
<p>International Journal of Mo dern <a href="/tags/Physics/" rel="tag">Physics</a> A</p><p> f</p><p> cWorld Scientic Publishing Company</p><p>JETS AND KINEMATICS IN HADRONIC COLLISIONS</p><p>ANDREW R BADEN</p><p>Physics Department University of Maryland</p><p>Col lege Park MD USA</p><p>Received September </p><p>Revised Decemb er </p><p>Analysis of collidingb eam hadron exp eriments p p X and p p X often dep end</p><p> up on observation of jets a highly collimated spray of particles suchas Keand</p><p> s forming clusters of energy dep osition in calorimeters In this pap er we outline howto</p><p> dene jets from such clusters and discuss the meaning of jet quantities such as transverse</p><p> energy and mass Data from the D exp eriment are used to illustrate these concepts In</p><p> addition we review the motivations for using certain optimal co ordinates for describing</p><p> energy<a href="/tags/Momentum/" rel="tag">momentum</a> vectors and deriveinteresting relationships among the kinematic</p><p> variables</p><p> Kinematics of Hadron Collider Events</p><p>To motivate some of the kinematic quantities traditionally used to describ e p p</p><p> p</p><p> exp eriments one must rst recognize that the centerofmass energy s of the</p><p> scattering in these exp eriments centers is not xed This is a direct consequence of</p><p></p><p> the proton substructure where the scattering constituents are quarks and gluons</p><p> that reside inside the nucleons with each parton carrying a fraction x of the total</p><p> nucleon energy Scattering of partons of dierent energy results in a centerof</p><p> momentum that do es not necessarily coincide with the lab oratory frame A lackof</p><p> knowledge of the centerofmass energy guides the choice of kinematic variables</p><p> Phase SpaceVolume</p><p>We start with the denition of a relativistically invariant phase <a href="/tags/Space_(mathematics)/" rel="tag">space</a> volume d</p><p></p><p> for an ob ject of momentum p and energy E For a xed particle mass d can b e</p><p></p><p> written as see </p><p></p><p> dp dp dp d p</p><p> x y z</p><p> d </p><p>E E</p><p>Dening z as the pp collision axis we see that of the momentum co ordinates</p><p> p p p and E only the rst two are invariant with resp ect to a Lorentz transfor</p><p> x y z</p><p> mation from the lab frame along the z direction by virtue of their direction b eing</p><p> normal to that of the b o ost In addition we see that even though the co ordinates p</p><p> and are not invariant with resp ect to b o osts along zinvariance will b e preserved</p><p> in the pro duct p cos sin whichisp </p><p> x</p><p>Achoice of momentum co ordinates which more explicitly reect the Lorentz</p><p> invariance of the phase space elementisp ym where p is the momentum</p><p>T T</p><p> transverse to z direction is the azimuthal angle ab out z m is the mass and y is</p><p> the rapidity along the z direction dened as </p><p> Jets and Kinematics in Hadronic Col lisions</p><p> E p cos </p><p> z</p><p> y ln ln </p><p> E p cos </p><p> z</p><p> or equivalently</p><p> cos tanh y </p><p> where pE and is as ab ove the p olar pro duction angle relativetothez</p><p> axis For a b o ost along thez direction with some a transformation from</p><p> b</p><p> the lab frame to the new frame will change the rapidity as follows</p><p> y y y</p><p> b</p><p> where</p><p> y ln </p><p> b b b</p><p>Because cos for b o osts along z it follows that</p><p> tanhy </p><p> b b</p><p>The advantage of using the ab ove set of co ordinates is clear the eect of a b o ost</p><p> along the z axis changes only y and that by only an additive constant</p><p>To calculate d in these co ordinates we rst dierentiate Eq </p><p> </p><p>y y E</p><p> dy dp </p><p> z</p><p>p E p</p><p> z z</p><p> </p><p> p p E</p><p> z z</p><p> dp</p><p> z</p><p> </p><p>E p E p E</p><p> z z</p><p> which simplies to</p><p> dp</p><p> z</p><p> dy </p><p>E</p><p>The comp onents dp and dp are related to the elements dp and d via a trans</p><p> x y T</p><p> formation from cartesian to p olar co ordinates in dimensions</p><p></p><p></p><p> d dp dp p dp d dp</p><p> x y T T</p><p>T</p><p></p><p>We can now write the volume element d as</p><p></p><p></p><p> dp dy d d </p><p>T</p><p></p><p>Thus particles pro duced in pro cesses that have a matrix elementthatvaries slowly</p><p> with rapidityy should b e distributed uniformly in y