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Showing posts with label Space News. Show all posts
Showing posts with label Space News. Show all posts

Saturday, July 9, 2016

A newfound alien planet is bullied by three suns


A newly discovered alien world has three masters.




The planet — which is about four times more massive than Jupiter and located about 340 light-years from Earth — orbits the brightest star in a three-star system.
The two other stars in the system also orbit the brightest star, circling one another like a dumbbell and exerting their gravitational influence over the planet, named HD 131399Ab.
"For about half of the planet's orbit, which lasts 550 Earth-years, three stars are visible in the sky," Kevin Wagner, the lead author of a study in the journal Science detailing the new finding, said in a statement. He added:
For much of the planet’s year the stars appear close together, giving it a familiar night-side and day-side with a unique triple-sunset and sunrise each day. As the planet orbits and the stars grow farther apart each day, they reach a point where the setting of one coincides with the rising of the other — at which point the planet is in near-constant daytime for about one-quarter of its orbit, or roughly 140 Earth-years.
Is it stable?
According to the study, HD 131399Ab's orbit brings it billions of miles away from its host star. The equivalent in our solar system would be a planet twice as far as Pluto from our sun.
HD 131399Ab also seems to have a tenuous hold on its orbit.
"If the planet was further away from the most massive star in the system, it would be kicked out of the system," Daniel Apai, a co-author of the study said in a statement.
Apai added that computer simulations show that this world could have been kicked out of its orbit if the star system changed just slightly.
Even still, it isn't a sure thing that the world will be in a stable orbit forever.
"It is not clear that the planet's orbit is stable over long periods of time, so it might be that we are catching this system in a special state in which the planet hasn't yet been ejected from the system,"
The planet and its stars are also unique in its own right,
"This system is surprising in that it is a planet found in a stellar system containing three stars, and in which all three stars exert a strong gravitational influence on the planet."
How to photograph a planet
HD 131399Ab was discovered with the Very Large Telescope in Chile by taking photos of the star system in infrared light.
Most methods for finding exoplanets — planets outside of our solar system — are more indirect, either hinging upon detecting minute dips in a star's light as a planet moves across its face, or watching for a "wobble" in a star produced by the gravitational tug of a large planet.
But this world was found using a "direct imaging" technique, which lets scientists literally "take a picture of a planetary system and study the light emerging from an exoplanet independent of its host star," Johnson said.
"High-contrast imaging surveys like this one are the only means of discovering planets in wide orbits around their stars, where wide is further away from the central star than Saturn is from the sun," Johnson added.
This world isn't the only planet found in multi-star systems.
Scientists have also found exoplanets in star systems boast two stars — colloquially known as "Tatooine" planets after Luke Skywalker's home world in Star Wars — and other planets have been found in three-star systems.
Researchers are particularly interested in learning more about these kinds of planetary systems to figure out exactly how uncommon they are.
"I think the next step is a dedicated imaging survey around multi-star systems to see if this type of system is a class of astronomical objects, or an aberration," Johnson said.
https://www.youtube.com/watch?v=OM22kY4SguM
http://science.sciencemag.org/…/…/2016/07/06/science.aaf9671
http://www.nasa.gov/…/20…/newly-discovered-planet-has-3-suns
http://mashable.com/…/alien-planet-found-in-three-star-sy…/…
http://www.eurekalert.org/pub_rel…/2016-07/uoa-ndp070116.php
http://mashable.com/2012/10/16/ph1-tatooine-planet/…

Cecile G. Tamura

Tuesday, June 21, 2016

சமஸ்கிருத‬ வானியல் நூல் ஆர்யபட்டீயம் ஜோதிடவியலின் வளர்ச்சி

இந்தியாவில் 5ம் நூற்றாண்டில் வாழ்ந்தஆர்யபட்டர்‬ எழுதிய சமஸ்கிருத‬ நூல் ஆர்யபட்டீயம்.
மேலை நாட்டு வானியல் விஞ்ஞானிகளை அதிர வைத்த
வானியல் நூல் இது!
கிரகணத்துக்கான காரணத்தை ஆர்யப்பட்டர் தனது நூலில் மிகத் தெளிவாக விளக்கி இருந்தார்.
"சடயாஷ்டி சசி சூர்யம் சகினாம் மகதிக பூசார்ய..........................."
நூல்; ஆர்யப்பட்டம் கோல் பாதம் சுலோகம் 39
இதன் பொருள்:

சூரியன் சந்திரனை மறைக்கும் போது சூரிய கிரகணம் தோன்றுகின்றது..
பூமி சந்திரனை மறைக்கும் போது சந்திரகிரகணம் தோன்றுகின்றது.
மேலும்,
அவர் கிரகணங்கள் எப்போதெல்லாம் தோன்றும் என்றும் பூமி சூரியனை சுற்ற 365 நாட்கள் 12 மணித்தியாலங்கள் 30 வினாடிகள் செல்லும் என்றும்,
பூமி தன்னத்தானே சுற்ற 23 மணித்தியாலங்கள் 56 நிமிடம் 4.1 வினாடி செல்லும் எனவும் அப்போதே துல்லியமாக கூறிவிட்டார்.!!

கணித மேதையாகவும்,வானியல் விஞ்ஞானியாகவும்
விளங்கிய இவரே பூஜ்ஜியத்தை(zero) கண்டறிந்தவர்!

