Showing posts with label Neutrons. Show all posts
Showing posts with label Neutrons. Show all posts

Wednesday, November 25, 2015

PART-3/8--The Universe: Big Bang to Now in 10 Easy Steps((The Origin, History, Evolution & Future of the Universe)

How the Universe Came to Be
INTRODUCTION
Credit: Subaru/ P. Capak (SSC/Caltech)
The broadly accepted theory for the origin and evolution of our universe is the Big Bang model, which states that the universe began as an incredibly hot, dense point roughly 13.7 billion years ago. So, how did the universe go from being fractions of an inch (a few millimeters) across to what it is today?

Here is a breakdown of the Big Bang to now in 10 easy-to-understand steps.



10.How It All Started
Credit: NASA/WMAP
The Big Bang was not an explosion in space, as the theory's name might suggest. Instead, it was the appearance of space everywhere in the universe, researchers have said. According to the Big Bang theory, the universe was born as a very hot, very dense, single point in space.
In 2001, NASA launched the Wilkinson Microwave Anisotropy Probe (WMAP) mission to study the conditions as they existed in the early universe by measuring radiation from the cosmic microwave background. Among other discoveries, WMAP was able to determine the age of the universe — about 13.7 billion years old.

9.The Universe's First Growth Spurt
Credit: NASA, ESA, and S. Beckwith (STScI) and the HUDF Team
When the universe was very young — something like a hundredth of a billionth of a trillionth of a trillionth of a second (whew!) — it underwent an incredible growth spurt. During this burst of expansion, which is known as inflation, the universe grew exponentially and doubled in size at least 90 times.
After inflation, the universe continued to grow, but at a slower rate. As space expanded, the universe cooled and matter formed.
8.Too Hot to Shine



Credit: NASA/WMAP
Light chemical elements were created within the first three minutes of the universe's formation. As the universe expanded, temperatures cooled and protons and neutrons collided to make deuterium, which is an isotope of hydrogen. Much of this deuterium combined to make helium.

For the first 380,000 years after the Big Bang, however, the intense heat from the universe's creation made it essentially too hot for light to shine. Atoms crashed together with enough force to break up into a dense, opaque plasma of protons, neutrons and electrons that scattered light like fog.
7.Let There Be Light
Credit: ESA/ LFI & HFI Consortia

About 380,000 years after the Big Bang, matter cooled enough for electrons to combine with nuclei to form neutral atoms. This phase is known as "recombination," and the absorption of free electrons caused the universe to become transparent. The light that was unleashed at this time is detectable today in the form of radiation from the cosmic microwave background.

Yet, the era of recombination was followed by a period of darkness before stars and other bright objects were formed.
6.Emerging from the Cosmic Dark Ages
Credit: ESA XMM-Newton/EPIC, LBT/LBC, AIP (J. Kohnert)
Roughly 400 million years after the Big Bang, the universe began to come out of its dark ages. This period in the universe's evolution is called the age of re-ionization.
During this time, clumps of gas collapsed enough to form the very first stars and galaxies. The emitted ultraviolet light from these energetic events cleared out and destroyed most of the surrounding neutral hydrogen gas. The process of re-ionization, plus the clearing of foggy hydrogen gas, caused the universe to become transparent to ultraviolet light for the first time.
5.More Stars and More Galaxies
Credit: ESA, Hubble, NASA
Astronomers comb the universe looking for the most far-flung and oldest galaxies to help them understand the properties of the early universe. Similarly, by studying the cosmic microwave background, astronomers can work backwards to piece together the events that came before.
4.Birth of Our Solar System


Credit: NASA

Our solar system is estimated to have been born a little after 9 billion years after the Big Bang, making it about 4.6 billion years old. According to current estimates, the sun is one of more than 100 billion stars in our Milky Way galaxy alone, and orbits roughly 25,000 light-years from the galactic core.

Many scientists think the sun and the rest of our solar system was formed from a giant, rotating cloud of gas and dust known as the solar nebula. As gravity caused the nebula to collapse, it spun faster and flattened into a disk. During this phase, most of the material was pulled toward the center to form the sun.
3.The Invisible Stuff in the Universe
Credit: X-ray: NASA/CXC/CfA/M.Markevitch et al.; Optical: NASA/STScI; Magellan/U.Arizona/D.Clowe et al.; Lensing Map: NASA/STScI; ESO WFI; Magellan/U.Arizona/D.Clowe et al.
In the 1960s and 1970s, astronomers began thinking that there might be more mass in the universe than what is visible.
This mysterious and invisible mass became known as dark matter. Dark matter is inferred because of the gravitational pull it exerts on regular matter. One hypothesis states the mysterious stuff could be formed by exotic particles that don't interact with light or regular matter, which is why it has been so difficult to detect.