This is the origin of the</p><p></p><p>rapidity plateau for singleparticle pro duction in hadronic collisions</p><p>Our chosen set of kinematic co ordinates is well suited to the analysis of physics</p><p> issues and is used extensively to describ e the results of measurements in high energy</p><p> physics In the following subsections wedevelop formulae and relationships among</p><p> p y andm and other quantities of interest</p><p>T</p><p> Transverse Energy E and Momentum p </p><p>T T</p><p>Jets and Kinematics in Hadronic Col lisions </p><p>One can dene the transverse energy E of a particle as its energy in the rest</p><p>T</p><p> frame where its p Because this quantityisinvariant to boosts along zwe can</p><p> z</p><p> write in general</p><p> </p><p>E p p m p m E p </p><p>T x y T z</p><p>From Eq we can solve for p yielding</p><p> z</p><p> p E tanh y </p><p> z</p><p>Combining the ab ovetwo equations gives</p><p></p><p> </p><p>E E E tanh y</p><p>T</p><p></p><p></p><p> E tanh y </p><p></p><p></p><p> E cosh y</p><p> or equiv alently</p><p>E E cosh y </p><p>T</p><p>Note that the p is always dened in terms of the momentum p as</p><p>T</p><p> p p sin </p><p>T</p><p>We wish to stress that these two relativistically invariantquantities E and p </p><p>T T</p><p> are not dened in the same way that is E E sin More on this b elow</p><p>T</p><p>Combining Eq and gives</p><p> p E sinh y </p><p> z T</p><p> Invariant Mass</p><p>The invariant mass of two particles is dened as</p><p> </p><p></p><p>M p p p p </p><p> </p><p></p><p> </p><p> </p><p> </p><p>E E p p m m</p><p> </p><p> </p><p>Using the p y and mvariables and applying equations from the pro ceeding</p><p>T</p><p> sections we calculate</p><p>E E E cosh y E cosh y </p><p> T T </p><p> and</p><p> </p><p> p p p p p p p p</p><p> x x y y z z </p><p> p cos p cos p sin p sin p p</p><p>T T T T z z </p><p> p p cos p p</p><p>T T z z </p><p> p p cos E sinh y E sinh y</p><p>T T T T </p><p> E E cos sinh y sinh y </p><p>T T T T </p><p> where p E sin cosh y and </p><p>T T T </p><p>Combining the ab ove results gives</p><p> Jets and Kinematics in Hadronic Col lisions</p><p> </p><p>M m m E E cosh y cos </p><p> t t t t</p><p> </p><p> where y y y and cosh y cosh y cosh y sinh y sinh y We will discuss</p><p> </p><p> the consequences of Eq in the limit in a subsequent section</p><p> PseudoRapidity</p><p>In order to determine the rapidity of a particle one needs b oth its cos and velo city</p><p> Since the velo city requires measuring b oth E and the mass m this precludes</p><p> using a single detector comp onent to measure rapidityHowever in the limit of</p><p> or m p Eq b ecomes cos tanhy which often pro vides an</p><p>T</p><p> excellentapproximation to use for the rapidityWe therefore dene the pseudo</p><p> rapidity as the rapidity of a particle with zero mass or y j </p><p> m</p><p>Using Eq for y and setting one obtains</p><p> cos </p><p> ln ln tan </p><p> cos </p><p> and the inverse equation which is often useful</p><p> cos tanh </p><p>Eliminating cos from Eqs and wehave the relationship</p><p> tanh y tanh </p><p>This last equation shows clearly that in the limit m or wehave y </p><p>The pseudorapidity dened to b e indep endentof is therefore another wayto</p><p> measure the lo cation of a particle equivalent to measuring its p olar angle In</p><p> addition we can use Eq to derive the transformation</p><p> d sin d d cosh </p><p>Since is always and the function tanhx is monotonic the pseudorapidity</p><p> j j of a particle of given p is larger than its true rapidity jy j Figure shows the</p><p>T</p><p> dierence b etween and y as a function of for protons for several choices of</p><p> constant p and Figure shows a similar plot for pions In each plot a dashed</p><p>T</p><p> line is drawn at constant j jjy j corresp onding to the size of the calorimeter</p><p></p><p> readout pad at D Rapidity and pseudorapidity are equal to within for pion</p><p> p of GeVc and proton p of GeVc for all This means that one</p><p>T T</p><p> can use in place of y in kinematic calculations involving pions and protons in this</p><p> range of p values</p><p>T</p><p>It is imp ortant to recall that for xed p the velo city is a function of pseudo</p><p>T</p><p> p</p><p> </p><p> rapidity To see the explicit form we start with pE E p m use</p><p>Eq for p and Eq to relate to to get</p><p>T</p><p> p</p><p>T</p><p> p</p><p> </p><p></p><p> </p><p> m