இவரது பெயரையே இந்தியாவின் முதல் செயற்கைக்கோளுக்கு வைக்கப் பட்டுள்ளது(ஆரியபட்டா)
ஆரிய பட்டீயம் போன்ற பல அறிவியல் சமஸ்கிருத நூல்கள் உலகப் பல்கலைக்கழகங்களில் கற்பிக்கப் படுகிறது.பாதுகாக்கப் படுகிறது.ஆனால் இங்கு?

ஜோதிடவியலின் பதினெட்டு மூலகர்த்தாக்களான,முனிவர்கள் அதன் வளர்ச்சிக்கும் பாடுபட்டவர்கள் ஆவர். அவர்கள் சூரிய, பிதாமக, வியாஸ, வசிஷ்ட, அத்ரி, பராசர, கஸ்யப, நாரத, கர்க, மரீசி, மனு, ஆங்கிரஸ, லோமச,  பௌலிச, ஸ்யவன,  யவன, பிருகு மற்றும் சௌனக ஆகிய ஒவ்வொருவரும் ஒவ்வொரு சித்தாந்ததை எழுதியுள்ளனர்.

இவர்களுக்குப்பின் பிருகு முனிவர், பிருகஸ்பதி,  பத்தராயணர், கபிலர், கஷ்யபர்,  மனு, மகரிஷி பராசரா, சதயாச்சார்யா, வராகிமிஹிரா, படோத்பவா,  வராஹிமிகிரரின் புதல்வர் பிருத்யுயசா, வைத்தியநாத தீட்சிதர், உத்திரகாலாமிர்தம்  எழுதிய  காளிதாசர்,  ஜாதகதத்வா   எழுதிய மகாதேவா, இன்னும் எத்தனையோ மகாமுனிகள், அறிஞர்கள், இந்திய ஜோதிட முன்னேற்றத்துக்குத் தங்கள் சேவையையும், பங்களிப்பையும் வாரி வழங்கியவர்கள் ஆவர்.

                மகரிஷி பராசரர் : இந்திய ஜோதிடத்தின் தந்தை எனப் பலராலும் புகழப்பட்டவர்.இவர் படைத்த மிகப் பெரிய ஜோதிடநூல்”பிருஹத் பராசர ஹோரா சாஸ்த்ரா” ஆகும்.

                மகரிஷி ஜெய்மினி : இவர் “வியாச மகரிஷி”யின் பிரதான சீடர்.இவர் தனது குரு வியாசரை “பத்ராயணர்” என குறிப்பிடுகிறார்.

இவரது சூத்திரங்களில்,ருத்ராம்சம், சஸ்த்தாம்சம்,சப்தாம்சம் மட்டுமின்றி இலக்னம் மற்றும் யோகங்கள் இணைக்கப்பட்டுள்ளன..

                ஆர்யபட்டா : வானியல் சாஸ்த்திரத்திலும்,கணிதத்திலும் சிறந்து விளங்கியவர்.பாடலிபுத்திரம் அருகே அஷ்மாக் என்ற கிராமத்தில் பிறந்தவர்.தனது பள்ளிப்படிப்பை குஷ்மபுராவில் முடித்தார்.

ஆர்யபட்டீயம்,ஆர்யபட்டா சித்தாந்தம் ஆகியவை இவரின் மிகச்சிறந்த படைப்புகளாகும்.

                வராஹிமிகிரர் :இவர் இந்திய வானியல்வலலுனர் ,கணிதமேதை மற்றும் ஜோதிடமேதையும் ஆவார்.

இவர் உஜ்ஜெய்னியில் பிறந்தவர்.ஐந்து வானியல் கணிதம் சம்பந்தமான நூல்களான சூர்யசித்தாந்தம்,ரோமகசித்தாந்தம்,பௌலிசசித்தாந்தம்,வசிஷ்டசித்தாந்தம், மற்றும் பிதாமகசித்தாந்தம் ஆகியவற்றின் சாரமே இவரின் பஞ்சசித்தாந்திகா சிறந்த நூலாகும்.

கலைக்களஞ்சியம் என பெயர பெற்றது இவரது பிருகத் சம்கிதா வாகும். இவரது புதல்வர் பிருத்யுயசாவின் ஜோதிடஉலகுக்கான பங்களிப்புத்தான் ஹோரா சாரா. தனது தந்தையின் நூல்களுக்கு மிகச் சிறந்த விளக்கங்களை அளித்துள்ளார்.வராகிமிகிரர்,கோள்கள் நீள்வட்டப் பாதையில் சூரியனைச் சுற்றிவருவதையும்,சூரியனுக்கு மிக அருகிலுள்ள கிரகங்கள் மிக வேகமாகச் சுற்றுவதையும், தூரத்திலிருக்கும் கிரகங்கள் மெதுவாகச் செல்வதையும் கேப்லருக்கு முன்னரே அறிந்திருந்தார் என சொல்லப்படுகிறது.

