Sunday, May 19, 2013

RolePlayGateway?

Welcome to Domus Saltus Mortuus

Your room is right this way...

Didn't mother always tell you to play with your food?

[i] Well, there's no need to tell you we are vampires now, is there? Surely even a human like you has figured that out? Well then, you best come in and let me tell you about our little....arrangement. This is our house, or as we like to call it, Domus Saltus Mortuus. House of the Dead. Yes, yes it's cliche but mother was one for those. Here is our feeding room. Strictly blood giving only. Your cubicle is over there. If one of the vampires come in, you are to sit there and offer up that...thick...warm...mmmm. What was I saying? Oh, your cubicle. Yes, you must behave yourself little darling.

Here is your bedroom. Strictly yours. Vampires won't be able to come in here unless invited. But be warned, once they have been in once, they don't need to be invited again.

And here are the vampire bedrooms. You will be spending a lot of time in here...trust me. It's dark and slightly too cold, but don't worry. We'll keep you warm...

So, let's talk business shall we?

Source: http://feeds.feedburner.com/RolePlayGateway

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Saturday, May 4, 2013

Singer bids tearful farewell to 'American Idol'

TV

13 hours ago

In the final moments of ?American Idol? on Thursday, Kree Harrison and Amber Holcomb stood at the center of the stage, awaiting Ryan Seacrest?s verdict. They knew one would be going home next week to fanfare and a parade, and one would be heading there for good because she was eliminated.

IMAGE: Angie Miller, Kree Harrison, Candice Glover

Getty Images file

Angie Miller, Kree Harrison and Candice Glover are "American Idol's" final three.

Kree looked tense. Amber? She looked resigned.

And she was right. The 18-year-old who had clearly tensed up on Wednesday?s performances was sent packing in the bad kind of way, finishing the season in fourth place. Much like Amber, the judges looked sad, but resigned.

?I never wanted to see it get to this point,? Nicki Minaj said, apparently not understanding that the point of the show is to whittle the number of contenders down each week until only one is left standing.

Though Ryan said the results were in no particular order, ?Idol? set the stage for the Kree-Amber pairing early. Jimmy Iovine?s comments on Wednesday?s performances made it clear where he hoped the night would go.

Jimmy acknowledged that Amber?s first performance was underwhelming, but that she knocked the second song out of the park. ?Was this enough to save her? I don?t know. But I hope so,? he said.

His comments about Kree were less positive. "In my opinion, Kree just hasn't lived up to her full potential over the past two weeks," he said. He admitted that both of her numbers were fine, but said he preferred contestants who alternated brilliance with mediocrity as opposed to those who stayed in the middle of the road.

While that?s his opinion, it wasn?t revealed until long after the voting lines had been closed. And Amber, who came up short in the two-week vote that totaled more than 81 million responses, was so emotionally spent on Wednesday that it might not have mattered.

Amber made sure that everyone would join her in tears at her exit, however, singing ?I Believe in You and Me? as her crying father joined her onstage and gave her a hug.

On the other hand, it was a big night for Candice. She was among the two lowest-vote getters a week ago, but was spared possible elimination when the show decided to bring everyone back. Taking full advantage of the second chance, she excelled in both of her solos and made it clear that she can?t be counted out.

?If I'm Bruno Mars, I go out and write a song for Candice's album right now," Jimmy said after listening to her cover of Mars? ?When I was Your Man.? Candice, who has an intensity onstage unmatched by her rivals, was thrilled to get the good news of her survival, wanting to hug anyone and everyone in her path.

As for Angie, while Jimmy noted that she lost a chance to take the driver?s seat in the competition, she was in no real danger of going home this week.

?It just wasn?t special enough,? he said of her performances. ?But it wasn?t bad enough to send her home.?

Or, rather, it was good enough to send her home in style next week, while Amber couldn?t avoid the more somber journey.