tanh E</p><p>T</p><p> which gives</p><p> p tanh </p><p>T</p><p> q</p><p> tanh y </p><p></p><p></p><p></p><p> m tanh E</p><p>T</p><p>Given the fact that j jjy jwewould exp ect that for xed p any single</p><p>T</p><p> particle sp ectrum that is indep endentofy d dy is constant would b ecome de</p><p> pleted in the central region when plotting as a function of Thistyp e of eect</p><p> would b e esp ecially large for particles with low p and signicant mass T</p><p>Jets and Kinematics in Hadronic Col lisions </p><p>Fig j j jy j for protons at various p </p><p>T</p><p>Fig j j jy j for pions at various p T</p><p> Jets and Kinematics in Hadronic Col lisions</p><p> d dy dy d</p><p> k </p><p> d dy d d</p><p> where k is a constant An analytic form for dy d can b e derived starting with Eq</p><p> substituting for using Eq dierentiating and rearranging terms to get</p><p> the result that</p><p> dy</p><p> </p><p> d</p><p> with given by Eq This result although somewhat surprising can b e</p><p> understo o d in the following sense at large y and therefore large the function</p><p> tanh y converges to Hence for large y b oth the tanh y and tanh converge to</p><p> which means whichwould b e true for large p and xed p In this case</p><p>T</p><p> there is little if any functional dep endence of y on Atsmally we can use the</p><p> approximation tanh y y and tanh to get the relation y whichgives</p><p> dy d We therefore exp ect dy d to b e constant for large y or with</p><p> all of the dep endence coming at small </p><p></p><p>Figure shows a histogram of dN d for pions generated with constant</p><p> p GeVc and uniformly in dN dy The smo oth curve is the function </p><p>T</p><p> that is dy d for pions with xed p GeVc</p><p>T</p><p>Fig The histogram shows dy d for pions generated uniformly in rapidity y with xed p </p><p>T</p><p>GeVc The smo oth curve is the corresp onding function </p><p> Invariant Masses for </p><p>In the limit m y and We can then write the invariantmass</p><p>T</p><p> of two massless particles using Eq as</p><p></p><p>E E cosh cos M</p><p>T T </p><p>Jets and Kinematics in Hadronic Col lisions </p><p>This expression is often quite useful as weshowbelow</p><p> Transverse Mass and Missing Transverse Energy</p><p>Noninteracting particles such as neutrinos can b e detected only via an apparent</p><p> imbalance of momentum in an event In p p or ppinteractions where most of the</p><p> longitudinal parallel to the b eam z momentum in the collision is lost down the</p><p> b eam pip e it is essentially imp ossible to measure momentum conservation along z</p><p>However given a detector with suciently large acceptance measuring momentum</p><p> balance in the plane transverse to the b eam direction is relatively straightforward</p><p>Thus that amount of transverse momentum required to satisfy momentum con</p><p> servation the missing transverse momentum can b e in large part attributed to</p><p> the presence of any unobserved noninteracting particles esp ecially when the total</p><p> momentum and energy in the detector is large since for small total detected en</p><p> ergy small uctuations in the measured momentum along anygiven direction can</p><p> give a small statistically insignicant missing transverse momentum Since the</p><p> neutrino is massless certainly on these scales this quantity missing transverse</p><p> momentum is virtually equivalenttothe missing transverse energy or E in the</p><p>T</p><p> event</p><p>For particles such as the W b oson which decayinto leptonneutrino pairs the</p><p> lack of a measurementofp for the neutrino precludes a direct measurementofthe</p><p> z</p><p> invariant mass of the W However one can calculate an in variant transverse mass of</p><p> these two particles denoted by M dened as the invariant particle mass using</p><p>T</p><p> only the momentum comp onents in the transverse plane p and p i From</p><p> xi yi</p><p> this denition the transverse mass is dened as</p><p> </p><p></p><p>M p p p p </p><p>T T </p><p>T</p><p>T T </p><p></p><p></p><p> where p E p For two zeromass particles E p wehave</p><p>Ti Ti Ti Ti</p><p>Ti</p><p></p><p> </p><p> E E p p M</p><p>T T T T </p><p>T</p><p>E E cos </p><p>T T </p><p></p><p></p><p> E E sin </p><p>T T </p><p></p><p> or equivalently</p><p> p</p><p></p><p> M sin E E </p><p>T T T </p><p></p><p>We can see that this formula is equivalent