                இவர்களைத் தவிரவும்,முதலாவது பாஸ்கரா,இரண்டாவது பாஸ்கரா,லல்லா,வடேஸ்வரா,வீரசேனா,ஜெயதேவா, ஆரியபட்டா ஒனறு/இரண்டு ,ஸ்ரீ பதிஎன  வானியல்,கணிதம்,ஜோதிடத்தின் வளர்ச்சிக்காக பாடுபட்டவர்கள் ஏராளம் இவ்வாறாக ஜோதிட வரலாற்றை எழுதிக் கொண்டே போகலாம். விரிவஞ்சி இத்துடன் முடித்துக் கொள்ளலாம்.. நன்றி-முகநூல் ஹிந்து மீடியா

Monday, June 20, 2016

Galaxies












Thanks to the Hubble Telescope, we know definitively that galaxies come in many various shapes and sizes. Many of the objects we thought were planetary nebula, when seen from Earth based telescopes, have now been proven to be galaxies and interacting galaxies. In fact, it is almost impossible to view an image made with the Hubble space telescope without also seeing numerous galaxies in the background.
Most galaxies come in four basic types: spiral, barred-spiral, elliptical, and irregular. There are also globular clusters and lenticular types and the rarer ring type. Galaxies also come in three size classes: dwarf, galaxy, and giant. Virtually all galaxies fall into the Hubble Classification Scheme created by Edwin Hubble in first half of the 20th century. The original was dubbed the "tuning fork" diagram, but it has since been updated and revised. The below images show the original and updated versions.
Spiral and Barred-Spiral Galaxies
This is the common form of galaxy. It is also the shape we tend to think of when we think "galaxy." They have a round, spheroidal core surrounded by the classic "pinwheel" with at least two arms, but most often have more. The core can actually resemble an elliptical galaxy and contains the metal-poor stars found in elliptical galaxies. Thus, the core stars can have a distinct yellowish to whitish tint, where the arms will have a bluish-white tint due to the younger stars that can be found there due to the rich star-breeding grounds of large dust and gas clouds like the Orion Nebula. The arms can be loosely or tightly packed, intact or patchy, closely or loosely wound. Barred-spirals will tend to have arms that are more loosely wound than in a spiral galaxy. Although it may appear to be so, the space between galaxy arms is far from empty and can have healthy star-breeding grounds. In fact, our stellar system is situated on the inner side of the Orion Spur.
Ring Galaxies
Ring galaxies were perhaps spiral or barred-spiral before colliding with another galaxy. These are the rarest of all galaxies. So far, we have only found 43 ring galaxies out of the few billions of galaxies discovered. This works out to about 1 in 65,000,000 galaxies being a ring galaxy. This type of galaxy has a structure similar to the spiral and barred-spiral galaxy; however, instead of the classic "pinwheel" structure, the ring galaxy has an elliptical core surrounded by a ring of stars. Some traces of spiral structuring may be seen between the ring and the core. Although ring galaxies have a smaller habitability zone, they may still have stellar systems that can be habitable.
Irregular Galaxies
Irregular galaxies are just that, rough assemblages of stars with little or no regular structure. The Large and Small Magellanic Galaxies are irregular companions of our Milky Way Galaxy. In fact, they may be remnants of collisions or close encounters with other galaxies. Irregulars tend to be too small to generate star-breeding grounds, but on occasion, they can. The Tarantula Nebula in the Large Magellanic Galaxy is a star-breeding area. Because some irregular galaxies can have star-breeding areas, there is a chance for stellar systems possessing terrestrial planets.
Elliptical Galaxies
Also referred to as "dead" galaxies, this type of galaxy has very little gas and dust for star-breeding and are predominantly old, metallicity poor stars. Elliptical galaxies have the widest range of sizes ranging from a couple thousand light years to truly immense monsters such as M87 in the Virgo Cluster which is over 3000× the size of our Milky Way (>30,000,000 ly across). Monsters like M87 tend to sit in the centroid region of galactic superclusters. Some elliptical galaxies may possess a dusty disc which could indicate a near dying region of star-breeding. However, there will be very little new star-breeding.
Lenticular Galaxies
As with the elliptical galaxies, lenticulars are considered to be "dead" galaxies. They can have a spheroidal and/or barred core, but exhibit very little else in common with the spiral and barred-spiral, except for overall shape. These galaxies have used up all of their interstellar hydrogen and helium and, thus, they will have an orangish-yellow to orangish-red glow. Lenticulars also have very little in the way of star-breeding areas since they have very little gas and dust. Virtually all of the stars in a lenticular galaxy are very old, most being twice as old as our star or older.
Interacting Galaxies
This is at least two galaxies, or more, that are about to collide or have just collided. Interacting galaxies tend to be hot breeding grounds for new stars, revitalizing perhaps two dead galaxies. Some of these can produce spectacular layouts.
Globular Clusters
These are very similar to open clusters, except in size and age. Globular clusters tend to be fuzzy balls of stars with an orangish-yellow to orangish-red glow. Like a lenticular galaxy, the stars tend to be old stars, most being 2× or older than our sun. The stars tend to be more closely packed in the center than with open clusters. The core, which is usually one to two parsecs in size, can contain as many as one to three thousand stars. It has never been verified that any globular cluster has a black hole as most other galaxies have. Mostly there will only be Jovian planets and Pluto-like ice balls within a globular cluster.
Open Clusters
Although not true galaxies, some consider open clusters to be dwarf galaxies inside other galaxies. Open clusters are actually regions within galaxies where new star formation is currently occurring or has recently occurred. They tend to have only a few tens to a few hundred stars and are rarely larger than 15 to 20 parsecs (48.925 to 65.234 light years) and rarely have any definitive structure. Open clusters are dominated by the young Population I blue-white O and B class stars and are also associated with emission and reflection nebulae (q.v.). Open clusters make poor areas for habitable terrestrial planets due to the immense radiation pumped out by the O and B stars. However, asteroid, planetesimal, and planetoid mining might be profitable, albeit dangerous.
Globular Common Open
Group of tens of thousands to hundreds of thousands of stars Group of stars held together by mutual gravitational attraction Group of hundreds of star
Highly symmetrical ball of stars All of its stars are the same age, having formed from the same cloud of gas and dust Irregular shaped grouping of stars
Frequently contains bright red giant stars Stars in the cluster are basically at the same distance from Earth Contains bright blue stars
Located in the halo or bulge of a galaxy The star color indicates the age of the stars in the cluster Located in the arms of spiral and barred-spiral galaxies
Composed of old stars that formed when the universe was younger Orbits the center of a galaxy Composed of young stars that recently formed in the disks of galaxies
No longer forming in or near any galaxy Continues to form in the arms of spiral and barred-spiral galaxies

