{"id":6433,"date":"2015-10-17T06:01:07","date_gmt":"2015-10-17T06:01:07","guid":{"rendered":"http:\/\/revoscience.com\/en\/?p=6433"},"modified":"2015-10-17T06:01:07","modified_gmt":"2015-10-17T06:01:07","slug":"scientists-precisely-count-particles-produced-in-a-typical-proton-collision","status":"publish","type":"post","link":"https:\/\/www.revoscience.com\/en\/scientists-precisely-count-particles-produced-in-a-typical-proton-collision\/","title":{"rendered":"Scientists precisely count particles produced in a typical proton collision."},"content":{"rendered":"<figure id=\"attachment_6434\" aria-describedby=\"caption-attachment-6434\" style=\"width: 639px\" class=\"wp-caption alignnone\"><a href=\"http:\/\/revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-6434\" src=\"http:\/\/revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg\" alt=\"Particles created from the proton collision stream out from the center of the Compact Muon Solenoid detector. They are first detected by the Silicon Tracker, whose data can be used to reconstruct the particle trajectories, indicated by yellow lines. An Electromagnetic Calorimeter detects energy deposited by electrons and photons, indicated by green boxes. The energy detected by the Hadronic Calorimeter, the primary component of jets, is indicated by blue boxes. Particles reaching the outermost parts of the detector are indicated in red. Image: CERN\" width=\"639\" height=\"426\" title=\"\" srcset=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg 639w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0-300x200.jpg 300w\" sizes=\"auto, (max-width: 639px) 100vw, 639px\" \/><\/a><figcaption id=\"caption-attachment-6434\" class=\"wp-caption-text\">Particles created from the proton collision stream out from the center of the Compact Muon Solenoid detector. They are first detected by the Silicon Tracker, whose data can be used to reconstruct the particle trajectories, indicated by yellow lines. An Electromagnetic Calorimeter detects energy deposited by electrons and photons, indicated by green boxes. The energy detected by the Hadronic Calorimeter, the primary component of jets, is indicated by blue boxes. Particles reaching the outermost parts of the detector are indicated in red.<br \/>Image: CERN<\/figcaption><\/figure>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">CAMBRIDGE, Mass. &#8212;\u00a0After 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) \u2014 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.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">In a paper to appear in the journal\u00a0<em>Physics Letters B,<\/em>\u00a0the Compact Muon Solenoid (CMS) collaboration at the European Organization for Nuclear Research (CERN) reports on the run\u2019s 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\u2019s Relativistic Heavy Ion Group, together with physics professors Gunther Roland and Bolek Wyslouch.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">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 \u201csnapshots\u201d of the interacting proton beams, and identified 150,000 events containing proton-proton collisions.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">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.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">Compared with the collider\u2019s first run, at an energy intensity of 7 TeV, the recent experiment at 13 TeV produced 30 percent more particles per collision.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">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 \u2014 a picture that may help scientists sift through average events looking for atypical particles.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">\u201cAt this high intensity, we will observe hundreds of millions of collisions each second,\u201d Lee says. \u201cBut 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\u2019ve prepared ourselves for the potential discovery of new particles.\u201d<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\"><strong>Shrinking the uncertainty of tiny collisions<\/strong><\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">Normally, 13 TeV is not a large amount of energy \u2014 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\u2019s energy density becomes enormous. When two such energy-packed protons smash into each other, they can knock off constituents from each proton \u2014 either quarks or gluons \u2014 that may, in turn, interact to produce entirely new particles.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">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.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\">[pullquote]\u201cFor 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,\u201d Lee says.[\/pullquote]<\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">\u201cFor 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,\u201d Lee says.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">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\u2019s CMS detector. The detector is built around a massive magnet that can generate a field that\u2019s 100,000 times stronger than the Earth\u2019s magnetic field.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">Typically, a magnetic field acts to bend charged particles that are produced by proton collisions. This bending allows scientists to measure a particle\u2019s momentum. However, an average collision typically produces lightweight particles with very low momentum \u2014 particles that, in a magnetic field, end up coiling their way toward the main collider\u2019s beam pipe, instead of bending toward the CMS detector.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">To count these charged, lightweight particles, the scientists analyzed the data with the detector\u2019s magnet off. While they couldn\u2019t measure the particles\u2019 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.\u00a0\u00a0<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">\u201cOur measurement actually shrinks the uncertainty dramatically, to just a few percent,\u201d Lee says.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\"><strong>Simulating the early universe<\/strong><\/span><\/p>\n<p style=\"color: #222222; text-align: left;\"><span style=\"color: #000000;\">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.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">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.<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">\u201cOne microsecond after the Big Bang, the universe was very dense and hot \u2014 about 1 trillion degrees,\u201d Lee says. \u201cWith lead ion collisions, we can reproduce the early universe in a \u2018small bang.\u2019 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.\u201d<\/span><\/p>\n<p style=\"color: rgb(34, 34, 34); text-align: justify;\"><span style=\"color: #000000;\">This research was funded, in part, by the U.S. Department of Energy.<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>CAMBRIDGE, Mass. &#8212; 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) \u2014 the highest energy ever achieved in a laboratory. <\/p>\n","protected":false},"author":2,"featured_media":6434,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[17],"tags":[],"class_list":["post-6433","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-research"],"featured_image_urls":{"full":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",639,426,false],"thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0-150x150.jpg",150,150,true],"medium":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0-300x200.jpg",300,200,true],"medium_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",639,426,false],"large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",639,426,false],"1536x1536":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",639,426,false],"2048x2048":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",639,426,false],"ultp_layout_landscape_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",639,426,false],"ultp_layout_landscape":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",639,426,false],"ultp_layout_portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",600,400,false],"ultp_layout_square":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",600,400,false],"newspaper-x-single-post":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",639,426,false],"newspaper-x-recent-post-big":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",540,360,false],"newspaper-x-recent-post-list-image":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",95,63,false],"web-stories-poster-portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",639,426,false],"web-stories-publisher-logo":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",96,64,false],"web-stories-thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/10\/MIT-Proton-Collision_0.jpg",150,100,false]},"author_info":{"info":["RevoScience"]},"category_info":"<a href=\"https:\/\/www.revoscience.com\/en\/category\/news\/research\/\" rel=\"category tag\">Research<\/a>","tag_info":"Research","comment_count":"0","_links":{"self":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/6433","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/comments?post=6433"}],"version-history":[{"count":0,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/6433\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media\/6434"}],"wp:attachment":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media?parent=6433"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/categories?post=6433"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/tags?post=6433"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}