to Eq with the condition </p><p> </p><p> that is the transverse mass and the invariant mass are equivalent for particles which</p><p> are pro duced at the same rapidity As such M M ignoring the</p><p>T </p><p> detector resolution and intrinsic width As a rule M will deviate from M</p><p>W T </p><p> as gets large that is as the particles decay more forwardbackward in the lab</p><p> frame Distributions in M will therefore have a tail at low M forwardbackward</p><p>T T</p><p> will p eak at M and will fall to zero ab ove M in the same manner as M </p><p> </p><p>It is imp ortant to note that these formulae require that E b e dened using Eq</p><p>T</p><p> as E sin They are equivalent only in the limit mp Of course and not</p><p>T</p><p>Eq is true in general As will b e shown b elow in the small mass limit of </p><p> the dierence b etween E and p b ecomes insignicant</p><p>T T</p><p>An interesting relationship involving the invariant mass of particles is</p><p> </p><p>M M M M m m m</p><p> </p><p> which in the limit of m becomes i</p><p> Jets and Kinematics in Hadronic Col lisions</p><p> </p><p>M M M M </p><p> </p><p>This formula is interesting to keep in mind when searching for b o dy decays say</p><p>A a b c If it is appropriate to ignore the three masses m m andm then</p><p> a b c</p><p> you do not havetoknowwhich of the three b o dies is a bor c sp ecically in order</p><p> to calculate the correct value for m you only havetoknow that these are the </p><p>A</p><p> b o dies of whichyou are interested</p><p></p><p>Lastly since the mass of the W particle is well known we can constrain the</p><p> invariantmassofthe e pair and solve for the longitudinal momentum of the</p><p> neutrino To do this we can use Eq </p><p></p><p>M E E cosh cos </p><p>T T </p><p>W</p><p>Rewriting this expression weget</p><p></p><p>M</p><p>W</p><p> cosh cos </p><p>E E</p><p>T T </p><p>Solving for gives</p><p> p</p><p></p><p> r r </p><p> ln </p><p></p><p> where r is the righthand side of Eq Because is the dierence in pseu</p><p> dorapiditybetween the electron and the neutrino there are two solutions to the</p><p> problem That is there is no way of resolving the ambiguity of whether the neu</p><p> trino is at a lower or higher rapidity relative to the electron as seen from the fact</p><p> that the hyp erb olic cosine cosh is even in Both solutions are p ossible at least</p><p> in principle</p><p> Jets</p><p> </p><p>Quantum Chromo dynamics QCD is the currently accepted theory of the strong</p><p> interaction b etween particles partons that carry color These partons quarks q</p><p> and gluons g app ear in detectors as sprays or jets of particles In this section</p><p> we will discuss issues concerning the observation of jets and their origin in QCD</p><p> Denition of a Jet</p><p>There are various ways to dene jets For instance most of the LEPPEPand</p><p></p><p>PETRA e e exp eriments dene jets using information just from tracking cham</p><p> bers One of the less ambiguous ways to dene jets is motivated bywhatwe</p><p> understand to b e the physics of fragmentation namely that a jet is the result of</p><p> the hadronization of a parent parton A way to visualize hadronization is through</p><p> wed virtual gluon emission by the parentpartonq q g and g g g follo</p><p> by gluon splitting to q q pairs forming the color singlet hadrons that we measure</p><p></p><p>For high precision studies of parton QCD fragmentation in e e collisions this</p><p> mo del is to o naive However in hadronic collisions where the presence of the soft</p><p></p><p>underlying event part of a high Q collision complicates the analysis the naive</p><p> mo del is adequate for describing how a parton turns into a jet</p><p>To see how this simple fragmentation mo del can b e related to the concept of</p><p> a jet we consider the transverse momentum k of radiated gluons relativeto</p><p>T</p><p></p><p> the jet axis The distribution of k has b een found to b e exp onential in k with</p><p>T</p><p>T</p><p> p</p><p> </p><p> and DORIS energies hk i MeVc at SPEAR s GeV increasing</p><p>T</p><p></p><p> to hk iGeV c at SppS energies We dene as the angle of the gluon with</p><p>T</p><p> resp ect to some reference in the plane p erp endicular to the momentum direction of</p><p>Jets and Kinematics in Hadronic Col lisions </p><p>Fig Radiated gluons make an angle with resp ect to an arbitrary