Image 1: Original Hubble Classification Scheme
Image 2: Revised Hubble Classification Scheme
Image 3: Milky Way Showing Our Sun's Approximate Position
Image 4: Example spiral galaxies.. M64 Hubble Images - The "BlackEye" Galaxy: a spiral choked with stellar dust.
Image 5: AM 0644-741, a ring galaxy in Volans
Image 6: NGC 3718 - "Bowtie" Galaxy: This one is the result of a collision/merge of at least two galaxies.
Image 7: M87: The largest know galaxy. Notice the jet from the black hole on the right side.
Image 8: Lenticular Galaxies - Centauri A
Image 9: Interacting Galaxies The "Rose" - Arp 273 is a group of interacting galaxies
Image 10: Open Clusters - NGC 290

Tuesday, June 14, 2016

The dark side of the universe – a primer




With dark matter, dark energy, phantom matter and even a dark force, physics news can sometimes sound like the voiceover for a superhero movie. So what’s behind all the ominous-sounding jargon?
Over the past 40 years astronomers have realised that everything we can see – all the stars, planets and galaxies – make up less than 5% of the entire universe. What is the rest? The short answer is, we have no idea.
What we do know is there are two gaping holes in our understanding of our universe. As a placeholder, physicists call them dark matter and dark energy.
In a nutshell, dark matter is the invisible stuff which we can only detect from the way its immense gravity moves stars and galaxies.
Dark energy, on the other hand, is the mysterious something causing the universe to expand with ever increasing speed.
We don’t know if dark matter and dark energy are related – in fact they’re probably two completely different phenomena, both called “dark” just because we can’t see them.
Dark matter
How was it discovered?
Since the 1930s astronomers knew that the way galaxies spin did not make sense. The stars at the edges of galaxies were moving much faster than expected – so fast they should have been flung off the cosmic merry-go-round and out into deep space.
But these strange motions could be explained if there was a bunch of extra matter in and around the galaxies – matter that we can’t see. It’s this “dark matter” that holds galaxies together.
Since then, many other observations beyond the scale of whirling galaxies, from the choreography of galaxy clusters, to the collision of nebulae, all suggested the same thing.
Although some physicists have entertained other theories, such as modifications to gravity, by now most are pretty sure dark matter exists. It’s the only explanation that suits all the data.
What do we know?
We know dark matter doesn’t emit light (nor does it absorb or reflect it), so it can’t be made of rogue planets or clouds of normal matter. We know it’s “cold” (which in physics-speak means it moves slowly compared with the speed of light). We know it has gravity. We also know it doesn’t interact very strongly with anything, even itself – otherwise the dark matter would collapse into flat structures such as galaxies, rather than the spherical haloes we detect.
Oh, and it makes up about 27% of the universe
.
What could dark matter be?
The bottom line is it is probably some new kind of particle (or a whole family of particles) that we have never detected before. Dark matter particles could be all around you, and floating through your body right this second.
This means the answer to this grand cosmological puzzle, affecting the universe on scales of mllions of light years, could lie in the physics of tiny particles, much smaller than an atom.
Over the past 30 years physicists have sifted through dozens of different dark matter candidates. The prime suspect at the moment is a kind of particle called a weakly interacting massive particle, or WIMP. This is a kind of heavy particles that feel only the weak force.
One of the goals of CERN’s Large Hadron Collider is to look for WIMPs (the same way it found the Higgs Boson in 2013) – the elusive dark matter particles might be created when protons are smashed together at near the speed of light.
Can we detect dark matter?
Besides CERN, there are more than 30 experiments around the world devoted to finding dark matter.
Some of these are dedicated telescopes searching for the signature of particles created when two particles of dark matter annihilate.
Others are giant vats of liquid xenon watching for a telltale flash when a dark matter particle nudges an atomic nucleus. None has yet made a convincing detection of a dark matter particle, although some of the experiments have ruled out various possibilities of what dark matter might be.
It remains a possibility that dark matter may never be directly detectable – especially if it turns out to be a particle that does not even feel the weak force.
The dark force and dark photons
Some physicists have proposed that dark matter particles can interact with one another via a new force of nature – called, yes, the dark force and transmitted by dark photons (aka dark radiation).
There may even be different kinds of dark matter, some of which feels the dark force, and some do not.
Dark energy
How was dark energy discovered?
In the early 20th century, physicists including Albert Einstein imagined the universe as static and unchanging. But in 1929 American astronomer Edwin Hubble observed the motions of exploding stars and discovered the universe was expanding. In fact the universe must have had a beginning – a moment of creation called the big bang.
We can imagine the big bang a bit like an explosion. But after that initial burst, physicists thought the expansion should begin to slow down over time, as gravity acted to pull everything back to a single point again.
The question was whether the universe would ever stop expanding and reverse direction, falling back into a “big crunch”.
Then, in 1998, things got a bit more complicated.
Using the same method as Edwin Hubble (and with the telescope named after him) astronomers found that the expansion of the universe was not slowing down, but instead was accelerating. Galaxies are flying away from each other faster and faster each year.
It was a strange and unexpected result. A bit like if you were driving on a flat highway, took your foot off the accelerator – and then your car began to speed up!
Yet the data were convincing. Physicists realised this expansion must be driven by some sort of energy, and they called it “dark energy”.
What we know
We know that dark energy affects the universe as a whole. We know it acts a bit like a negative gravity pushing galaxies away from one another.
We also know that dark energy did not kick in until a few billion years ago. (For the first half of its life, the expansion of the universe was slowing down due to gravity pulling everything together.)
This makes physicists think dark energy is somehow tied up with space itself. This means its density in space is always the same, but as the universe expands (that is as more space is created), the amount of dark energy also increases.
This would explain why the amount of dark energy was insignificant when the universe was small.
What could it be?
The answer to the mystery
of dark energy might also lie in the minuscule quantum realm.
In quantum theory, “empty space” is not empty at all, but filled with a soup of particles continually popping into and out of existence. As weird as it sounds, physicists have actually measured the force created by these so-called “virtual particles” in the lab.
The problem is, when physicists try to calculate how much energy these virtual particles contribute to each cubic metre of empty space, they come out with a number that’s a factor of 10120 too large when compared to the density of dark energy (as measured from the accelerated expansion of the universe). That's a 1 with 120 zeroes after it, a ludicrous answer called “the worst theoretical prediction in the history of physics”.
Quintessence
Some physicists think dark energy could be akin to a fifth force of nature, pervading all of space. They call it “quintessence”, after the fifth element predicted by the Greek philosophers. As opposed to the cosmological constant, the quintessence is imagined to change over time – it was once attractive, but is now repulsive.
The big rip and phantom dark energy
In some theories, the quintessence can continue to grow stronger (in which case it’s called phantom dark energy).
This could destroy the universe.
If the expansion of the universe continues to accelerate, eventually reach the speed of light – first galaxies and stars would be cut off from one another, then eventually the space between the sun and the Earth would expand faster than the speed of light and individual atoms would be torn asunder as the space within them expanded at faster than the speed of light. This is the big rip.
A new gravity?
Dark energy might not be a new force, it might just be a sign that, at very large scales, gravity does not behave as Einstein’s theory of general relatively describes.
The ΛCDM (lambda cold dark matter) model
This is the name for the astrophysicists’ current best picture of the way the cosmos is screwed together.
Λ (or lambda) stands for dark energy, while cold dark matter describes the consensus that dark matter must be made up of some kind of slow moving, previously unknown particle.
In this picture, dark matter makes up 27% of the mass-energy of the universe, dark energy makes up about 68%, and ordinary matter – that of the stars and galaxies and our own flesh and blood – makes up less than 5%.
thanks 
Cecile G. Tamura