Dark matter is thought to make up 23 percent of the universe. In comparison, only 4 percent of the universe is composed of regular matter, which encompasses stars, planets and people.
2.The Expanding and Accelerating Universe
Credit: NASA, ESA, D. Coe (NASA Jet Propulsion Laboratory/California Institute of Technology, and Space Telescope Science Institute), N. Benitez (Institute of Astrophysics of Andalusia, Spain), T. Broadhurst (University of the Basque Country, Spain), and H. Ford
In the 1920s Hubble observed that the universe is not static, but rather is expanding.

Decades later, in 1998, the prolific space telescope named after the famous astronomer, the Hubble Space Telescope, studied very distant supernovas and found that, a long time ago, the universe was expanding more slowly than it is today. This discovery was surprising because it was long thought that the gravity of matter in the universe would slow its expansion, or even cause it to contract.

Dark energy is thought to be the strange force that is pulling the cosmos apart at ever-increasing speeds, but it remains undetected and shrouded in mystery. The existence of this elusive energy, which is thought to make up 73 percent of the universe, is one of the most hotly debated topics in cosmology.
1.Still a Lot to Learn
Credit: NASA
Dark matter and dark energy remain two of the biggest mysteries, but cosmologists continue to probe the universe in hopes of better understanding how it all began.




http://www.space.com/13320-big-bang-universe-10-steps-explainer.html


Saturday, October 10, 2015

Top 10 subatomic surprises

Nobel Prize–winning neutrinos rank among science’s most unexpected discoveries
The 20th century brought many surprising discoveries about the subatomic realm, including that there are many, many types of subatomic particles, some of which are seen above in the aftermath of gold ion collisions at Brookhaven National Laboratory's Relativistic Heavy Ion Collider.
Neutrinos are popular among the people who award the Nobel prizes.

In 1995 Fred Reines won the physics Nobel for detecting neutrinos, bizarre subatomic particles that some experts said could never be detected. In 2002, Ray Davis and Masatoshi Koshiba won for measuring how many neutrinos the sun sends to the Earth. In 1988, the physics prize honored the discovery of the muon neutrino, one of three “flavors” in the neutrino family. And this year, Takaaki Kajita and Arthur McDonald shared the prize for demonstrating that neutrinos can change themselves from one flavor into another.

Wolfgang Pauli, the Austrian physicist who predicted the neutrino’s existence, also won a Nobel, but not for the neutrino (he did a lot of other very important stuff). He might have won for the neutrino except that his prediction came in the form of a letter to physicists attending a conference that Pauli decided to skip so he could go to a dance.

Pauli’s idea that a previously unknown and uncharged particle could explain a perplexing physics mystery came as a surprise. That particle’s eventual detection was perhaps even more surprising still. But neutrinos are just one of many surprises from the subatomic realm that physicists encountered during the 20th century. I can think of at least 10 more, thereby qualifying this topic for a top 10 list. Starting with:

10. There is, in fact, such a thing as subatomic.
Throughout the 19th century, the existence of atoms was a hot topic, thanks largely to the success of the atomic theory in chemistry articulated by English schoolteacher John Dalton. Before then atoms had been primarily a philosophical concept, showing up in arguments about the ultimate nature of matter but typically regarded as beyond the reach of experimental investigation. Many physicists believed atoms were fictions, perhaps convenient for explaining experimental results although not physically real. But hints accumulated that atoms not only existed, but also weren’t really atoms, if you applied the etymological definition of atom as something indivisible. The periodic repetition of atomic properties identified by Russian chemist Dmitri Mendeleyev suggested some sort of internal atomic structure. By the late 19th century more clues had accumulated, and J.J. Thomson’s discovery of the electron in 1897 — the first subatomic particle to be identified — pretty much clinched the case that atoms had parts.

9. Atomic nucleus
Once physicists agreed that atoms had parts, the next task was figuring out how those parts arranged themselves. Thomson suggested that his negatively charged electrons dispersed themselves like plums in a positively charged pudding. But when Ernest Rutherford had his assistants shoot alpha particles at a thin sheet of gold, some of the alpha particles bounced backward. To express his surprise, Rutherford commented that it was like shooting an artillery shell at a piece of tissue paper and seeing it bounce back at you. He soon figured out that almost all of the atom’s mass was crunched into a tiny ball in the middle. Rutherford called that ball the kern; today it’s known as the nucleus.

