Big Bang Discovery: Physicists Hail Cosmic 'Holy Grail' As Nobel Prize Beckons

Physicists Hail Cosmic 'Holy Grail'
|

An echo of the universe's cataclysmic birth has been detected by scientists in a landmark discovery described as the "Holy Grail" of cosmology.

British physicists have called it the most significant finding in cosmological science in "years".

If confirmed, the findings are likely to win the team a Nobel prize for physics.

Ripples in the fabric of space itself known as gravitational waves were identified by a specially designed telescope at the south pole.

Like a cosmic tsunami, they were generated when the universe suddenly exploded into existence almost 14 billion years ago.

Scientists believe the cosmos expanded at an enormous rate - faster than the speed of light - in the first tiny fraction of a second after the Big Bang.

The theory, called "inflation", was dreamed up to explain why the universe today is so remarkably uniform.

The announcement from the Harvard-Smithsonian Center for Astrophysics in the US provides the first direct "smoking gun" evidence of inflation.

Open Image Modal

Above: the BICEP2 telescope in the Antarctic where the key observations were made

It also challenges scientists to grapple with a new mystery, because no-one can yet explain how inflation happened.

The signal detected by the BICEP2 (Background Imaging of Cosmic Extragalactic Polarazation) telescope is much stronger than expected.

"This has been like looking for a needle in a haystack, but instead we found a crowbar," said team co-leader Dr Clem Pryke, from the University of Minnesota.

Rumours about the discovery had been rife in the world of astrophysics. To make sure they got it right, the scientists analysed their data for more than three years before making it public.

British expert Dr Ed Daw, from the University of Sheffield, said: "Gravitational waves emitted at the time of the big bang can tell us how the universe came to exist.

"If these results prove correct, we will have new key information on the very early Universe, information that is hard to get from any other source."

Gravitational waves were predicted in Albert Einstein's General Theory of Relativity. Their potential sources include super-dense neutron stars and black holes, as well as the Big Bang. However, until now they have never been seen directly.

Open Image Modal

Above: BICEP2 looked for an imprint of primordial gravitational waves in the cosmic microwave background (CMB), a faint radiation afterglow left over from when the universe was just 400,000 years old.

"Our team hunted for a special type of polarization called 'B-modes' which represents a twisting or 'curl' pattern in the polarized orientations of the ancient light," said one of the lead scientists Professor Jamie Bock, from the California Institute of Technology.

The swirly B-mode pattern provided a unique gravitational wave signature.

"This is the first direct image of gravitational waves across the primordial sky," said team member Professor Chao-Lin Kuo, from Stanford University in California.

Astrophysicist Professor Avi Loeb, from Harvard University, said: "This work offers new insights into some of our most basic questions: Why do we exist? How did the universe begin? These results are not only a smoking gun for inflation, they also tell us when inflation took place and how powerful the process was."