Source: http://www.today.com/entertainment/singer-bids-tearful-farewell-american-idol-6C9753442

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Friday, May 3, 2013

An anarchic region of star formation

May 2, 2013 ? The Danish 1.54-metre telescope located at ESO's La Silla Observatory in Chile has captured a striking image of NGC 6559, an object that showcases the anarchy that reigns when stars form inside an interstellar cloud.

NGC 6559 is a cloud of gas and dust located at a distance of about 5000 light-years from Earth, in the constellation of Sagittarius (The Archer). The glowing region is a relatively small object, just a few light-years across, in contrast to the one hundred light-years and more spanned by its famous neighbour, the Lagoon Nebula (Messier 8, eso0936). Although it is usually overlooked in favour of its distinguished companion, NGC 6559 has the leading role in this new picture.

The gas in the clouds of NGC 6559, mainly hydrogen, is the raw material for star formation. When a region inside this nebula gathers enough matter, it starts to collapse under its own gravity. The centre of the cloud grows ever denser and hotter, until thermonuclear fusion begins and a star is born. The hydrogen atoms combine to form helium atoms, releasing energy that makes the star shine.

These brilliant hot young stars born out of the cloud energise the hydrogen gas still present around them in the nebula [1]. The gas then re-emits this energy, producing the glowing threadlike red cloud seen near the centre of the image. This object is known as an emission nebula.

But NGC 6559 is not just made out of hydrogen gas. It also contains solid particles of dust, made of heavier elements, such as carbon, iron or silicon. The bluish patch next to the red emission nebula shows the light from the recently formed stars being scattered -- reflected in many different directions -- by the microscopic particles in the nebula. Known to astronomers as a reflection nebula, this type of object usually appears blue because the scattering is more efficient for these shorter wavelengths of light [2].

In regions where it is very dense, the dust completely blocks the light behind it, as is the case for the dark isolated patches and sinuous lanes to the bottom left-hand side and right-hand side of the image. To look through the clouds at what lies behind, astronomers would need to observe the nebula using longer wavelengths that would not be absorbed.

The Milky Way fills the background of the image with countless yellowish older stars. Some of them appear fainter and redder because of the dust in NGC 6559.

This eye-catching image of star formation was captured by the Danish Faint Object Spectrograph and Camera (DFOSC) on the 1.54-metre Danish Telescope at La Silla in Chile. This national telescope has been in use at La Silla since 1979 and was recently refurbished to turn it into a remote-controlled state-of-the-art telescope.

Notes

[1] These young stars are usually of spectral type O and B, with temperatures between 10,000 and 60,000 K, which radiate huge amounts of high energy ultraviolet light that ionises the hydrogen atoms.

[2] Rayleigh scattering, named after the British physicist Lord Rayleigh, happens when light is scattered off particles of material that are much smaller than the wavelength of the light. It is much more effective for short wavelengths of light, that is, wavelengths corresponding to the blue end of the visible spectrum, so the result is a bluish diffuse light. This is the same mechanism that explains the blue colour of the daytime cloud-free sky.

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The above story is reprinted from materials provided by European Southern Observatory (ESO).

Note: Materials may be edited for content and length. For further information, please contact the source cited above.


Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.

Source: http://feeds.sciencedaily.com/~r/sciencedaily/most_popular/~3/zRze14ddwwc/130502082252.htm

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How to frustrate a quantum magnet: 16 atomic ions simulate a quantum antiferromagnet

May 3, 2013 ? Frustration crops up throughout nature when conflicting constraints on a physical system compete with one another. The way nature resolves these conflicts often leads to exotic phases of matter that are poorly understood. This week's issue of Science features new results from the research group of Christopher Monroe at the JQI, where they explored how to frustrate a quantum magnet composed of sixteen atomic ions -- to date the largest ensemble of qubits to perform a simulation of quantum matter.