8. Neutrons
Before the 1930s, physicists knew about two subatomic particles: the proton and the electron, which seemed to explain everything about matter. But in 1920 Rutherford had suggested the existence of another particle in the nucleus, a neutral particle about the same mass as the proton. In 1932, Rutherford’s protégé James Chadwick found the neutron. The discovery of the neutron was a big surprise, the late Hans Bethe, one of the last century’s most prominent nuclear physicists, once told me. But how could it be a surprise? I asked. Hadn’t Rutherford already predicted its existence? “Yes,” Bethe said, “but nobody would believe him except Chadwick.” (Historical footnote: Pauli called his new particle a “neutron” because it had no charge. But it was not the same as Chadwick’s neutron, which was much more massive. So Enrico Fermi called Pauli’s particle the neutrino, Italian for “little neutral one.”)

7. Subatomic particles are actually waves (sometimes)
Thomson won a Nobel Prize in 1906 for the experiments establishing the existence of the first known subatomic particle, the electron. So he must have been surprised when, in 1937, his son George also won a Nobel Prize — for demonstrating that electrons (at least in some experiments) were actually waves. This wave-particle duality is at the heart of quantum physics, which is of course full of so many surprises that it will get its own top 10 list someday.

6. Neutrinos can be detected
In 1934, Bethe and Rudolf Peierls calculated that neutrinos would interact so weakly with matter that you’d be stupid to try to detect one. You would need a tank of solid matter (perhaps liquid hydrogen) roughly 1,000 light-years across. “There is no practically possible way of observing the neutrino,” they concluded. But if the odds are a gazillion to one against detecting a neutrino, all you need to do is make a gazillion neutrinos and your chances will be much better. There was no way to do that in 1934, but after nuclear fission was discovered a few years later, and then nuclear reactors were invented, physicists all of a sudden had a prolific source of neutrinos. So Fred Reines and his collaborator Clyde Cowan set up detectors outside a reactor (after rethinking their first idea, which was to set off an atomic bomb) and recorded clear-cut evidence of neutrinos’ existence in 1956. “So why did we want to detect the free neutrino?” Reines said later. “Because everybody said you couldn’t do it.”

5. There are a gazillion subatomic particles
By the 1950s, physicists had built atom smashers powerful enough not only to reveal the particles within the atom, but to create new ones, subatomic in size but not ordinarily atomic constituents. Dozens of new particles appeared in atom smasher debris, their names outnumbering the available letters in the Greek alphabet. Leon Lederman (one of the 1988 Nobel winners for the muon neutrino discovery) once told me he was waiting in a lunch line with Fermi and asked the great physicist what he thought of the newly discovered V-zero-2 particle. “My boy,” Fermi replied, “if I could remember the names of these particles I would have become a botanist.”

4. Quarks
In the 1950s, physicists were surprised to learn about all the subatomic particles that did not actually reside in atoms. Then in the 1960s came the surprise that the subatomic particles residing in the atomic nucleus comprised a set of three still smaller particles — and that those particles carried electric charges a fraction of the supposedly unitary charge of protons or electrons. Murray Gell-Mann, who called those particles quarks, almost gave up on his idea because of the fractional charges, which most people considered impossible. But once he realized fractional charges were OK because the quarks couldn’t escape from the nucleus, he published his Nobel Prize–winning idea. A few years later, when experiments confirmed the existence of his quarks, many physicists were surprised. But Gell-Mann wasn’t.

3. Parity violation
Long before the explosion of subatomic particle discoveries, the esteemed mathematician Hermann Weyl noted that nature knew nothing about handedness (or parity). “There can be no doubt,” he wrote, “that all natural laws are invariant with respect to an interchange of right and left.” But then in 1956, Chen Ning Yang and Tsung-Dao Lee raised some doubts that left-right symmetry was obeyed in certain cases where subatomic particles decayed. Soon thereafter experiments confirmed Yang and Lee’s suspicion. “It was so surprising,” Lederman told me. “It was socko!”

2. Protons don’t decay
Outside the atomic nucleus, neutrons are notoriously unstable, decaying within a few minutes to form a proton, an electron, and (of course) a neutrino (well, actually an antineutrino, but that’s not important right now). The leftover proton, though, is supposedly stable and should last forever. But in the 1970s, theorists began to believe that protons should also decay (although in trillions of trillions of trillions of years, rather than a few minutes). But that surprise never happened — prodigious efforts to detect proton decay have turned up no sign of it. And that’s an even bigger surprise.

1. Positrons
In 1932, the neutron wasn’t the only surprising subatomic particle to be discovered. That same year Carl Anderson analyzed the tracks of cosmic rays in a cloud chamber and found one that looked like it belonged to an electron, except that it curved the wrong direction. It turned out to be the positron, the antiparticle of the electron (Anderson called it a “positive electron”). The discovery of an antimatter particle was in some senses a big surprise, but maybe it shouldn’t have been, since Paul Dirac had deduced its existence by analyzing his equation describing electrons. So maybe the surprise was that somebody could infer the existence of something so strange just by playing around with equations.

https://www.sciencenews.org/