Stressed-out laser diode may deliver 200Gb/s data rates

https://arstechnica.com/?p=1488883

Laser beams illuminating unit of Diode Pumped Green Laser.
Enlarge /

Laser beams illuminating unit of Diode Pumped Green Laser.

Forrest Anderson | The LIFE Images Collection | Getty Images

The data usage of the modern world is absolutely mind-boggling. We have giant, air-conditioned buildings dedicated to shuffling bits around at high speed. And for what? To ensure that Instagram can tell Facebook to tell its advertisers that you really love rubber duckies.

Vicious truth-telling aside, the infrastructure underlying data centers is based on lasers that are modulated at high speed. Thanks to some recently published research, however, the latest and greatest of the hardware currently in our data centers will start to look very slow. A speed-up of about a factor of 10 may be just around the corner.

Birefringence is your friend

It turns out that the key to making a laser go faster is to make it a bit shoddy. Let’s break that down.

To transfer information, it’s common to modulate the brightness of the laser light. For a laser diode, this is done by varying the electrical current supplied to the diode. But it doesn’t matter how quickly you can vary the current; the laser will respond in its own sweet time. Overcoming that limitation traditionally involves turning the power up, but this new approach avoids that requirement.

To understand this idea, we need to review several concepts. So buckle up and prepare to ride Chris’ concept rollercoaster.

The lasers in telecommunications are made from semiconductor crystals. The speed at which light travels through a material is modified by the material’s refractive index. Air has a refractive index that is just a whisker over one. Glass is about 1.3, and semiconductors are typically around three to four. That means the speed of light slows down by a factor of three to four, while the wavelength contracts by the same factor.

However, crystals are not perfect. They often have strain that distorts the crystal structure. This means that an electric field along one direction will experience a slightly different refractive index compared to an electric field that is rotated 90 degrees. And photons have electric fields.

Imagine two photons traveling together through our strained semiconductor. One has its electric field oriented horizontally, and the other vertically. They start out perfectly synchronized with each other, but after a short distance they are no longer in sync because one photon is traveling slightly slower than the other. From the perspective of a viewer looking down the barrel of the photon gun, the electric field appears to trace out an ellipse.

If we pass a stream of photons through a polarization filter, which blocks certain orientations, the intensity of the output beam will fluctuate as the electric field traces this ellipse. The rate of fluctuation—how quickly the ellipse gets traced—depends on the difference in refractive index for horizontal and vertically polarized photons (called birefringence). The bigger the difference, the faster the fluctuations.

This has been known for a long time and is generally considered an annoyance. But remember, fluctuations in brightness can be used to carry data; the question here is whether we can turn this annoyance into something useful.

Electrons have polarization, too

To use this system to carry information, we need to control the rotation of the ellipse. That means controlling the number of photons in each polarization.

The polarization of light that is emitted by an electron in a laser diode is given by the change in spin as the electron loses energy. So an electron enters the diode spin up, emits a photon, loses energy, and flips to spin down. Likewise, a photon that enters the diode spin down will emit a photon, lose energy, and flip to spin up. The balance between spin-up and spin-down electrons determines the polarization of the emitted light.

To encode information, the balance between spin-up and spin-down electrons that enter the laser diode should change: say from 75:25 for a logical one to 25:75 for a logical zero. The resulting light polarization would fluctuate as fast as we can switch between these two balance of spins in the electron current to the laser diode.

Therein lies the next problem. The electrons don’t immediately lose their energy. Instead, many of them hang around awaiting inspiration before doing so. These tardy electrons smear out the sharp modulation that we put into the laser, and this limits the data transfer rate to speeds that we can already achieve with current technology. Hence, we might put in a stream of electrons that are all spin up. A few of them emit immediately, but the rest first bounce around losing their spin orientation before they emit. The result is a background of light that contains no information, and, on top of that, weak flashes that carry information.

To get higher speeds and clear signals, we need to force the electrons to lose their spin orientation very quickly. This happens naturally when the electrons bounce off the imperfections in the crystal.

The need for speed

To get things to flip spin quickly, the researchers used a laser diode that was… a bit poor. The time that a spin-polarized current would stay polarized was really small, meaning that spin flips happen quickly. The researchers attached the laser diode to a cantilever and bent the cantilever. That stressed the laser diode along one direction, changing its refractive index drastically.

The researchers showed that they could drive intensity oscillations at up to 200GHz, which is an order of magnitude better than previous results.

Sending information is another story, though; the researchers couldn’t directly test that. Instead, they used their experimental data to model the laser. With that model, they could see how changing the spin orientation of the injected electrons would change the output of the laser. They showed that for modulation speeds up to 200GHz, information was encoded—in the words of telecommunications engineers everywhere, the eyes were open.

This research will revolutionize short-distance network traffic. Not only do data rates go up, but energy per bit goes down by over an order of magnitude. There is, however, a small issue. At the moment, I don’t think there is a single device on the planet that can modulate the spin orientation of an electric current at 200GHz. Photodetectors at the receiver may also need some attention. But those developments are only a matter of time once the underlying technology is available.

