Sunday 8 June 2014

New ‘doping’ method improves properties of carbon nanotubes

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Yale University researchers have developed a simple method for controlling the “doping” of carbon nanotubes (CNTs), a chemical process that optimizes the tubes’ properties. Reported April 29 in Nano Letters, the method could improve the utility of doped CNTs in a number of nanotechnologies and flexible electronics, including CNT-silicon hybrid solar energy cells. Led by André Taylor of the Yale School of Engineering & Applied Science and Nilay Hazari of Yale’s chemistry department, the researchers developed a method that uses organic compounds with a metal core — known as metallocenes — to produce two possible types of doped CNTs. A small amount of metallocenes in solution is deposited on the CNTs, which are then rotated at high speed. This simple “spin coating” process spreads the solution evenly across the surface of the CNTs, resulting in high doping levels that can improve electrical utility. Using the method, the researchers found that doping with electron-deficient metallocenes, such as those with a cobalt core, results in CNTs with more positively charged electron “holes” than available negatively charged electrons to fill those holes; these CNTs are known as “p-type” because of their positive charge. On the other hand, doping with electron-rich metallocenes, such as

The post New ‘doping’ method improves properties of carbon nanotubes has been published on Technology Org.

 
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Twitter releasing trove of user data to scientists for research

Science Focus

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Twitter has a 200-million-strong and ever-growing user base that broadcasts 500 million updates daily. It has been lauded for its ability to unsettle repressive political regimes, bring much-needed accountability to corporations that mistreat their customers, and combat other societal ills (whether such characterizations are, in fact, accurate). Now, the company has taken aim at disrupting another important sphere of human society: the scientific research community.

Back in February, the site announced its plan—in collaboration with Gnip—to provide a handful of research institutions with free access to its data sets from 2006 to the present. It's a pilot program called “Twitter Data Grants,” with the hashtag #DataGrants. At the time, Twitter’s engineering blog explained the plan to enlist grant applications to access its treasure trove of user data:

Twitter has an expansive set of data from which we can glean insights and learn about a variety of topics, from health-related information such as when and where the flu may hit to global events like ringing in the new year. To date, it has been challenging for researchers outside the company who are tackling big questions to collaborate with us to access our public, historical data. Our Data Grants program aims to change that by connecting research institutions and academics with the data they need.

In April, Twitter announced that, after reviewing the more than 1,300 proposals submitted from more than 60 different countries, it had selected six institutions to provide with data access. Projects approved included a study of foodborne gastrointestinal illnesses, a study measuring happiness levels in cities based on images shared on Twitter, and a study using geosocial intelligence to model urban flooding in Jakarta, Indonesia. There's even a project exploring the relationship between tweets and sports team performance.

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 » see original post http://feeds.arstechnica.com/~r/arstechnica/science/~3/sC5o5y20Rzk/
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Beyond LHC: Particle physicists explore the potential of more powerful proton colliders

Science Focus

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An international group of about 100 physicists gathered last week for the first formal workshop at SLAC to explore the world of high-energy physics beyond CERN’s Large Hadron Collider, which is famous for unearthing the Higgs boson – and even beyond the International Linear Collider, a facility that hasn’t been built yet. Their focus: a 100 tera-electronvolt (TeV) proton-proton collider about seven times more powerful than the LHC will be when it reaches its maximum energy of 14 TeV in 2015.  Members of the Physics at 100 TeV workshop gather for a photo. (Lori Ann White/SLAC) Getting Ready for the Future “It does seem like a crazy thing to hold a workshop like this when the LHC hasn’t even hit 14 TeV,” said Tim Cohen, a member of the SLAC particle theory group and one of the organizers of the workshop, along with SLAC colleagues Michael Peskin and Jay Wacker and experimentalist Mike Hance from Lawrence Berkeley Lab. “But I think the Snowmass process we went through last summer has the HEP community really looking toward the future.” The Snowmass process refers to a lengthy planning and consensus-building effort by the high-energy physics community that culminated in a week-long meeting, during which

The post Beyond LHC: Particle physicists explore the potential of more powerful proton colliders has been published on Technology Org.

