Experimenting with 40 trillion electron-volts: it takes hundred of physicists several years to design experimental detectors for the Superconducting Super Collider.Experimenting With 40 Trillion Electron-Volts
With much of the emphasis recently on the competition among 25 states to be the site of the proposed Superconducting Super Collider
The Superconducting Super Collider (SSC) was a ring particle accelerator which was planned to be built in the area around Waxahachie, Texas. (SN: 9/12/87, p. 167), the ambitious physics of the project tends to get lost. But to anyone involved in particle physics particle physics
or high-energy physics
Study of the fundamental subatomic particles, including both matter (and antimatter) and the carrier particles of the fundamental interactions as described by quantum field theory. , the SSC SSC Secondary School Certificate
SSC Standard Systems Center (USAF)
SSC State Services Commission (New Zealand)
SSC Swedish Space Corporation
SSC Salem State College (Massachusetts) involves a fantastic amount of energy, and physicists' eyes tend to gleam as they talk about what they will do with it--or rather, what nature will do with it while they watch. Each head-on collision A head-on collision is one where the front ends of two ships, trains, planes or vehicles hit each other, as opposed to a side-collision or rear-end collision. Rail transport
With rail, a head-on collision often implies a collision on a single line railway. of two protons in the SSC would provide 40 trillion electron-volts (40 GeV) of energy. That's 40,000 times the mass of a proton.
For several years now, particle physicists have gathered for a couple of weeks each summer to work out their ideas on how to design the equipment that will record the results of those collisions, and gradually the designs are beginning to jell. This year's Workshop on Experiments, Detectors and Experimental Areas for the Super Collider col`lid´er
n. 1. (Physics) a
See also Berzerkley, BSD.
Note to British and Commonwealth readers: that's /berk'lee/, not /bark'lee/ as in British Received Pronunciation. , produced drawings of large pieces of experimental equipment that seem to be settling into basic categories.
The installations the experimenters discuss are large and complicated. As Roger Cashmore Roger John Cashmore CMG is Principal of Brasenose College, Oxford and Professor of Experimental Physics in the University of Oxford.
His interests include the origin of the masses of particles and the Higgs boson.
Cashmore was born on 22 August 1944. of the Fermi National Accelerator Laboratory Fermi National Accelerator Laboratory (Fermilab), physical science research center located near Batavia, Ill., est. 1968 as the National Accelerator Laboratory, renamed 1974 in honor of Enrico Fermi. It was built on the site of the former village of Weston. in Batavia, Ill., points out, it takes about five years to build one of these detectors. If construction of the SSC goes forward on schedule, completion is expected in 1996. Therefore, in a couple of years physicists will have to develop these concepts into plans out of which hardware can be made.
They are not there yet, but scientists are standing at blackboards drawing up arrangements of different elements they think they need. As they do, they get sardonic comments from the audience:
"Amazing,' says one observer, "how they plan to levitate lev·i·tate
intr. & tr.v. lev·i·tat·ed, lev·i·tat·ing, lev·i·tates
To rise or cause to rise into the air and float in apparent defiance of gravity. a heavy magnet like that!'
"They intend it to be superconducting,' says another, pushing in the needle a little farther.
Yes, they intend it to be superconducting, but no, they do not intend to levitate many tons of magnet by the Meissner effect Meissner effect
The expulsion of magnetic flux from the interior of a superconducting metal when it is cooled in a magnetic field to below the critical temperature, near absolute zero, at which the transition to superconductivity takes place. . (A piece of metal in a superconducting state will expel a magnetic field from within itself. As has been demonstrated recently in television news reports of the new high-temperature super-conductors, the repulsion repulsion /re·pul·sion/ (re-pul´shun)
1. the act of driving apart or away; a force that tends to drive two bodies apart.
2. so generated will levitate a small object.) As Cashmore points out, "These things "These Things" is an EP by She Wants Revenge, released in 2005 by Perfect Kiss, a subsidiary of Geffen Records. Music Video
The music video stars Shirley Manson, lead singer of the band Garbage. Track Listing
1. "These Things [Radio Edit]" - 3:17
2. don't just float in midair.' There is a lot of engineering design to be done, and that could require tradeoffs with characteristics important to the data-taking. Particularly, the supports for heavy items like magnets could invade and degrade the hermeticity, the self-contained and sealed-off character, that experimental physicists desire in elements of the detecting equipment.
The physicists want the detectors to be able to identify the stable and the fairly long-lived radioactive particles that come out of the proton-proton collisions and determine the energies they carry and the size and direction of their momenta. Most of the unknown particles they seek will be too short-lived to make much direct impression on the detectors, so the presence of any of them will be revealed by the identity and behavior of its decay products. The name of the game is by their fruits shall ye know them.
The list of things they want to look for is fairly long. All these things are apparently heavier than particles now known and so require more energy for their production. Some of the things on the list would contribute to a rounding out and deeper understanding of the present "standard model,' which contains successful theories of two important parts of particle physics. Others pertain to pertain to
verb relate to, concern, refer to, regard, be part of, belong to, apply to, bear on, befit, be relevant to, be appropriate to, appertain to attempts to go beyond the standard model to unite its elements with explanations of phenomena not now included and produce a more comprehensive theory. Finally, some theoretical exercises seek to go below the standard model to see whether there is a level of reality and structure below the most basic one now contemplated by the standard model.