Sunday, May 29, 2016

Far-Future of Space Travel? The Planet's First Experimental Wormhole Created

Cecile G. Tamura



"If you have a wormhole, then you can turn them into time machines for going backward in time," says Caltech's Kip Thorne. "Wormholes" are cosmic tunnels that can connect two distant regions of the universe, or even to a parallel universe, and have been popularised by the dissemination of theoretical physics and by works of science fiction like Stargate, Star Trek or, more recently, Interstellar.
In 1935, Albert Einstein and Nathan Rosen used the theory of general relativity to propose the existence of "bridges" or paths through space-time called Einstein-Rosen bridges or wormholes that connect two different points in space-time, theoretically creating a shortcut that could reduce travel time and distance. But, using present-day technology it would be impossible to create a gravitational wormhole, as the field would have to be manipulated with huge amounts of gravitational energy, which no-one yet knows how to generate. In electromagnetism, however, advances in metamaterials and invisibility have allowed researchers to put forward several designs to achieve this.
In 2015, scientists in the Department of Physics at the Universitat Autònoma de Barcelona designed and created in the laboratory the first experimental wormhole that can connect two regions of space magnetically. This consists of a tunnel that transfers the magnetic field from one point to the other while keeping it undetectable - invisible - all the way.
The magnetic wormhole is an analogy of gravitational ones, as it "changes the topology of space, as if the inner region has been magnetically erased from space", explains Àlvar Sánchez, the lead researcher.
The researchers used metamaterials and metasurfaces to build the tunnel experimentally, so that the magnetic field from a source, such as a magnet or a an electromagnet, appears at the other end of the wormhole as an isolated magnetic monopole. This result is strange enough in itself, as magnetic monopoles - magnets with only one pole, whether north or south - do not exist in nature. The overall effect is that of a magnetic field that appears to travel from one point to another through a dimension that lies outside the conventional three dimensions.
The wormhole in this experiment is a sphere made of different layers: an external layer with a ferromagnetic surface, a second inner layer, made of superconducting material, and a ferromagnetic sheet rolled into a cylinder that crosses the sphere from one end to the other. The sphere is made in such a way as to be magnetically undetectable - invisible, in magnetic field terms - from the exterior.
These same researchers had already built a magnetic fibre in 2014: a device capable of transporting the magnetic field from one end to the other. This fibre was, however, detectable magnetically. The wormhole developed now, though, is a completely three-dimensional device that is undetectable by any magnetic field.
This means a step forward towards possible applications in which magnetic fields are used: in medicine for example. This technology could, for example, increase patients' comfort by distancing them from the detectors when having MRI scans in hospital, or allow MRI images of different parts of the body to be obtained simultaneously.
This study, published in Scientific Reports, involved the UAB Department of Physics researchers Jordi Prat, Carles Navau and Àlvar Sánchez, who is also a lecturer at ICREA Academy.
Who knows where future advances in wormhole research could take us. But as physicist Michio Kaku says:"Combining quantum entanglement with wormholes yields mind boggling results about black holes. But I don't trust them until we have a theory of everything which can combine quantum effects with general relativity. i.e. we need to have a full blown string theory resolve this sticky question."