Originating in large part with Richard Feynman's 1982 proposal, quantum simulation has evolved into a field where scientists use a controllable quantum system to study a second, less experimentally feasible quantum phenomenon. In short, a full-scale quantum computer does not yet exist and classical computers often cannot solve quantum problems, thus a "quantum simulator" presents an attractive alternative for gaining insight into the behaviors of complex material. Says Monroe, "With just 30 or so qubits, we should be able to study ordering and dynamics of this many-body system that cannot be predicted using conventional computers. In the future, make that a few hundred qubits and there's simply not enough room in the universe for all the memory required to do the calculation."

In this experiment, JQI physicists engineer a quantum magnet using lasers and ion qubits. The ion trap platform has long been a leader in the field of quantum information and is an ideal playground for quantum simulations (see image 1 in gallery of ion trap used here). Ions are charged particles that interact strongly via the Coulomb force, which is an attraction/repulsion that decreases as particles separate. When a handful of positively charged ytterbium ions are thrown together, they repel each other, and, for this oblong ion trap, form a linear crystal (see gallery image 2 of real camera images of single ions arranged in a crystal). Each ion has two internal energy states that make up a qubit.

Laser beams can manipulate the Coulomb force to create tunable, long range magnetic-like interactions, where each ion qubit represents a tiny magnet*. Imagine that invisible springs connect the ions together. Vibrations occurring on one side of the crystal affect the entire crystal. This is called collective motion and is harnessed to generate a force that depends on how a magnet is oriented (which state the qubit is in). The team can program this state-dependent force by simultaneously applying multiple laser beams, whose colors (frequencies) are specially chosen with respect to the internal vibrations of the ion crystal. The amount of influence each magnet has on the rest of the chain primarily depends on the choice of laser frequencies. The crystal geometry has little to do with the interactions. In fact, for some laser configurations the ions that are farthest apart in space interact most strongly.

Phenomena due to this type of magnet-magnet interaction alone can be explained without quantum physics. An additional uniform magnetic field, (here created with yet another laser beam), is necessary for introducing quantum phase transitions and entanglement. This added magnetic field (oriented perpendicular to the direction of the interactions) induces quantum fluctuations that can drive the system into different energy levels.

In the experiment, the long-range ion-ion interaction and a large effective magnetic field are turned on simultaneously. In the beginning of the simulation the ion magnets are oriented along the direction of the effective magnetic field. In the quantum world, if a magnet is pointing along some direction with certainty, its magnetic state along any perpendicular direction is totally random. Hence the system is in a disordered state along the perpendicular direction of magnetic [spin] interactions.

During the quantum simulation the magnetic field is reduced and the ion crystal goes from being in this disordered state, with each ion magnet pointing along a random direction, to being determined by the form of the magnetic interactions. For some cases of antiferromagnetic (AFM) interactions, the spins will end in a simple up-down-up-down-etc. configuration. With the turn of some knobs, the team can cause the AFM interactions to instead frustrate the crystal. For example, nearest neighbor AFM interactions can compete strongly with the next-nearest neighbor interactions and even the next-next-nearest neighbor constraints. The crystal can easily form various antiferromagnetic combinations, instead of the simple nearest neighbor antiferromagnet (up down up down). In fact, with a few technical upgrades, the researchers can potentially engineer situations where the magnets can reside in an exponentially large number of antiferromagnetic states, generating massive quantum entanglement that accompanies this frustration.

Previously, this same group of researchers performed quantum simulations of a ferromagnet (all magnets oriented same direction) and of the smallest system exhibiting frustration. Their ability to utilize the collective motion allows them to explore different facets of quantum magnetism. The team can 'at will' modify how the different collective modes contribute to magnetic order by merely changing the laser colors and/or the ion separation. This new work demonstrates the versatility of their system, even as particles are added. As lead author Dr. Rajibul Islam explains "We have a knob that adjusts the range of the interaction, something that is unavailable in real materials. This type of simulation could therefore help in the design of new types of materials that possess exotic properties, with potential applications to electrical transport, sensors, or transducers."

*Physicists use mathematical spin models, such as the Ising model studied here, to understand quantum magnets, thus in this news article, for clarity the ions are called "magnets." In the language of the Science Magazine article, they are called "spins."

