. Pryke26, A. Rest27, C. L. Reichardt17, J. E. Ruhl25, J. T. Sayre25, K. K. Schaffer1,8,28, E. Shirokoff17, H. G. Spieler19, J. S. Spilker20, B. Stalder29, Z. Staniszewski25, A. A. Stark29, K. T. Story1,10, E. R. Switzer30, K. Vanderlinde31,32, and R. Williamson1,2

lmocanu@uchicago.edu
1 Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
2 Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637, USA
3 California Institute of Technology, Pasadena, CA 91125, USA
4 University of Chicago, Chicago, IL 60637, USA
5 European Southern Observatory, Alonso de Córdova 3107, Vitacura Santiago, Chile
6 Faculty of Engineering, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile
7 Department of Astrophysical and Planetary Sciences and Department of Physics, University of Colorado, Boulder, CO 80309, USA
8 Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA
9 Laboratoire AIM-Paris-Saclay, CEA/DSM/Irfu-CNRS-Université Paris Diderot, CEA-Saclay, Orme des Merisiers, F-91191 Gif-sur-Yvette, France
10 Department of Physics, University of Chicago, Chicago, IL 60637, USA
11 Cavendish Laboratory, University of Cambridge, 19 J.J. Thomson Avenue, Cambridge CB3 0HE, UK
12 Argonne National Laboratory, Argonne, IL 60439, USA
13 Department of Physics and Atmospheric Science, Dalhousie University, Halifax NS B3H 3J5, Canada
14 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
15 NIST Quantum Devices Group, Boulder, CO 80305, USA
16 Department of Physics, McGill University, Montreal, Quebec H3A 2T8, Canada
17 Department of Physics, University of California, Berkeley, CA 94720, USA
18 Department of Physics, University of California, Davis, CA 95616, USA
19 Physics Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA
20 Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA
21 Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
22 Department of Physics, Ludwig-Maximilians-Universität, D-81679 München, Germany
23 Excellence Cluster Universe, D-85748 Garching, Germany
24 Max-Planck-Institut für extraterrestrische Physik, D-85748 Garching, Germany
25 Physics Department, Center for Education and Research in Cosmology and Astrophysics, Case Western Reserve University, Cleveland, OH 44106, USA
26 Department of Physics, University of Minnesota, Minneapolis, MN 55455, USA
27 Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218, USA
28 Liberal Arts Department, School of the Art Institute of Chicago, Chicago, IL 60603, USA
29 Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
30 Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George St., Toronto, Ontario M5S 3H8, Canada
31 Dunlap Institute for Astronomy & Astrophysics, University of Toronto, 50 St George St, Toronto, Ontario M5S 3H4, Canada
32 Department of Astronomy & Astrophysics, University of Toronto, 50 St George St, Toronto, Ontario M5S 3H4, Canada
 
L. M. Mocanu et al. 2013 ApJ 779 61. doi:10.1088/0004-637X/779/1/61
Received 12 June 2013, accepted for publication 18 October 2013. Published 25 November 2013.
© 2013. The American Astronomical Society. All rights reserved.

Abstract

We present a point-source catalog from 771 deg2 of the South Pole Telescope Sunyaev-Zel'dovich survey at 95, 150, and 220 GHz. We detect 1545 sources above 4.5σ significance in at least one band. Based on their relative brightness between survey bands, we classify the sources into two populations, one dominated by synchrotron emission from active galactic nuclei, and one dominated by thermal emission from dust-enshrouded star-forming galaxies. We find 1238 synchrotron and 307 dusty sources. We cross-match all sources against external catalogs and find 189 unidentified synchrotron sources and 189 unidentified dusty sources. The dusty sources without counterparts are good candidates for high-redshift, strongly lensed submillimeter galaxies. We derive number counts for each population from 1 Jy down to roughly 11, 4, and 11 mJy at 95, 150, and 220 GHz. We compare these counts with galaxy population models and find that none of the models we consider for either population provide a good fit to the measured counts in all three bands. The disparities imply that these measurements will be an important input to the next generation of millimeter-wave extragalactic source population models.

Wednesday, July 3, 2013

Scientists obtain ground-breaking measurements using infrared light

                                CLS Spectroscopist Brant Billinghurst conducts research on the CLS Far-IR
                               beamline. (Photo Courtesy: Canadian Light Source)
My Note: More on the Canadian Light Source synchrotron, which was posted about earlier here:
http://terahertztechnology.blogspot.com/2013/07/scientists-obtain-ground-breaking.html

Research will have implications for synchrotrons around the world
Scientists at the Canadian Light Source (CLS) have obtained high-resolution measurements in the infrared spectrum that could change the way research is conducted using synchrotron light.
CLS Spectroscopist Brant Billinghurst said he and his colleagues were working on methods to produce intense terahertz radiation (at the far end of the infrared spectrum) while conducting research on the Far-IR beamline, an experimental station at the CLS.
The research was recently published under the name “Observation of superradiant synchrotron radiation in the terahertz region” in Physical Review Special Topics – Accelerators and Beams.
Billinghurst said they tried something unusual with the synchrotron that allowed them, for the first time, to make a high-resolution measurement of superradiant synchrotron radiation.
“For this technique to work, you need a synchrotron, electrons in small bunches, and stable beam. So, it’s very specific,” said Billinghurst.
Unlike the high-energy photons needed for experiments using X-rays, the techniques used in the infrared region benefit from turning the synchrotron energy way down, to 1.5 GeV, making it possible for the technique to work.
Billinghurst pointed out that the idea for synchrotron superradiance appears in a definitive textbook, Classical Electrodynamics, by physicist John David Jackson, in 1962, but that no one had actually reported high-resolution results until now.
These findings have some interesting implications and could allow for spectroscopy in the Terahertz region at higher resolution than is currently feasible. This discovery could have implications for research at synchrotrons around the world. However, there are a number of technical issues that would have to be solved before this would be possible, said Billighurst.
The infrared spectrum is used for a number of experiments at the CLS, including better understanding of the materials that compose the universe.
Read the full academic article in Physical Review Special Topics.