Friday, May 20, 2016

New Support for Alternative Quantum View


An experiment claims to have invalidated a decades-old criticism against pilot-wave theory, an alternative formulation of quantum mechanics that avoids the most baffling features of the subatomic universe.
Of the many counterintuitive features of quantum mechanics, perhaps the most challenging to our notions of common sense is that particles do not have locations until they are observed. This is exactly what the standard view of quantum mechanics, often called the Copenhagen interpretation, asks us to believe. Instead of the clear-cut positions and movements of Newtonian physics, we have a cloud of probabilities described by a mathematical structure known as a wave function. The wave function, meanwhile, evolves over time, its evolution governed by precise rules codified in something called the Schrödinger equation. The mathematics are clear enough; the actual whereabouts of particles, less so. Until a particle is observed, an act that causes the wave function to “collapse,” we can say nothing about its location. Albert Einstein, among others, objected to this idea. As his biographer Abraham Pais wrote: “We often discussed his notions on objective reality. I recall that during one walk Einstein suddenly stopped, turned to me and asked whether I really believed that the moon exists only when I look at it.”
But there’s another view — one that’s been around for almost a century — in which particles really do have precise positions at all times. This alternative view, known as pilot-wave theory or Bohmian mechanics, never became as popular as the Copenhagen view, in part because Bohmian mechanics implies that the world must be strange in other ways. In particular, a 1992 study claimed to crystalize certain bizarre consequences of Bohmian mechanics and in doing so deal it a fatal conceptual blow. The authors of that paper concluded that a particle following the laws of Bohmian mechanics would end up taking a trajectory that was so unphysical — even by the warped standards of quantum theory — that they described it as “surreal.”

Nearly a quarter-century later, a group of scientists has carried out an experiment in a Toronto laboratory that aims to test this idea. And if their results, first reported earlier this year, hold up to scrutiny, the Bohmian view of quantum mechanics — less fuzzy but in some ways more strange than the traditional view — may be poised for a comeback.
Saving Particle Positions
Bohmian mechanics was worked out by Louis de Broglie in 1927 and again, independently, by David Bohm in 1952, who developed it further until his death in 1992. (It’s also sometimes called the de Broglie–Bohm theory.) As with the Copenhagen view, there’s a wave function governed by the Schrödinger equation. In addition, every particle has an actual, definite location, even when it’s not being observed. Changes in the positions of the particles are given by another equation, known as the “pilot wave” equation (or “guiding equation”). The theory is fully deterministic; if you know the initial state of a system, and you’ve got the wave function, you can calculate where each particle will end up.
That may sound like a throwback to classical mechanics, but there’s a crucial difference. Classical mechanics is purely “local” — stuff can affect other stuff only if it is adjacent to it (or via the influence of some kind of field, like an electric field, which can send impulses no faster than the speed of light). Quantum mechanics, in contrast, is inherently nonlocal. The best-known example of a nonlocal effect — one that Einstein himself considered, back in the 1930s — is when a pair of particles are connected in such a way that a measurement of one particle appears to affect the state of another, distant particle. The idea was ridiculed by Einstein as “spooky action at a distance.” But hundreds of experiments, beginning in the 1980s, have confirmed that this spooky action is a very real characteristic of our universe.
In the Bohmian view, nonlocality is even more conspicuous. The trajectory of any one particle depends on what all the other particles described by the same wave function are doing. And, critically, the wave function has no geographic limits; it might, in principle, span the entire universe. Which means that the universe is weirdly interdependent, even across vast stretches of space. The wave function “combines — or binds — distant particles into a single irreducible reality,” as Sheldon Goldstein, a mathematician and physicist at Rutgers University, has written.
The differences between Bohm and Copenhagen become clear when we look at the classic “double slit” experiment, in which particles (let’s say electrons) pass through a pair of narrow slits, eventually reaching a screen where each particle can be recorded.
When the experiment is carried out, the electrons behave like waves, creating on the screen a particular pattern called an “interference pattern.” Remarkably, this pattern gradually emerges even if the electrons are sent one at a time, suggesting that each electron passes through both slits simultaneously.