Frequency Information

This experiment is all about frequency. The ions themselves are vibrating at a frequency determined by an electrostatic trap--about 1 MHz or 1 million vibrations/second. The ion qubit is made from two internal energy levels that are separated in frequency by about 12 GHz or 12 billion vibrations/second (microwave domain). When radiation with a frequency that matches either of these frequencies shines onto the ion, then the radiation is said to be in resonance with that transition. For example, 12 GHz microwave radiation will make the ion qubit cycle between two internal states. If MHz radiation is coupled to the ion, it will begin vibrating. In the quantum regime, the quanta of vibration called a phonon can be controllably added and removed from the system. These phonons act as communication channels for the magnets, and are instrumental in generating rich varieties of interactions.

Scientists must be clever about generating frequencies. We are constantly being bathed in radiation from cellphones (GHz), infrared (terahertz or 1000 GHz), UV radiation (petahertz or 1 million GHz), and more--much of this goes unnoticed. The ion here is sensitive to only very precise frequencies. To get that qubit to flip flop between two qubit states, they need to apply a radiation at precisely 12.642819 GHz. To create spin-spin interactions, they also need to simultaneously excite its motion--it is vibrating at a frequency that is 10,000 times smaller. Lasers are the key--here at 369 nm, just barely in the ultraviolet regime. Previously, a JQI news item described how they can use a pulsed laser to generate 12.642819 GHz. Scientists control the frequency, power and the direction of light waves very precisely by hitting the laser beams with sound waves and oscillating electric fields (in devices such as the acousto- and electro-optic modulators). These devices act to add lower frequencies necessary for exciting the motion in the trap as well as fine tune the main laser beam to address certain atomic transitions. This method, called modulation, is versatile and is one of the key features that make this and other quantum physics experiments possible.

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The above story is reprinted from materials provided by Joint Quantum Institute, University of Maryland.

Note: Materials may be edited for content and length. For further information, please contact the source cited above.


Journal Reference:

  1. R. Islam, C. Senko, W. C. Campbell, S. Korenblit, J. Smith, A. Lee, E. E. Edwards, C.- C. J. Wang, J. K. Freericks, C. Monroe. Emergence and Frustration of Magnetism with Variable-Range Interactions in a Quantum Simulator. Science, 2013; 340 (6132): 583 DOI: 10.1126/science.1232296

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.

Source: http://feeds.sciencedaily.com/~r/sciencedaily/top_news/top_science/~3/3CQ9yU-Wkjw/130503105041.htm

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Van Gogh Museum reopens with display on his craft

(AP) ? The Van Gogh Museum in Amsterdam has reopened its doors to the public after a seven-month renovation, kicking off with "Vincent At Work," an exhibition that shows Van Gogh's working methods, right down to the paints, brushes and other tools he used.

Appropriately, the final painting curators hung Wednesday was a self-portrait in which Van Gogh painted himself behind a canvas, brushes and palette in hand.

Another highlight is the display of two versions of Van Gogh's famed yellow "Sunflowers" on either side of the green-dominated portrait "La Berceuse." In a surviving letter, Van Gogh indicated he intended the paintings, which usually hang in three different museums, to be displayed that way.

All three of Amsterdam's biggest art museums have now reopened after major renovations.

Associated Press

Source: http://hosted2.ap.org/APDEFAULT/4e67281c3f754d0696fbfdee0f3f1469/Article_2013-05-01-Netherlands-Van%20Gogh/id-3f5600b328b34a52baa3c306ba95c094

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Thursday, May 2, 2013

Kurtz leaves DailyBeast after retracted blog post

FILE - This April 25, 2012 file photo shows journalist Howard Kurtz at the world premiere of "Knife Fight" during the 2012 Tribeca Film Festival in New York. Kurtz has left online news and commentary site The Daily Beast, a day after the website retracted one of his blog posts about the coming out of NBA player Jason Collins. Both Kurtz and Daily Beast editor-in-chief Tina Brown confirmed his departure over Twitter. Kurtz did not acknowledge any link between the retraction and his departure. He tweeted that ?we began to move in different directions, both sides agreed it was best to part company.? (AP Photo/Evan Agostini, file)