One part of the standard model is the theory known as quantum chromodynamics quantum chromodynamics (QCD), quantum field theory that describes the properties of the strong interactions between quarks and between protons and neutrons in the framework of quantum theory. . This deals with quarks, the particles made out of quarks (which are all but a dozen of the known particles) and the force that animates them, the short-range "strong' force or strong interaction. The other part of the model is the theory called electroweak e·lec·tro·weak
Of or relating to the combination of the electromagnetic and weak nuclear forces in a unified theory. or sometimes electroasthenodynamics, which covers particles and phenomena animated by the electromagnetic force electromagnetic force
One of the four known basic forces in the universe. Electromagnetism is responsible for interactions between charged particles that occur because of their charge, and for the emission and absorption of photons (electromagnetic radiation). and the other kind of short-range force, the "weak' interaction.
Related to the standard model are searches for new kinds of quarks, particularly for heavy kinds. Some physicists still hope to find free quarks, although the usual theory says quarks cannot be free. Experimenters talk of looking for Looking for
In the context of general equities, this describing a buy interest in which a dealer is asked to offer stock, often involving a capital commitment. Antithesis of in touch with. gluons Gluons
The hypothetical force particles believed to bind quarks into “elementary” particles. Although theoretical models in which the strong interactions of quarks are mediated by gluons have been successful in predicting, interpreting, and , the particles that embody the strong force and carry it from place to place. They also want to study the detailed physics of things now known but on the edge of current experimental capability.
One such instance is the "b' quark, the heaviest now definitely known. At the workshop many physicists spoke of the importance of studying the behavior of the B particles, the family of things made from b quarks. Another example is the z and w particles that play a central role in electroweak theory. How do they behave in detail? Are there more of them than we now know--heavier ones, perhaps?
The icing on the cake, so to speak, is the Higgs particles. One of the important unsolved questions is how different particles get mass and how each kind gets the specific amount it has. At the basis of the standard model is a mechanism, the Higgs mechanism, that purports to deal with the question of how mass comes about. If the Higgs mechanism exists, then a family of particles, presumably pre·sum·a·ble
That can be presumed or taken for granted; reasonable as a supposition: presumable causes of the disaster. very heavy particles, called the Higgs particles, exists. Finding them would cause great rejoicing among physicists.
Going beyond the standard model, supersymmetry Supersymmetry
A conjectured enhanced symmetry of the laws of nature that would relate two fundamental observed classes of particles, bosons and fermions. theory attempts to unite the standard model with phenomena controlled by the force of gravity. It gets its name because it proposes that for every particle known to the standard model there exists a supersymmetric partner that has the same properties but obeys the opposite of the two kinds of statistical law that apply to subatomic particles, Bose-Einstein statistics and Fermi-Dirac statistics. Many want to search for these supersymmetric partners, particularly those corresponding to particles that play important roles in the standard model. These partners would be photinos, gluinos, squarks, sleptonz, zuinos and winos (pronounced "weenos').
Underneath the standard model is the realm of "compositeness.' The standard model holds that everything is built out of six kinds of quarks and six kinds of leptons, and that these quarks and leptons are the most elementary forms of matter. Up to now, whenever physicists have thought they had reached the most elementary constituents of matter, they have been proven wrong. There is a faction of theorists who think they are still wrong. Believers in compositeness say the quarks and leptons are themselves composite, made of more elementary objects, which may be called preons or technicolor quarks or something else.
In addition to all this are things that even theoretical physicists call exotic, but that nevertheless may exist. Summing up for the working group that considered exotic particles, Allan Litke of the University of California The University of California has a combined student body of more than 191,000 students, over 1,340,000 living alumni, and a combined systemwide and campus endowment of just over $7.3 billion (8th largest in the United States). at Santa Cruz said, "The search for exotics must proceed. The impact is so great.' He cited a new energy range and the possibility of new physics and big surprises as reasons for it.
Litke specifically mentioned attempting to detect magnetic monopoles, free quarks, new kinds of heavy quarks and heavy stable particles. Physics now knows two kinds of stable particles, protons and electrons, which, with neutrons, are the constituents of ordinary atoms. The heavy stable particles would be at least 100 times as heavy as protons. They would have lifetimes greater than 10 million seconds (about 116 days), which amounts to stability compared to the millisecond One thousandth of a second. See space/time and ohnosecond.
(unit) millisecond - (ms) One thousandth of a second, one thousand microseconds. A long time for a modern computer. , microsecond One millionth of a second. See space/time and ohnosecond.
(unit) microsecond - One millionth (10^-6) of a second. and shorter existences of typical unstable particles. This would be a strange new kind of matter indeed.
At the workshop, each important family of particles--the Higgses, the Bs, the supersymmetry particles, and so on-- had a small group of physicists that discussed how best to study it. Then the groups dealing with specific particles got together with hardware specialists and fed their requirements into possible designs for general-purpose detectors.