PICS: Space Is Incredible
Europa(01 of41)
Open Image Modal
The icy surface of Europa is shown strewn with cracks, ridges and "chaotic terrain," where the surface has been disrupted and ice blocks have moved around. New laboratory experiments show that water ice and frozen sulfur dioxide react even at the frigid temperatures of Europa. Because the reaction occurs without the aid of radiation, it could take place throughout the moon's thick ice layer—an outcome that would revamp current thinking about the chemistry and geology of this moon and perhaps others. (credit:NASA/JPL/University of Arizona)
Venus(02 of41)
Open Image Modal
Unlike Earth, Venus lacks a magnetic field to deflect powerful solar outbursts -- as can be seen in this NASA-created image, a still from the video "Dynamic Earth: Exploring Earth's Climate Engine." (credit:NASA)
Saturn's Storm(03 of41)
Open Image Modal
This vertigo-inducing, false-color image from NASA's Cassini mission highlights the storms at Saturn's north pole. The angry eye of a hurricane-like storm appears dark red while the fast-moving hexagonal jet stream framing it is a yellowish green. Low-lying clouds circling inside the hexagonal feature appear as muted orange color. A second, smaller vortex pops out in teal at the lower right of the image. The rings of Saturn appear in vivid blue at the top right. (credit:NASA/JPL-Caltech/SSI)
Carina Nebula(04 of41)
Open Image Modal
This Hubble photo is of a small portion of a large star-birthing region in the Carina Nebula. Towers of cool hydrogen laced with dust rise from the wall of the nebula. (credit:NASA)
Gas Falling Into A Black Hole(05 of41)
Open Image Modal
This computer simulation shows gas from a tidally shredded star falling into a black hole. Some of the gas also is being ejected at high speed into space. (credit:NASA; S. Gezari, The Johns Hopkins University; and J. Guillochon, University of California, Santa Cruz)
'Black Marble'(06 of41)
Open Image Modal
This image of Asia and Australia at night is a composite assembled from data acquired by the Suomi NPP satellite in April and October 2012. (credit:NASA Earth Observatory)
Ring Nebula(07 of41)
Open Image Modal
In this composite image, visible-light observations by NASA’s Hubble Space Telescope are combined with infrared data from the ground-based Large Binocular Telescope in Arizona to assemble a dramatic view of the well-known Ring Nebula. (credit:NASA, ESA, C.R. Robert O’Dell (Vanderbilt University), G.J. Ferland (University of Kentucky), W.J. Henney and M. Peimbert (National Autonomous University of Mexico) Credit for Large Binocular Telescope data: David Thompson (University of Arizona))
Supernova Remnant(08 of41)
Open Image Modal
A delicate ribbon of gas floats eerily in our galaxy. A contrail from an alien spaceship? A jet from a black-hole? Actually this image, taken by NASA's Hubble Space Telescope, is a thin section of a supernova remnant caused by a stellar explosion that occurred more than 1,000 years ago. (credit:Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) Acknowledgment: W. Blair (Johns Hopkins University))
Jupiter and Ganymede(09 of41)
Open Image Modal
NASA's Hubble Space Telescope caught Jupiter's moon Ganymede playing a game of "peek-a-boo." In this crisp image, Ganymede is shown just before it ducks behind the giant planet. (credit:NASA, ESA, and E. Karkoschka (University of Arizona))
Crab Nebula(10 of41)
Open Image Modal
The Crab Nebula is a supernova remnant, all that remains of a tremendous stellar explosion. Observers in China and Japan recorded the supernova nearly 1,000 years ago, in 1054. (credit:NASA, ESA, J. Hester and A. Loll (Arizona State University))
Lagoon Nebula(11 of41)
Open Image Modal
A spectacular NASA/ESA Hubble Space Telescope image reveals the heart of the Lagoon Nebula. Seen as a massive cloud of glowing dust and gas, bombarded by the energetic radiation of new stars, this placid name hides a dramatic reality. (credit:NASA, ESA)
Mercury(12 of41)
Open Image Modal
This colorful view of Mercury was produced by using images from the color base map imaging campaign during the spacecraft MESSENGER's primary mission. The colors are not what Mercury would look like to the human eye, but rather the colors enhance the chemical, mineralogical, and physical differences between the rocks that make up Mercury's surface. (credit:NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington )
Cat's Eye Nebula(13 of41)
Open Image Modal
The Cat's Eye Nebula, one of the first planetary nebulae discovered, also has one of the most complex forms known to this kind of nebula. Eleven rings, or shells, of gas make up the Cat's Eye. Each 'ring' is actually the edge of a spherical bubble seen projected onto the sky -- that's why it appears bright along its outer edge. (credit:NASA, ESA, HEIC, and The Hubble Heritage Team (STScI/AURA) Acknowledgment: R. Corradi (Isaac Newton Group of Telescopes, Spain) and Z. Tsvetanov (NASA))
Spiral Galaxy(14 of41)
Open Image Modal
The vibrant magentas and blues in this Hubble image of the barred spiral galaxy M83 reveal that the galaxy is ablaze with star formation. Also known as the Southern Pinwheel, the galaxy lies 15 million light-years away in the constellation Hydra. (credit:NASA, ESA, and the Hubble Heritage Team (STScI/AURA) Acknowledgement: W. Blair (STScI/Johns Hopkins University) and R. O'Connell (University of Virginia))
Aurora(15 of41)
Open Image Modal
Swirls of green and red appear in an aurora over Whitehorse, Yukon on the night of September 3, 2012. The aurora was due to a coronal mass ejection from the sun, which erupted on August 31. (credit:Courtesy of David Cartier, Sr.)
Eta Carinae(16 of41)
Open Image Modal
NASA's Hubble Telescope captured an image of the binary star system Eta Carinae. This image consists of ultraviolet and visible light images from the High Resolution Channel of Hubble's Advanced Camera for Surveys. (credit: ESA/NASA)
Saturn's Moons(17 of41)
Open Image Modal
Saturn's orange moon Titan peeks from behind two of Saturn's rings. Small, battered Epimetheus, another of Saturn's 62 moons, appears just above the rings. (credit:NASA/JPL/Space Science Institute)
Saturn's Auroras(18 of41)
Open Image Modal
Scientists first observed Saturn’s auroras in 1979. Decades later, these shimmering ribbons of light still fascinate. For one thing they’re magnificently tall, rising hundreds of miles above the planet’s poles. And unlike on Earth, where bright displays fizzle after only a few hours, auroras on Saturn can shine for days. Auroras are produced when speeding particles accelerated by the sun’s energy collide with gases in a planet’s atmosphere. The gases fluoresce, emitting flashes of light at different wavelengths. (credit:NASA)
'Star Formation Laboratory'(19 of41)
Open Image Modal
The dwarf galaxy NGC 4214 is ablaze with young stars and gas clouds. Located around 10 million light-years away in the constellation of Canes Venatici (The Hunting Dogs), the galaxy's close proximity, combined with the wide variety of evolutionary stages among the stars, make it an ideal laboratory to research the triggers of star formation and evolution. (credit:NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration)
Red Dwarf Star(20 of41)
Open Image Modal
Artist's depiction of the powerful flare that erupted from the red dwarf star EV Lacertae in 2008. (credit:Casey Reed/NASA)
Coronal Mass Ejection(21 of41)
Open Image Modal
On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space. The coronal mass ejection, or CME, traveled at over 900 miles per second. The CME did not travel directly toward Earth, but did connect with Earth's magnetic environment, or magnetosphere, causing auroras to appear on the night of Monday, September 3. (credit:NASA/GSFC/SDO)
Centaurus A(22 of41)
Open Image Modal
Resembling looming rain clouds on a stormy day, dark lanes of dust crisscross the giant elliptical galaxy Centaurus A. Hubble's panchromatic vision, stretching from ultraviolet through near-infrared wavelengths, reveals the vibrant glow of young, blue star clusters and a glimpse into regions normally obscured by the dust. (credit:NASA/Cheryl Gundy, STSCI)
Andromeda Galaxy(23 of41)
Open Image Modal
This mosaic of M31 merges 330 individual images taken by the Ultraviolet/Optical Telescope aboard NASA's Swift spacecraft. It is the highest-resolution image of the galaxy ever recorded in the ultraviolet. (credit:NASA/Swift/Stefan Immler (GSFC) and Erin Grand (UMCP))
Mickey Mouse On Mercury?(24 of41)
Open Image Modal
This scene is to the northwest of the crater Magritte, in Mercury's south. The image is not map projected; the larger crater actually sits to the north of the two smaller ones. The shadowing helps define the striking "Mickey Mouse" resemblance, created by the accumulation of craters over Mercury's long geologic history. (credit:NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington)