FILE - This April 25, 2012 file photo shows journalist Howard Kurtz at the world premiere of "Knife Fight" during the 2012 Tribeca Film Festival in New York. Kurtz has left online news and commentary site The Daily Beast, a day after the website retracted one of his blog posts about the coming out of NBA player Jason Collins. Both Kurtz and Daily Beast editor-in-chief Tina Brown confirmed his departure over Twitter. Kurtz did not acknowledge any link between the retraction and his departure. He tweeted that ?we began to move in different directions, both sides agreed it was best to part company.? (AP Photo/Evan Agostini, file)

FILE - This April 25, 2012 file photo shows journalist Howard Kurtz at the world premiere of "Knife Fight" during the 2012 Tribeca Film Festival in New York. Kurtz has left online news and commentary site The Daily Beast, a day after the website retracted one of his blog posts about the coming out of NBA player Jason Collins. Both Kurtz and Daily Beast editor-in-chief Tina Brown confirmed his departure over Twitter. Kurtz did not acknowledge any link between the retraction and his departure. He tweeted that ?we began to move in different directions, both sides agreed it was best to part company.? (AP Photo/Evan Agostini, file)

(AP) ? Columnist Howard Kurtz left The Daily Beast on Thursday, a day after the website retracted one of his blog posts about the coming out of NBA player Jason Collins.

Both Kurtz and Daily Beast editor-in-chief Tina Brown confirmed his departure over Twitter.

Kurtz did not acknowledge any link between the retraction and his departure.

He tweeted that "as we began to move in different directions, both sides agreed it was best to part company."

He added that "this was in the works for some time" and that it was time for him to "move on to other opportunities."

In the retracted post, Kurtz says Collins didn't "come clean" about the fact that he was engaged to be married to a woman before declaring he was gay.

But Collins does just that in the Sports Illustrated piece that came out Monday.

Brown tweeted simply that Kurtz and The Daily Beast had "parted company ... we wish him well."

Kurtz, The Washington Post's former media columnist, is also the host of CNN's "Reliable Sources." CNN did not immediately respond to a request for comment.

Kurtz and a spokesman for The Daily Beast also did not immediately respond to requests for comment.

Associated Press

Source: http://hosted2.ap.org/APDEFAULT/495d344a0d10421e9baa8ee77029cfbd/Article_2013-05-02-DailyBeast-Kurtz/id-45e63400d7ce4ec3a3631e4d461b208c

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Wingnut Persecution Complex of the Day: The Military Is Threatening to Court Martial Christians! (Little green footballs)

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Canada Launches Space Robot-Themed $5 Bill with Astronaut's Help

The Bank of Canada had appropriate help Tuesday (April 30) launching its new space-themed $5 bill ? the Canadian commander of the International Space Station (ISS).

"Let me show you an example of how we can reach new heights of innovation," Canadian Space Agency astronaut and Expedition 35 commander Chris Hadfield said, while revealing the astronaut- and robot-arm-adorned bank note from on board the orbiting complex.

Hadfield held up the new blue-color note and let it float in front of him during a live broadcast from the space station. [Chris Hadfield's Video Guide to Life in Space]

According to the Bank of Canada, the new $5 bill features "leading-edge security features" as already present in the $20, $50 and $100 polymer notes now in circulation. The bank also released its new $10 note today, which depicts a Canadian train.

"The polymer series notes are at the frontier of bank note technology. The new $5 and $10 bank notes depict the frontiers of our country and our planet," Bank of Canada Governor Mark Carney said. "It is fitting that we are today crossing the final frontier for a world first ? the unveiling of a bank note from space."

The new bills include transparent and holographic design elements, making them part of the most secure bank note series ever issued by the Bank of Canada. The polymer series is also described as more economical, lasting at least two and half times longer than cotton-based paper notes, and they will be recycled in Canada.