These general-purpose detectors are usually called "four-pi' detectors because they aim to surround one of the six proton-proton collision points in the SSC as completely as possible with detecting equipment. "Four-pi' is mathematical jargon for a complete sphere. These detector designs have evolved over the years, and they will probably continue to evolve until the hardware is finally screwed down--or maybe until it is torn down. (One proposed design from previous years was completely junked at this year's meeting.)
The changes arise from new discoveries in ongoing experimental physics, from new theoretical insights and from developments in detecting technology. In this year's workshop, as in those of previous years and perhaps those also of a couple of years to come, the sessions in which the physicists considering particular kinds of particles got together with the hardware specialists tended to begin with someone going to the blackboard to draw as the others called out their desires for this or that piece of equipment.
In one such session, consideration started with the calorimeter calorimeter: see calorimetry.
Device for measuring heat produced during a mechanical, electrical, or chemical reaction and for calculating the heat capacity of materials. that forms the centerpiece of each of these designs. This one was 2 meters in radius and 12 meters long--through some in the group thought it might be made shorter. A calorimeter consists of alternating layers of something dense and heavy like uranium that takes energy from passing particles and so enables observers to calculate how much energy they started with, and something that records the particles' presence. Inside the 2 meters of this calorimeter there will also be equipment to image the tracks of the particles. The consensus was that 1.5 meters of depth would be required for the tracking. The woman at the board drew it in.
Someone mentioned a flux return. This calorimeter will have a solenoidal magnetic field provided by a 7-meter super-conducting coil. The field will bend the trajectories of electrically charged particles and aid their identification and measurement. The field must loop back outside the calorimeter and rejoin itself at the other end. In the open it could interfere with equipment placed outside the calorimeter. A lot of iron is provided to confine it. Add half a meter for the coil and a meter of iron for the flux return.
"Do we need to go beyond a calorimeter and tracking?' someone asked.
People interested in B particles and Higgs particles definitely want more. They want to be able to discriminate electrons and muons from the background. So 3 more meters of muon muon (my`ŏn), elementary particle heavier than an electron but lighter than other particles having nonzero rest mass. identifiers were added. The sketch then called for an object 16 meters in diameter and more than 12 meters long when end pieces are added. This is a small one. The other four are larger. All but one have magnetic calorimeters.
Questions of adjustment and accommodation continually arise in these discussions. As one discussion leader put it, "What components of the detector would you least like to give up? Suppose we came back and said the momentum resolution had to be poorer. How much compromise would you be willing to make?'
These large detectors are beginning to have family resemblances. Advocates of a dipole magnetic field point out that the UA1 detector that has done outstanding work at the CERN CERN or European Organization for Nuclear Research, nuclear and particle physics research center straddling the French-Swiss border W of Geneva, Switzerland. laboratory in Geneva Geneva, canton and city, Switzerland
Geneva (jənē`və), Fr. Genève, canton (1990 pop. 373,019), 109 sq mi (282 sq km), SW Switzerland, surrounding the southwest tip of the Lake of Geneva. , Switzerland, is a dipole. Another CERN detector, L3 (SN: 1/19/85, p.45), which is being built for CERN's new collider LEP (Light Emitting Polymer) An organic polymer that glows (emits photons) when excited by electricity. LEP screens are used to make organic LED (OLED) displays and are expected to compete with LCD screens in the future. See OLED. , may have an offspring at the SSC. Samuel C.C. Ting of CERN described the proposal, which proponents call L3 1. "We're not good at naming these things,' Ting confides. "We were never able to find a correct name.'
L3, which is well on the way to completion, involves 440 physicists, represents an international industrial effort and will contain more iron than the Eiffel Tower. According to Ting, L3 1 will be even more collossal. An attempt to provide precision lepton lepton (lĕp`tŏn') [Gr.,=light (i.e., lightweight)], class of elementary particles that includes the electron and its antiparticle, the muon and its antiparticle, the tau and its antiparticle, and the neutrino and antineutrino associated with (electron and muon) detection in the trillion-volt energy region, it will be an experiment lasting 10 years and involving "God knows how many physicists.'
Ting and others believe that precise measurement of leptons will be an important way of discovering new phenomena at these ultrahigh ul·tra·high
Exceedingly high: an ultrahigh vacuum. energies. To do it, L3 1 will put lepton identifiers around a 17,700-ton magnet, which will provide a 7,500-gauss magnetic field in a 300-ton calorimeter. The whole detector will be 23.8 meters high and 20.8 meters long, using 27,500 tons of iron. They estimate a cost of $93 million.
In his summary talk Cashmore rated each of the proposed general-purpose detectors on a scale of 10 for each of its important characteristics. When he had added and weighted all the scores, all five detectors came out more or less even. Time and the development of detail will indicate preferences, he said.
As these are items whose cost goes into the hundreds of millions of dollars, an important question is how many of them the SSC will need. Obviously one, says Cashmore, and preferably at least two. There will probably never be another accelerator equal to the SSC in energy, he notes, so it would be good to have at least two independent detectors to confirm each other's discoveries.