Solar Energy News  
TIME AND SPACE
Latest experiment at Large Hadron Collider reports first results
by Staff Writers
Boston MA (SPX) Oct 15, 2015


File image.

After a two-year hiatus, the Large Hadron Collider, the largest and most powerful particle accelerator in the world, began its second run of experiments in June, smashing together subatomic particles at 13 teraelectronvolts (TeV) - the highest energy ever achieved in a laboratory. Physicists hope that such high-energy collisions may produce completely new particles, and potentially simulate the conditions that were seen in the early universe.

In a paper to appear in the journal Physics Letters B, the Compact Muon Solenoid (CMS) collaboration at the European Organization for Nuclear Research (CERN) reports on the run's very first particle collisions, and describes what an average collision between two protons looks like at 13 TeV. One of the study leaders is MIT assistant professor of physics Yen-Jie Lee, who leads MIT's Relativistic Heavy Ion Group, together with physics professors Gunther Roland and Bolek Wyslouch.

In the experimental run, researchers sent two proton beams hurtling in opposite directions around the collider at close to the speed of light. Each beam contained 476 bunches of 100 billion protons, with collisions between protons occurring every 50 nanoseconds. The team analyzed 20 million "snapshots" of the interacting proton beams, and identified 150,000 events containing proton-proton collisions.

For each collision that the researchers identified, they determined the number and angle of particles scattered from the colliding protons. The average proton collision produced about 22 charged particles known as hadrons, which were mainly scattered along the transverse plane, immediately around the main collision point.

Compared with the collider's first run, at an energy intensity of 7 TeV, the recent experiment at 13 TeV produced 30 percent more particles per collision.

Lee says the results support the theory that higher-energy collisions may increase the chance of finding new particles. The results also provide a precise picture of a typical proton collision - a picture that may help scientists sift through average events looking for atypical particles.

"At this high intensity, we will observe hundreds of millions of collisions each second," Lee says. "But the problem is, almost all of these collisions are typical background events. You really need to understand the background well, so you can separate it from the signals for new physics effects. Now we've prepared ourselves for the potential discovery of new particles."

Shrinking the uncertainty of tiny collisions
Normally, 13 TeV is not a large amount of energy - about that expended by a flying mosquito. But when that energy is packed into a single proton, less than a trillionth the size of a mosquito, that particle's energy density becomes enormous. When two such energy-packed protons smash into each other, they can knock off constituents from each proton - either quarks or gluons - that may, in turn, interact to produce entirely new particles.

Predicting the number of particles produced by a proton collision could help scientists determine the probability of detecting a new particle. However, existing models generate predictions with an uncertainty of 30 to 40 percent. That means that for high-energy collisions that produce a large number of particles, the uncertainty of detecting rare particles can be a considerable problem.

"For high-luminosity runs, you might have up to 100 collisions, and the uncertainty of the background level, based on existing models, would be very big," Lee says.

To shrink this uncertainty and more precisely count the number of particles produced in an average proton collision, Lee and his team used the Large Hadron Collider's CMS detector. The detector is built around a massive magnet that can generate a field that's 100,000 times stronger than the Earth's magnetic field.

Typically, a magnetic field acts to bend charged particles that are produced by proton collisions. This bending allows scientists to measure a particle's momentum. However, an average collision typically produces lightweight particles with very low momentum - particles that, in a magnetic field, end up coiling their way toward the main collider's beam pipe, instead of bending toward the CMS detector.

To count these charged, lightweight particles, the scientists analyzed the data with the detector's magnet off. While they couldn't measure the particles' momentum, they could precisely count the number of charged particles, and measure the angles at which they arrived at the detector. The measurements, Lee says, give a more accurate picture of an average proton collision, compared with existing theoretical models.

"Our measurement actually shrinks the uncertainty dramatically, to just a few percent," Lee says.

Simulating the early universe
Knowing what a typical proton collision looks like will help scientists set the collider to essentially see through the background of average events, to more efficiently detect rare particles.

Lee says the new results may also have a significant impact on the study of the hot and dense medium from the early universe. In addition to proton collisions, scientists also plan to study the highest-energy collisions of lead ions, each of which contain 208 protons and neutrons. When accelerated in a collider, lead ions flatten into disks due to a force called the Lorentz contraction. When smashed together, lead ions can generate hundreds of interactions between protons and produce an extremely dense medium that is thought to mimic the conditions of space just after the Big Bang. In this way, the Large Hadron Collider experiment could potentially simulate the condition of the very first moments of the early universe.

"One microsecond after the Big Bang, the universe was very dense and hot - about 1 trillion degrees," Lee says. "With lead ion collisions, we can reproduce the early universe in a 'small bang.' If we can understand what one proton collision looks like, we may be able to get some more insights about what will happen when hundreds of them occur at the same time. Then we can see what we can learn about the early universe."


Thanks for being here;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.
SpaceDaily Contributor
$5 Billed Once


credit card or paypal
SpaceDaily Monthly Supporter
$5 Billed Monthly


paypal only


.


Related Links
Massachusetts Institute of Technology
Understanding Time and Space






Comment on this article via your Facebook, Yahoo, AOL, Hotmail login.

Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle

Previous Report
TIME AND SPACE
A resonator for electrons
Zurich, Switzerland (SPX) Oct 15, 2015
More than two thousand years ago the Greek inventor and philosopher Archimedes already came up with the idea of using a curved mirror to reflect light in such a way as to focus it into a point - legend has it that he used this technique to set fire to the ships of the Roman enemies. Today such curved or parabolic mirrors are used in a host of technical applications ranging from satellite dishes ... read more


TIME AND SPACE
New UT study highlights environmental, economic shortcomings of federal biofuel laws

Light emitting diodes made from food and beverage waste

Study: Africa's urban waste could produce rural electricity

Researchers create inside-out plants to watch how cellulose forms

TIME AND SPACE
Robots are learning to fall with grace

More-flexible machine learning

Psychic robot will know what you really meant to do

Bio-inspired robotic finger looks, feels and works like the real thing

TIME AND SPACE
Adwen and IWES sign agreement for the testing of 8MW turbine

US has fallen behind in offshore wind power

Moventas rolls out breakthrough up-tower planetary repairs for GE fleet

Chinese firm invests in Mexican wind power projects

TIME AND SPACE
French love affair with diesel set to end

Tesla cars can now almost drive themselves

Uber slip exposes data of some US drivers

VW to recall 8.5 mn vehicles in Europe as Italian police raid offices

TIME AND SPACE
Single atom alloy platinum-copper catalysts cut costs, boost green tech

Geothermal energy: Look to the Denver-Julesberg Basin

Knit it, braid it, turn it on and use it!

New Oregon approach for 'nanohoops' could energize future devices

TIME AND SPACE
Japan restarts second reactor despite opposition

Nuclear waste ship leaves France for Australia

Sweden to close two more nuclear reactors

Russia, China Plan to Develop Nuclear Markets Globally

TIME AND SPACE
To reach CO2, energy goals, combine technologies with stable policies

EDF for carbon price floor

Shift from fossil fuels risks popping 'carbon bubble': World Bank

DOE selects UC Berkeley to lead US-China energy and water consortium

TIME AND SPACE
Could contaminated land actually be good for trees

Rising seas will drown mangrove forests

Climbing plants disturb carbon storage in tropical forests

Extreme Amazon weather could have global climate consequences









The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us.