Nature, 2019, DOI: 10.1038/s41586-019-1073-y (About DOIs)

via Ars Technica https://arstechnica.com

April 12, 2019 at 10:17AM

Sony’s Giant 17-foot tall 16K UHD TV Needs a BIG Room

https://www.legitreviews.com/sonys-giant-17-foot-tall-16k-uhd-tv-needs-a-big-room_211395

Posted by

Shane McGlaun |

Fri, Apr 12, 2019 – 8:02 AM

I’m all for big TVs, the bigger the screen, the better. In fact, given the space and inclination, I’d go all-in on a projector instead of a TV. Sony has a new UHD TV that is the biggest we’ve ever seen. The giant MicroLED display is 17-feet high and 63-feet long.

That is about the size of a bus. I want to play Red Dead Redemption 2 on it. The tech inside the TV is called Crystal LED, and it has 16k screen resolution. That’s a lot.

That resolution gives 16 times the pixels you will find in a typical 4K UHD display. The giant screen isn’t a single massive screen; rather it is a bunch of bezel-free panels put together.

From a distance in photos, you can’t tell there are seams, but it’s not clear if you can tell up close. Screens like this are expected to replace the projector and silver screen at movie theaters one day reports Maxim.

via Legit Reviews Hardware Articles http://bit.ly/2BUcaU4

April 12, 2019 at 08:08AM

One Falcon Heavy rocket launched, three Falcon cores landed.

https://arstechnica.com/?p=1489733

The Falcon Heavy rocket, at sunset along the Florida coast.
Enlarge /

The Falcon Heavy rocket, at sunset along the Florida coast.

Trevor Mahlmann for Ars Technica

On Wednesday evening, SpaceX ended its first attempt to fly the Falcon Heavy rocket and its Arabsat-6A payload in the middle of a two-hour launch window. The upper-level wind shear was unacceptable, and with a poor forecast, it just didn’t make sense to load kerosene and oxygen on the rocket.

Now, the rocket is back on the launch pad for another attempt Thursday, with a similar launch window, opening at 6:35pm ET (10:35 UTC) and closing at 8:31pm ET (00:31 UTC). The upper-level wind forecast for this evening is considerably better.

This will be the Falcon Heavy rocket’s second flight, following a successful first launch in February 2018, during which the company famously flung Elon Musk’s cherry red Tesla Roadster into deep space. Starman is still out there, by the way, in an elliptical orbit around the Sun. Earth-based telescopes may be able to see him in the early 2020s, certainly no later than 2047.

Although the Falcon Heavy has proven itself flight-worthy, this is still just the second launch of a rocket with a staggering 27 engines, so there is definitely some uncertainty. Although SpaceX has made “many good design improvements” from the rocket that launched 14 months ago, Musk said there is a 5 to 10 percent chance of failure with this mission.

Ahead of Thursday’s launch attempt, the company said the rocket—composed of three Falcon 9, Block 5 cores—remains in good condition. Each of the three cores is new, and SpaceX is counting on re-using the two side boosters for another Falcon Heavy mission as early as June—the launch of the US Air Force’s Space Test Program-2 mission carrying several military and scientific research satellites.

To facilitate this, the two side boosters will attempt to land back at SpaceX’s Landing Zones 1 and 2 at Cape Canaveral Air Force Station, while the center core will attempt to land on the Of Course I Still Love You drone ship in the Atlantic Ocean. During the rocket’s first launch in 2018, the side boosters made it, but the center core missed its drone ship landing.

The webcast should begin about 20 minutes before the rocket’s anticipated liftoff. It will include coverage of the landing attempts and satellite deploy.

Falcon Heavy Arabsat-6A mission.

via Ars Technica https://arstechnica.com

April 11, 2019 at 04:11PM

Disney Streaming Service: Release Date, Original Series, Price and More!

https://www.geeksaresexy.net/2019/04/12/disney-streaming-service-release-date-original-series-price-and-more/

Disney Streaming Service: Release Date, Original Series, Price and More!

We can now expect the new Disney streaming service to be launched November 12th. With upcoming exclusive products such as Star Wars: The Mandalorian, Marvel spin-off series featuring Hawkeye, Loki and Scarlet Witch and behind the scene End Game clips, Disney will be hitting hard on the streaming market with this new channel. And don’t forget they now control Hulu.

At launch, the service will include all Marvel movies, everything Star Wars, 400 library movie titles, 25 original series, 100 recent blockbusters, 30 seasons of The Simpsons, and all the Disney classics from the past.

So get ready: Disney, Marvel, Lucasfilm, Pixar and National Georaphic all bundled up for only $6.99 a month.

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via [Geeks Are Sexy] Technology News http://bit.ly/23BIq6h

April 12, 2019 at 08:00AM