direction in the plane</p><p> p erp endicular to the jet axis</p><p> the parent parton see Figure Since the physics of gluon radiation is indep endent</p><p> of this angle we exp ect the probability distribution for will b e uniform in The</p><p> jet axis can b e dened by a cluster of calorimeter cells less often bytracks in the</p><p></p><p> tracking chamb er in space that minimize the total vector k of the jet remnants</p><p>T</p><p>This means requiring</p><p>X</p><p></p><p> k </p><p>Ti</p><p>We can use Eq to form the jet cluster into an equivalent particle with</p><p></p><p></p><p>momentum p E p that can b e used for example to calculate an invariant</p><p> mass for example W jet jet Let us sp ecialize to calorimetry and assume that</p><p> the jet will b e constructed as a cluster of cells or towers for pro jective geometry</p><p> calorimeters If one represents the energy E in each cell of a calorimeter i as a</p><p> i</p><p></p><p>particle with zero mass one can then dene E E n where n is the unit vector</p><p> i i i i</p><p> pointing from the interaction vertex to cell i The jet is therefore dened in the rest</p><p> frame of the detector as an ob ject consisting of a set of these zero mass particles</p><p> E one p er calorimeter cell Note that this representation of and therefore p</p><p> i i</p><p> a jet using zero mass particles do es not imply that the jet also has zero mass or</p><p> p E since the constituents the cells will eachhave an op ening angle b etween</p><p> them and this op ening angle will generate a jet mass To see this explicitly</p><p> consider Eq the invariant mass of two particles If the particles have zero mass</p><p> we drop the terms m and m set E p and E p leaving</p><p> </p><p> </p><p>M E E cos E E sin </p><p> </p><p></p><p> where is the angle b etween the two particles We see clearly that if the</p><p> invariant mass is also zero</p><p> Jets and Kinematics in Hadronic Col lisions</p><p>To form a jet from these calorimeter cells wemust apply Eq relativeto</p><p> the axis that denes the jet direction The transformation of the cells to this axis</p><p> involves an Euler rotation with degrees of freedom and The rotation</p><p> jet jet</p><p></p><p> </p><p> matrix M dened by E M E is a function of the yet to b e determined Euler</p><p> i</p><p> i</p><p></p><p> angles and is given by</p><p> </p><p> sin cos </p><p> jet jet</p><p> A</p><p> cos cos cos sin sin </p><p> jet jet jet jet jet</p><p> sin cos sin sin cos </p><p> jet jet jet jet jet</p><p>The transformation equations which relate the cell energies in the frame of the jet</p><p>primed to those in the frame of the detector unprimed are therefore</p><p></p><p>E E sin E cos </p><p> xi jet yi jet</p><p> xi</p><p> E sin </p><p>Ti i</p><p></p><p> E cos cos E cos sin E sin E</p><p> xi jet jet yi jet jet zi jet</p><p> yi</p><p> cos E cos sin E</p><p> jet Ti i jet zi</p><p></p><p>E E sin cos E sin sin E cos </p><p> xi jet jet yi jet jet zi jet</p><p> zi</p><p> sin E cos cos E </p><p> jet Ti i jet zi</p><p> where E E sin and As a check of Eq we can</p><p>Ti i i i i jet</p><p> imagine a jet with a single tower which when rotated to the jet axis should retrieve</p><p> </p><p>E E and E E Thus setting remember that is the</p><p> jet</p><p> x y z</p><p></p><p> dierence in between the jet and the tower the ab ove equations yield E </p><p> x</p><p> </p><p>E E sin E cos using tan E E and E E sin </p><p> z jet T jet jet T z T jet</p><p> y z</p><p> sin and E E cos Here wehave E cos E using E E</p><p> jet z jet z jet jet T</p><p> assumed that suchahyp othetical jet would b e massless since it is contained in a</p><p> single tower allowing E p in the ab ove This is discussed further b elow</p><p> jet jet</p><p>The momentum vectors of eachtower can now b e rotated into the frame of</p><p> </p><p> the jet summed over the transverse comp onents E k and E k and</p><p> xi yi</p><p> xi yi</p><p> separately set to zero as required by Eq </p><p>X X X</p><p></p><p>E sin E cos E </p><p> jet xi jet yi</p><p> xi</p><p> i i i</p><p> and</p><p>X X</p><p></p><p> E cos cos E</p><p> xi jet jet</p><p> yi</p><p> i i</p><p>X X</p><p>E sin E cos sin </p><p> yi jet zi jet jet</p><p> i i</p><p> </p><p>We therefore havetwo equations and and two unknowns and </p><p> jet jet</p><p>Solving Eq yields the following relation</p><p>P P</p><p>E sin E</p><p>Ti i yi</p><p>P P</p><p> tan </p><p> jet</p><p>E E cos </p><p> xi Ti i</p><p>Solving Eq gives</p><p>Jets and Kinematics in Hadronic Col lisions </p><p>P P</p><p> cos E sin E</p><p> jet xi jet yi</p><p> i i</p><p>P</p><p> tan </p><p> jet</p><p>E</p><p> zi</p><p> i</p><p>Equations and describ e the co ordinates of the jet cluster in a waywhich</p><p> is consistent with the dening Eq </p><p>The jet is a true physical ob ject which mighthave originated through the show</p><p></p><p> ering of some virtual parton and it must therefore haveavector E p that</p><p> jet jet</p><p> corresp onds to an ob ject of some nite mass We can dene the angles of our jet in</p><p> the lab oratoryasfollows</p><p> p</p><p> yj et</p><p> tan </p><p> jet</p><p> p</p><p> xj et</p><p> and</p><p> p</p><p> tj et</p><p> tan </p><p> jet</p><p> p</p><p> zj et</p><p> or equivalently using the relation that sinh tan </p><p> p</p><p> zj et</p><p> sinh </p><p> jet</p><p> p</p><p> tj et</p><p>Equating the numerators and denominators of Eqs and we obtain the</p><p> result</p><p> tow er s</p><p>X</p><p> p E</p><p> xj et xi</p><p> i</p><p> tow er s</p><p>X</p><p>E sin cos </p><p> i i i</p><p> i</p><p> tow er s</p><p>X</p><p>E cos </p><p>Ti i</p><p> i</p><p> and</p><p> tow er s</p><p>X</p><p> p E</p><p> yj et yi</p><p> i</p><p> tow er s</p><p>X</p><p>E sin sin </p><p> i i i</p><p> i</p><p> tow er s</p><p>X</p><p> E sin </p><p>Ti i</p><p> i</p><p>By comparing the numerators and denominators of Eqs and weget</p><p> Jets and Kinematics in Hadronic Col lisions</p><p> towers</p><p>X</p><p> p E</p><p> zj et zi</p><p> i</p><p> towers</p><p>X</p><p> E cos </p><p> i i</p><p> i</p><p> towers</p><p>X</p><p>E tanh </p><p> i i</p><p> i</p><p> towers</p><p>X</p><p> E sinh </p><p>Ti i</p><p> i</p><p> where wehave again used the relationship sinh tan andnotshown the details</p><p> of the algebra Wehave also used the fact that for the towers E E sin </p><p>Ti i i</p><p> rememb ering that in our approximation each calorimeter tower b e represented as a</p><p> particle of zero mass</p><p>It should b e recognized that the co ordinate was derived from Eq </p><p> jet</p><p> and the co ordinate from Eq using the relationship log tan </p><p> jet</p><p>Consequently the true do es not corresp ond to the energy weighted result </p><p> jet</p><p>P P</p><p>E E </p><p>Ti i Ti</p><p>The energy of the jet is given by an energy sum over all towers in the cluster</p><p> tow er s</p><p>X</p><p>E E </p><p> i jet</p><p> i</p><p>Wehave therefore established a selfconsistent prescription for turning a cluster</p><p> of energy towers into a physical jet which is a particle with momentum in the</p><p> detector frame given by</p><p>X X X X</p><p></p><p></p><p> p E p E E n </p><p> i i i i i</p><p> jet</p><p> and with directional co ordinates or and derived from the ab ove</p><p> jet jet jet</p><p> momentum comp onents or as calculated using Eq through </p><p>It is worth investigating expressions for the jet vector that involve not just</p><p> sums o ver towers at sp ecic angles and but rather sums that involve angles</p><p> i i</p><p> relative to the jet axis and </p><p> i jet i i jet i</p><p>The expression for p is straightforward Weusethenumerator of Eq </p><p>Tjet</p><p>X X</p><p> p cos E sin E</p><p>Tjet jet xi jet yi</p><p> i i</p><p> and substitute in E E cos and E E sin Thisgives</p><p> xi Ti i yi Ti i</p><p>X X</p><p> sin E cos sin E p cos </p><p> i Ti i jet Ti Tjet jet</p><p> i i</p><p>X</p><p>E cos </p><p>Ti i i</p><p>Jets and Kinematics in Hadronic Col lisions </p><p> </p><p>The expression for E is not as straightforward First we form E E p</p><p>Tjet</p><p> z</p><p>T</p><p> </p><p> and use the relation cosh x sinh x to get</p><p> </p><p>E E p</p><p>Tjet jet zj et</p><p> </p><p> E cosh sinh p cosh sinh </p><p> jet jet jet zj et jet jet</p><p> </p><p> E cosh p sinh E sinh p cosh </p><p> jet jet zj et jet jet jet zj et jet</p><p>If we add and subtract the quantityE p sinh cosh and then use Eqs</p><p> jet zj et jet jet</p><p> and in the ab ove equation weget</p><p> </p><p>E E cosh p sinh E sinh p cosh </p><p> jet jet zj et jet jet zj et jet</p><p>Tjet</p><p>X X X X</p><p> </p><p> E cosh E sinh E sinh E cosh </p><p> i jet zi jet i jet zi jet</p><p>X X</p><p></p><p> E cosh cosh E sinh sinh </p><p>Ti i jet Ti i jet</p><p>X X</p><p></p><p> E cosh sinh E sinh cosh </p><p>Ti i jet Ti i jet</p><p>X X</p><p> </p><p> E cosh E sinh </p><p>Ti i Ti i</p><p>This equation is not altogether transparent However consider the symmetry of</p><p> the sinh and cosh functions the former is o dd the latter is even If the jet is</p><p> symmetric in energy and physical extent ab out the jet axis then the sum over</p><p>E sinh will vanish leaving</p><p>Ti i</p><p>X</p><p>E E cosh </p><p>Tjet Ti i</p><p>Eqs and will prove useful later in our exp osition</p><p> Jet or Clustering Algorithm</p><p>The nal missing ingredient is an algorithm for determining which calorimeter cells</p><p> to include in a cluster that is consistent with Eq One suchscheme usually</p><p> </p><p> referred to as a xedcone algorithm used byUA CDF and D works</p><p> in the following way</p><p> All towers ab ove a mo derate energy threshold serve as seed towers for initial</p><p>protoclusters</p><p> All immediately neighb oring towers within some cone cuto R in space</p><p>a common range for the cone cuto R is relative to the center of</p><p> p</p><p> </p><p> are added to form a new cluster The the protocluster R </p><p> centroids or st moments of the cluster in and are recalculated These</p><p> towers mayormay note b e sub ject to a small energy threshold</p><p> If the jet centroid in changes by more than some small preset value then</p><p> all towers within the cone R are recombined to form a new cluster Again</p><p> the centroids are calculated in and This pro cedure is iterated until the</p><p> centroid of the cluster remains stable</p><p> After all clusters are found some maycontain overlapping same calorimeter</p><p> towers If so such clusters are merged dep ending on the fraction of transverse</p><p> energy present in the shared towers The smaller E cluster is then subsumed T</p><p> Jets and Kinematics in Hadronic Col lisions</p><p>A threshold parameter controls the merging Forthedatatobeshown in this</p><p> rep ort the merging parameter was set to of the energy shared by</p><p> anytwo clusters will cause merging</p><p>Another algorithm called the nearestneighb or algorithm was the primary clus</p><p></p><p> tering algorithm used by UA and is describ ed elsewhere</p><p> The Shape of a Jet</p><p>Equation can b e used to calculate the comp onent of the tower energy or</p><p> </p><p> momentum that is transverse to the jet direction k E E For those</p><p> xi yi</p><p>Ti</p><p> towers that are close to the jet axis the smallangle limit of Eq gives</p><p></p><p>E E </p><p>Ti i</p><p> xi</p><p></p><p>E sin E cos E</p><p> jet zi jet Ti</p><p> yi</p><p> sin E cos cos E sin </p><p> jet i i jet i i</p><p> E sin </p><p> i i</p><p> E </p><p> i i</p><p> E </p><p>Ti i</p><p> where wehave used sin from Eq and the relation E E sin </p><p>Ti i i</p><p>Squaring and adding the comp onents gives</p><p> </p><p> k E </p><p>Ti Ti i i</p><p> or equivalently</p><p> k E R </p><p>Ti Ti i</p><p> where R is the distance b etween the jet and cell i in space dened by</p><p> i</p><p> </p><p> R</p><p> i i i</p><p>Thus the momentum of each particle in the plane is given by the pro duct of</p><p> the E of the particle in the lab frame and the distance in space from the jet</p><p>T</p><p> axis Since the k are exp ected to b e symmetrically distributed ab out the jet axis</p><p>Ti</p><p> ve circular shap es in space Of course this Figure this suggests that jets ha</p><p> small angle limit is not a go o d approximation for particles cells that are far o</p><p> the jet axis</p><p>It is b est to dene the shap e of a jet using an energy weighting pro cedure This</p><p> reduces the dep endence of the shap e on low energy towers that are b oth far from</p><p> the jet axis and have a negligible contribution to the total jet energy The shap e</p><p> of a jet is often characterized byanE weighted second momentvariance of the</p><p>Ti</p><p> distance in the transverse plane Since the rst momentvanishes</p><p>X X</p><p></p><p></p><p> k E R </p><p>Ti Ti i</p><p> wehave</p><p>P P</p><p> </p><p>E E R</p><p>Ti Ti</p><p> i i i</p><p>P P</p><p> </p><p>R</p><p>E E</p><p>Ti Ti</p><p> which is equivalentto</p><p></p><p> </p><p> R</p><p>Jets and Kinematics in Hadronic Col lisions </p><p> when we dene and as</p><p> </p><p>P P</p><p> </p><p>E E </p><p>Ti Ti</p><p> i i</p><p>P P</p><p> </p><p> </p><p>E E</p><p>Ti Ti</p><p>Referring to data for some sp ecic R we rst dene</p><p> q</p><p> p</p><p></p><p> </p><p> R</p><p>R</p><p> using events from