Aurora From Space(25 of41)
Open Image Modal
From space, the aurora is a crown of light that circles each of Earth’s poles. The IMAGE satellite captured this view of the aurora australis (southern lights) on September 11, 2005, four days after a record-setting solar flare sent plasma—an ionized gas of protons and electrons—flying towards the Earth. The ring of light that the solar storm generated over Antarctica glows green in the ultraviolet part of the spectrum, shown in this image. From the Earth’s surface, the ring would appear as a curtain of light shimmering across the night sky. (credit:NASA/Goddard Space Flight Center Scientific Visualization Studio)
Daybreak On Mars(26 of41)
Open Image Modal
This computer-generated view depicts part of Mars at the boundary between darkness and daylight. Gale Crater looms in the distance, distinguished from adjacent craters by its central mountain of strata. Gale Crater straddles the dichotomy boundary of Mars, which separates the broad, flat, and young northern plains from the much older and rougher southern highlands. (credit:NASA/JPL-Caltech)
Saturn(27 of41)
Open Image Modal
As Saturn's rings orbit the planet, a section is typically in the planet's shadow, experiencing a brief night lasting from 6 to 14 hours. However, about once every 15 years, night falls over the entire visible ring system for about four days. This happens during Saturn's equinox, when the sun is directly over the planet's equator. At this time, the rings, which also orbit directly over the planet's equator, appear edge-on to the sun. During equinox, light from the sun hits the ring particles at very low angles, accenting their topography and giving us a three-dimensional view of the rings. (credit:NASA/JPL/Space Science Institute)
Jupiter(28 of41)
Open Image Modal
New red spot appears on Jupiter. (credit:M. Wong and I. de Pater (University of California, Berkeley))
Cygnus X(29 of41)
Open Image Modal
Cygnus X hosts many young stellar groupings. The combined outflows and ultraviolet radiation from the region's numerous massive stars have heated and pushed gas away from the clusters, producing cavities of hot, lower-density gas. In this infrared image, ridges of denser gas mark the boundaries of the cavities. Bright spots within these ridges show where stars are forming. (credit:NASA/IPAC/MSX)
Spiral Galaxy(30 of41)
Open Image Modal
The Hubble Space Telescope revealed this majestic disk of stars and dust lanes in this view of the spiral galaxy NGC 2841. A bright cusp of starlight marks the galaxy's center. Spiraling outward are dust lanes that are silhouetted against the population of whitish middle-aged stars. Much younger blue stars trace the spiral arms. (credit:NASA)
Horsehead Nebula(31 of41)
Open Image Modal
Astronomers have used NASA's Hubble Space Telescope to photograph the iconic Horsehead Nebula in a new, infrared light to mark the 23rd anniversary of the famous observatory's launch aboard the space shuttle Discovery on April 24, 1990.
Planetary Nebula(32 of41)
Open Image Modal
This planetary nebula's simple, graceful appearance is thought to be due to perspective: our view from Earth looking straight into what is actually a barrel-shaped cloud of gas shrugged off by a dying central star. Hot blue gas near the energizing central star gives way to progressively cooler green and yellow gas at greater distances with the coolest red gas along the outer boundary.
Hubble Images Searchlight Beams from a Preplanetary Nebula(33 of41)
Open Image Modal
The NASA/ESA Hubble Space Telescope has been at the cutting edge of research into what happens to stars like our sun at the ends of their lives. One stage that stars pass through as they run out of nuclear fuel is called the preplanetary or protoplanetary nebula stage. This Hubble image of the Egg Nebula shows one of the best views to date of this brief but dramatic phase in a star’s life
Dying Star (34 of41)
Open Image Modal
A Dying Star Shrouded by a Blanket of Hailstones Forms the Bug Nebula (NGC 6302)
Colossal Glow(35 of41)
Open Image Modal