Those who embrace the Copenhagen view have come to live with this state of affairs — after all, it’s meaningless to speak of a particle’s position until we measure it. Some physicists are drawn instead to the Many Worlds interpretation of quantum mechanics, in which observers in some universes see the electron go through the left slit, while those in other universes see it go through the right slit — which is fine, if you’re comfortable with an infinite array of unseen universes.
By comparison, the Bohmian view sounds rather tame: The electrons act like actual particles, their velocities at any moment fully determined by the pilot wave, which in turn depends on the wave function. In this view, each electron is like a surfer: It occupies a particular place at every specific moment in time, yet its motion is dictated by the motion of a spread-out wave. Although each electron takes a fully determined path through just one slit, the pilot wave passes through both slits. The end result exactly matches the pattern one sees in standard quantum mechanics.
For some theorists, the Bohmian interpretation holds an irresistible appeal. “All you have to do to make sense of quantum mechanics is to say to yourself: When we talk about particles, we really mean particles. Then all the problems go away,” said Goldstein. “Things have positions. They are somewhere. If you take that idea seriously, you’re led almost immediately to Bohm. It’s a far simpler version of quantum mechanics than what you find in the textbooks.” Howard Wiseman, a physicist at Griffith University in Brisbane, Australia, said that the Bohmian view “gives you a pretty straightforward account of how the world is…. You don’t have to tie yourself into any sort of philosophical knots to say how things really are.”
But not everyone feels that way, and over the years the Bohm view has struggled to gain acceptance, trailing behind Copenhagen and, these days, behind Many Worlds as well. A significant blow came with the paper known as “ESSW,” an acronym built from the names of its four authors. The ESSW paper claimed that particles can’t follow simple Bohmian trajectories as they traverse the double-slit experiment. Suppose that someone placed a detector next to each slit, argued ESSW, recording which particle passed through which slit. ESSW showed that a photon could pass through the left slit and yet, in the Bohmian view, still end up being recorded as having passed through the right slit. This seemed impossible; the photons were deemed to follow “surreal” trajectories, as the ESSW paper put it.
The ESSW argument “was a striking philosophical objection” to the Bohmian view, said Aephraim Steinberg, a physicist at the University of Toronto. “It damaged my love for Bohmian mechanics.”
But Steinberg has found a way to rekindle that love. In a paper published in Science Advances, Steinberg and his colleagues — the team includes Wiseman, in Australia, as well as five other Canadian researchers — describe what happened when they actually performed the ESSW experiment. They found that the photon trajectories aren’t surrealistic after all — or, more precisely, that the paths may seem surrealistic, but only if one fails to take into account the nonlocality inherent in Bohm’s theory.

The experiment that Steinberg and his team conducted was analogous to the standard two-slit experiment. They used photons rather than electrons, and instead of sending those photons through a pair of slits, they passed through a beam splitter, a device that directs a photon along one of two paths, depending on the photon’s polarization. The photons eventually reach a single-photon camera (equivalent to the screen in the traditional experiment) that records their final position. The question “Which of two slits did the particle pass through?” becomes “Which of two paths did the photon take?”
Importantly, the researchers used pairs of entangled photons rather than individual photons. As a result, they could interrogate one photon to gain information about the other. When the first photon passes through the beam splitter, the second photon “knows” which path the first one took. The team could then use information from the second photon to track the first photon’s path. Each indirect measurement yields only an approximate value, but the scientists could average large numbers of measurements to reconstruct the trajectory of the first photon.

The team found that the photon paths do indeed appear to be surreal, just as ESSW predicted: A photon would sometimes strike one side of the screen, even though the polarization of the entangled partner said that the photon took the other route.
But can the information from the second photon be trusted? Crucially, Steinberg and his colleagues found that the answer to the question “Which path did the first photon take?” depends on when it is asked.
At first — in the moments immediately after the first photon passes through the beam splitter — the second photon is very strongly correlated with the first photon’s path. “As one particle goes through the slit, the probe [the second photon] has a perfectly accurate memory of which slit it went through,” Steinberg explained.
But the farther the first photon travels, the less reliable the second photon’s report becomes. The reason is nonlocality. Because the two photons are entangled, the path that the first photon takes will affect the polarization of the second photon. By the time the first photon reaches the screen, the second photon’s polarization is equally likely to be oriented one way as the other — thus giving it “no opinion,” so to speak, as to whether the first photon took the first route or the second (the equivalent of knowing which of the two slits it went through).
The problem isn’t that Bohm trajectories are surreal, said Steinberg. The problem is that the second photon says that Bohm trajectories are surreal — and, thanks to nonlocality, its report is not to be trusted. “There’s no real contradiction in there,” said Steinberg. “You just have to always bear in mind the nonlocality, or you miss something very important.”
Faster Than Light
Some physicists, unperturbed by ESSW, have embraced the Bohmian view all along and aren’t particularly surprised by what Steinberg and his team found. There have been many attacks on the Bohmian view over the years, and “they all fizzled out because they had misunderstood what the Bohm approach was actually claiming,” said Basil Hiley, a physicist at Birkbeck, University of London (formerly Birkbeck College), who collaborated with Bohm on his last book, The Undivided Universe. Owen Maroney, a physicist at the University of Oxford who was a student of Hiley’s, described ESSW as “a terrible argument” that “did not present a novel challenge to de Broglie–Bohm.” Not surprisingly, Maroney is excited by Steinberg’s experimental results, which seem to support the view he’s held all along. “It’s a very interesting experiment,” he said. “It gives a motivation for taking de Broglie–Bohm seriously.”
On the other side of the Bohmian divide, Berthold-Georg Englert, one of the authors of ESSW (along with Marlan Scully, George Süssman and Herbert Walther), still describes their paper as a “fatal blow” to the Bohmian view. According to Englert, now at the National University of Singapore, the Bohm trajectories exist as mathematical objects but “lack physical meaning.”
On a historical note, Einstein lived just long enough to hear about Bohm’s revival of de Broglie’s proposal — and he wasn’t impressed, dismissing it as too simplistic to be correct. In a letter to physicist Max Born, in the spring of 1952, Einstein weighed in on Bohm’s work:
Have you noticed that Bohm believes (as de Broglie did, by the way, 25 years ago) that he is able to interpret the quantum theory in deterministic terms? That way seems too cheap to me. But you, of course, can judge this better than I.
But even for those who embrace the Bohmian view, with its clearly defined particles moving along precise paths, questions remain. Topping the list is an apparent tension with special relativity, which prohibits faster-than-light communication. Of course, as physicists have long noted, nonlocality of the sort associated with quantum entanglement does not allow for faster-than-light signaling (thus incurring no risk of the grandfather paradox or other violations of causality). Even so, many physicists feel that more clarification is needed, especially given the prominent role of nonlocality in the Bohmian view. The apparent dependence of what happens here on what may be happening there cries out for an explanation.
“The universe seems to like talking to itself faster than the speed of light,” said Steinberg. “I could understand a universe where nothing can go faster than light, but a universe where the internal workings operate faster than light, and yet we’re forbidden from ever making use of that at the macroscopic level — it’s very hard to understand.”
by : Dan Falk
http://advances.sciencemag.org/content/2/2/e1501466
https://www.quantamagazine.org/20150910-einstein-insanity/
https://www.quantamagazine.org/20140624-fluid-tests-hint-a…/
https://www.quantamagazine.org/20140624-fluid-tests-hint-a…/
https://books.google.com.ph/books…
http://www.thefunisreal.com/tag/de-broglie-bohm-mechanics/
http://math.mit.edu/~bush/?p=3087