The Bank of Canada's new $5 bank note features a space-theme with the Canadarm2 robotic arm, Dextre manipulator and a spacewalking astronaut.
CREDIT: Bank of Canada/collectSPACE.com

The new $5 bill, as revealed by Hadfield, features images of the Canadian-built Canadarm2 and Dextre, robotic arms and manipulators that were used to build and now maintain the space station. They symbolize Canada's ongoing contribution to the international space program.

Hadfield, who in 2001 became the first Canadian to walk in space while helping to install the Canadarm2 outside the space station, said he tries to inspire young Canadians to aim high.

"This new $5 bill should do the same," he said. "By giving prominence to Canadian achievements in space, this bank note reminds us that not even the sky is the limit."

The note's design also includes a spacewalking astronaut, though the Bank of Canada did not specify if it was meant to be Hadfield. The astronaut can be identified though, as a Canadian by the country's red and white, maple-leaf flag appearing on the arm of the spacesuited figure.

The front of the new $5 bank note features a portrait of Sir Wilfrid Laurier, the Prime Minister of Canada from 1896 to 1911. The previous $5 bill, still in circulation, also features Laurier on one side. The reverse depicts children engaged in winter sports, including sledding and hockey.

The Bank of Canada's new space-themed $5 note is a safer kind of dollar. From left to right: David Saint-Jacques, Canadian Astronaut; the Honourable Jim Flaherty, Minister of Finance; Mark Carney, Governor of the Bank of Canada; Paul G. Smith, Chairman of the Board of Directors of VIA Rail Canada.
CREDIT: Bank of Canada

The $5 bill is the lowest denomination bank note circulated in Canada. The new space-themed bill will be available to the public starting in November.

This is not the first time that Hadfield has been included in the release of Canadian money. The Royal Canadian Mint released coins in 2006 that featured the Canadarm2 and a portrait of the record-setting astronaut. The silver and gold coins carried a face value of $30 and $300, respectively.

In addition to the Canadarm2 and the two-armed Dextre (the latter also known as the Special Purpose Dexterous Manipulator), Canada's space achievements also include the Canadarm, the robotic arm flown on board the now-retired space shuttle.

The first Canadarm flown in space was returned by NASA to Canada last year to go on public display at the Canada Aviation and Space Museum in Ottawa.

Click through to collectSPACE.com to watch video of astronaut Chris Hadfield revealing the new Canadian $5 bank note from on board the International Space Station.

Follow collectSPACE.com on Facebook and on Twitter at @collectSPACE. Copyright 2013 collectSPACE.com. All rights reserved.

Source: http://www.space.com/20908-canada-launches-space-money-astronaut.html

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Zuckerberg Group Faces Liberal Ire (ABC News)

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Wednesday, May 1, 2013

Supernova Remnant SNR 0519: Deep Space Explosion Photo Shows Ghostly Remains Of White Dwarf Star

The "thin, blood-red shells" of gas in this amazing deep-space image are SNR 0519, the remains of a sun-like star that exploded in a supernova about 600 years ago.

This photo of the supernova remnant, which is located about 150,000 light years from Earth in the southern constellation Dorado, was taken by the Hubble Space Telescope and released April 29.

Get larger sizes here
super nova remnant

Supernovae are brilliant explosions that occur at the end of some stars' lives, and they come in two main types. Type I supernovae occur in binary (two-star) systems, when a white dwarf draws mass out of its companion star until the dwarf reaches a critical mass and explodes. In Type II supernovae, a star runs out of nuclear fuel, collapses under its own gravity, implodes and ejects its stellar material into space.

Based on the electromagnetic radiation it emits, scientists think SNR 0519 is the remnant of a type I supernova.

The remnants of some large stars that go supernova can form black holes as they collapse.

A version of the image was submitted to the Hubble Telescope's Hidden Photo Treasures contest last year and won sixth place.

Also on HuffPost:

Source: http://www.huffingtonpost.com/2013/05/01/supernova-remnant-0519-photo-white-dwarf-star_n_3186842.html

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