Saturn’s auroras put on a dazzling display of light. Scientists first observed Saturn’s auroras in 1979. Decades later, these shimmering ribbons of light still fascinate. For one thing they’re magnificently tall, rising hundreds of miles above the planet’s poles. And unlike on Earth where bright displays fizzle after only a few hours, auroras on Saturn can shine for days. Auroras are produced when speeding particles accelerated by the sun’s energy collide with gases in a planet’s atmosphere. The gases fluoresce, emitting flashes of light at different wavelengths. Watch the video (1.usa.gov/IFW5o7) to see an edge-on view of Saturn’s northern and southern lights courtesy of NASA’s Hubble Space Telescope.
Supermoon(36 of41)
Open Image Modal
Up there in the sky – it's not a bird or a plane; it's a "Supermoon." Bigger and brighter then normal full moons, the supermoon on June 22/23 will be the closest and largest full moon for all of 2013. The moon will be some 29,000 miles closer to Earth than the farthest point in its orbit, but not to worry the moon will still be more than 221,000 miles away from our blue planet.
Hubble Sees Stars and a Stripe in Celestial Fireworks(37 of41)
Open Image Modal
This image is a composite of visible (or optical), radio, and X-ray data of the full shell of the supernova remnant from SN 1006. The radio data show much of the extent that the X-ray image shows. In contrast, only a small linear filament in the northwest corner of the shell is visible in the optical data. The object has an angular size of roughly 30 arcminutes (0.5 degree, or about the size of the full moon), and a physical size of 60 light-years (18 parsecs) based on its distance of nearly 7,000 light-years. The small green box along the bright filament at the top of the image corresponds to the dimensions of the Hubble release image.
NASA's Hubble Shows Milky Way is Destined for Head-On Collision(38 of41)
Open Image Modal
This illustration shows a stage in the predicted merger between our Milky Way galaxy and the neighboring Andromeda galaxy, as it will unfold over the next several billion years. In this image, representing Earth's night sky in 3.75 billion years, Andromeda (left) fills the field of view and begins to distort the Milky Way with tidal pull.
New Supernova Remnant Light Up(39 of41)
Open Image Modal
Astronomers using NASA's Hubble Space Telescope are witnessing the unprecedented transition of a supernova to a supernova remnant, where light from an exploding star in a neighboring galaxy, the Large Magellanic Cloud, reached Earth in February 1987. Named Supernova 1987A, it was the closest supernova explosion witnessed in almost 400 years.
Aurora Australis from Space(40 of41)
Open Image Modal
From space, the aurora is a crown of light that circles each of Earth’s poles. The IMAGE satellite captured this view of the aurora australis (southern lights) on September 11, 2005, four days after a record-setting solar flare sent plasma—an ionized gas of protons and electrons—flying towards the Earth. The ring of light that the solar storm generated over Antarctica glows green in the ultraviolet part of the spectrum, shown in this image. The IMAGE observations of the aurora are overlaid onto NASA’s satellite-based Blue Marble image. From the Earth’s surface, the ring would appear as a curtain of light shimmering across the night sky.
Daybreak at Gale Crater(41 of41)
Open Image Modal
The Curiosity rover bristles with multiple cameras and instruments, including Goddard's Sample Analysis at Mars (SAM) instrument suite. By looking for evidence of water, carbon, and other important building blocks of life in the Martian soil and atmosphere, SAM will help discover whether Mars ever had the potential to support life. Curiosity will be delivered to Gale crater, a 96-mile-wide crater that contains a record of environmental changes in its sedimentary rock, in August 2012.

BICEP2 was the second stage of the mission to detect gravitational waves.

The scientists travelled to the South Pole to take advantage of its cold, dry, stable air.

"The South Pole is the closest you can get to space and still be on the ground," said principal investigator Professor John Kovac, from the Harvard-Smithsonian Centre for Astrophysics.

"It's one of the driest and clearest locations on Earth, perfect for observing the faint microwaves from the Big Bang."

The scientists acknowledge that interaction between CMB and space dust could produce a similar effect as that produced by primordial gravitational waves. But they have made painstaking efforts to rule out such a possibility.