Cecile G. Tamura

Monday, May 16, 2016

Habitats and Sleep Chambers


Self-assembling space habitats and a deep sleep chamber for long-duration space missions sound like ideas ripped right from the pages of a science fiction novel, but these are some of the visionary projects NASA is currently developing.
Through NASA’s Innovative Advanced Concepts program (NIAC), the agency invests in many seemingly impossible technologies. Known for taking out-of-the-box concepts that seem like science fiction and turning them into science fact, the program is changing the future of space travel.
NASA just announced that eight concepts were given the green light to move to the next development phase. NIAC’s phase II awards $500,000 for two years of study in order to further test these technologies. This year's selections include a special habitat designed to induce cryosleep for on long-duration missions, a robotic space habitat that is able to build itself and grow in lunar orbit (making it a perfect orbital outpost), and much more.
“The NIAC program is one of the ways NASA engages the U.S. scientific and engineering communities, including agency civil servants, by challenging them to come up with some of the most visionary aerospace concepts,” Steve Jurczyk, associate administrator of NASA’s Space Technology Mission Directorate said in a statement. “This year’s Phase II fellows have clearly met this challenge.”
Here on Earth when we go on long trips, rest stops and gas stations are essential. This is also true for long-duration space travel. Fuel is heavy and expensive to launch, so why not have a series of orbital outposts set up like rest stops throughout the Solar System? Here’s where NIAC comes in. A group of engineers is testing the feasibility of growable habitats. Not to be confused with expandable space habitats like BEAM, these Growth-Adapted Tensegrity Structures (GATs) would be built in space by robots and are able to grow and evolve as needed. The project will explore the possibility of setting up the first outpost just beyond the Moon, and if successful we could eventually see these throughout the Solar System.
Right now NASA has its sights set on Mars, but eventually the agency plans on venturing out into deep space—a journey that could take years rather than months. To help mitigate the effects of aging on long-duration space travel, a group of engineers is working to develop a deep sleep chamber. This could lay the foundation for future cryo-sleep chambers and other forms of suspended animation. The proposed chamber is designed to medically-support astronauts who are in a deep sleep. Over the next two years, engineers will assess how long-duration sedation affects our organs and how to counteract bone loss and muscle atrophy that occurs during deep sleep.
Last month, Stephen Hawking teamed up with Yuri Milner to announce their plans of sending a fleet of tiny spacecraft to Alpha Centauri with lasers. The project is revolutionary because we don’t currently have the technology capable of sending one spacecraft, let alone a fleet to our closest stellar neighbor in any reasonable amount of time. However, one NIAC proposal is looking at a new method of propulsion to help us do just that. The Directed Energy Interstellar Study aims to pave the way for interstellar travel. Current propulsion systems cannot achieve the relativistic speeds required for interstellar travel, but by scaling down the spacecraft and directing them with specialized lasers, researchers believe they can.
This type of technology will not only revolutionize space travel but could allow us to study nearby exoplanets in greater detail.
Program executives are hopeful that with the additional funding, these projects will all go on to do what NIAC does best: change the possible.
http://www.nasa.gov/…/tensegrity-approaches-to-in-space-con…
http://www.nasa.gov/…/niac-2016-phase-i-and-phase-ii-select…
http://motherboard.vice.com/…/nasa-is-investing-in-growable…
http://www.nasa.gov/…/fi…/files/Bradford_2013_PhI_Torpor.pdf
http://motherboard.vice.com/re…/a-brief-history-of-cryosleep
http://motherboard.vice.com/…/starshot-alpha-centuri-stephe…
http://www.deepspace.ucsb.edu/…/directed-energy-interstella…
https://www.nasa.gov/…/deep-in-directed-energy-propulsion-f…