 
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 » see original post http://feedproxy.google.com/~r/TechnologyOrgPhysicsNews/~3/SoZmzIzyyZc/
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Sleep's memory role discovered

Science Focus

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Scientists in China and the US use advanced microscopy to discover exactly how a good night's sleep improves learning and memory. 
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 » see original post http://www.bbc.co.uk/news/health-27695144#sa-ns_mchannel=rss&ns_source=PublicRSS20-sa
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Monogram - Crab Pulsar Time Lapse - Neutron Star Sticker

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tagged with: stars, galaxies, astronomy, envelope sealers, crbplsr, crab pulsar, time lapse astronomy, neutron star, matter and antimatter, near light speed, monogram initials, monograms

Galaxies, Stars and Nebulae series Multiple observations made over several months with NASA's Chandra X-ray Observatory and the Hubble Space Telescope captured the spectacle of matter and antimatter propelled to near the speed of light by the Crab pulsar, a rapidly rotating neutron star the size of Manhattan.

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Image credit: NASA's Chandra X-ray Observatory and the Hubble Space Telescope

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Open Cluster NGC 290: A Stellar Jewel Box

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Surprisingly strong magnetic fields challenge black holes' pull

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A new study of supermassive black holes at the centers of galaxies has found magnetic fields play an impressive role in the systems' dynamics. In fact, in dozens of black holes surveyed, the magnetic field strength matched the force produced by the black holes' powerful gravitational pull, says a team of scientists from the U.S. Department of Energy's Lawrence Berkeley National Laboratory and Max Planck Institute for Radio Astronomy (MPIfR) in Bonn, Germany. The findings are published in this week's issue of Nature.



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Hubble Interacting Galaxy NGC 6786 iPad Case

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Monogram - Stellar Nursery R136, Tarantula Nebula Sticker

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Galaxies, Stars and Nebulae series Hundreds of brilliant blue stars wreathed by warm, glowing clouds in appear in this the most detailed view of the largest stellar nursery in our local galactic neighborhood. The massive, young stellar grouping, called R136, is only a few million years old and resides in the 30 Doradus (or Tarantula) Nebula, a turbulent star-birth region in the Large Magellanic Cloud (LMC), a satellite galaxy of our Milky Way.
There is no known star-forming region in our galaxy as large or as prolific as 30 Doradus. Many of the diamond-like icy blue stars are among the most massive stars known. Several of them are over 100 times more massive than our Sun. These hefty stars are destined to pop off, like a string of firecrackers, as supernovas in a few million years. The image, taken in ultraviolet, visible, and red light by Hubble's Wide Field Camera 3, spans about 100 light-years.
The movement of the LMC around the Milky Way may have triggered the massive cluster's formation in several ways. The gravitational tug of the Milky Way and the companion Small Magellanic Cloud may have compressed gas in the LMC. Also, the pressure resulting from the LMC plowing through the Milky Way's halo may have compressed gas in the satellite. The cluster is a rare, nearby example of the many super star clusters that formed in the distant, early universe, when star birth and galaxy interactions were more frequent.
The LMC is located 170,000 light-years away and is a member of the Local Group of Galaxies, which also includes the Milky Way. The Hubble observations were taken Oct. 20-27, 2009. The blue color is light from the hottest, most massive stars; the green from the glow of oxygen; and the red from fluorescing hydrogen.

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Image credit: Hubble's Wide Field Camera 3

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Boomerang Nebula Wall Graphic

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"The Hubble Space Telescope has "caught" the Boomerang Nebula in these new images taken with the Advanced Camera for Surveys. This reflecting cloud of dust and gas has two nearly symmetric lobes (or cones) of matter that are being ejected from a central star. Over the last 1,500 years, nearly one and a half times the mass of our Sun has been lost by the central star of the Boomerang Nebula in an ejection process known as a bipolar outflow. The nebula's name is derived from its symmetric structure as seen from ground-based telescopes. Hubble's sharp view is able to resolve patterns and ripples in the nebula very close to the central star that are not visible from the ground.

...The Boomerang Nebula is located about 5,000 light-years from Earth in the direction of the Southern constellation Centaurus. Submillimeter radio measurements made in 1995 show the deep interior of the nebula to have a temperature of only one degree Kelvin above absolute zero, with absolute zero equal to nearly -460 degrees Fahrenheit. This makes the inner regions of the Boomerang Nebula one of the coldest known places in the universe."

(qtd. from Hubblesite.org NewsCenter release STScI-2005-25)

Credit: NASA, ESA and The Hubble Heritage Team (STScI/AURA)

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Hubble Sees a Cosmic Caterpillar Cases For iPad

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