D describ ed in App endix Sample This data sample was</p><p> selected to minimize jet merging to a pro cess that has origin in higherorder</p><p>QCD eects that are distinct from those of jet fragmentation</p><p>Figure shows the distribution of the second moment for three jet cone</p><p>R</p><p> cutos of R and The p oints are D data The eect of the cone</p><p> cuto is clear the larger the cone the larger the nd moment in b oth mean and</p><p> width The main source of the broadening is simply due to the presence of additional</p><p> towers for the larger cone cutos Figure also shows the results of Gaussian ts</p><p> to the distributions The ts reveal that for unmerged jets the distribution of jet</p><p> widths is well describ ed by a Gaussian with a central value that is a function of</p><p> the cone cuto This is not to say that the energy ow around the jet axis has a</p><p>Gaussian distribution rather this is only describing the uctuations in the jet</p><p>R</p><p>RMS around the average which is itself a function of the jet cone parameter</p><p>R</p><p>Table shows the results for the ts and Figure shows that the central value of</p><p>Table Results of a Gaussian t to distributions of using the data from Sample </p><p>R</p><p>R RMS </p><p>R R</p><p> </p><p> </p><p> </p><p> the distribution in mean of the Gaussian scales linearly with the cone cuto </p><p>R</p><p>The small angle approximation used ab ove is clearly excellent Figure shows</p><p> that even for jets with R ab out of the time This shows that</p><p>R</p><p> the ab ove approximationisvalid for all but p erhaps of the R jets with</p><p> largest RMS widths</p><p> Jet Correlation Matrix</p><p>Detector eects gluon radiation and the underlying event all contribute to dis</p><p> torting the shap e of jets Figure shows a sketchofatypical elliptical real jet</p><p> with dened as the smaller of the angles b etween the semima jor axis and either</p><p> the or axis The angle can b e calculated from the variance in and as</p><p> dened in Eq and from the corresp onding correlation term dened as</p><p></p><p>P</p><p>E </p><p>Ti i i</p><p>P</p><p> </p><p></p><p>E</p><p>Ti</p><p>The shap e of the jet can b e characterized by the correlation term and the</p><p></p><p>diagonal terms and in the shap e matrix</p><p> </p><p> </p><p> </p><p> </p><p> </p><p> </p><p></p><p> Up on diagonalization the two eigenvalues corresp onding to the semima jor </p><p></p><p> and semiminor axes are </p><p> Jets and Kinematics in Hadronic Col lisions</p><p>Fig Jet probability distribution in for single unmerged jets</p><p>R</p><p>Fig Results of a Gaussian t to distributions in as a function of the cone cuto RThe</p><p>R</p><p> straight line is from a linear t to the p oints yielding R R</p><p>Jets and Kinematics in Hadronic Col lisions </p><p>η</p><p>α φ</p><p>Fig Jet ellipse Semima jor and minor axes represent the square ro ot of the second moment</p><p> in and </p><p> </p><p> Jets and Kinematics in Hadronic Col lisions</p><p> s</p><p> </p><p></p><p> </p><p> </p><p></p><p></p><p> </p><p></p><p></p><p> </p><p> </p><p>It is clear that for a circular jet and </p><p> </p><p></p><p>Wenow return to Eq which dened the quantity the RM S width of</p><p>R</p><p> the jet in space This quantity is of course the square ro ot of the sum of the two</p><p> diagonal terms of the shap e matrix and not the ro ot of the sum of the squares of</p><p> these two terms The odiagonal term do es not aect </p><p> R</p><p> The E of a Jet</p><p>T</p><p>A common way for exp erimenters to characterize the hard scattering energy scale</p><p></p><p>Q for QCD collisions which pro duce jets is to use the transverse energy E of</p><p>T</p><p> a pro duced jet The measure of E which is most often used to compare data to</p><p>T</p><p>QCD theory is</p><p> tow er s</p><p>X</p><p>E E </p><p>T Ti</p><p> i</p><p>It has the advantage that one can hop e to establish a corresp ondence b etween the</p><p> energy observed in eachtower exp erimen t and the particles radiated by a jet a</p><p> hadronized parton There are however two other ways to dene E one of which</p><p>T</p><p> is more amenable for treating a jet as a collection of physical ob jects particles</p><p> and p ossibly more appropriate for calculating invariant masses involving jets The</p><p>rst is</p><p>E E sin </p><p>T jet jet</p><p> where sin is related to through Eq and E is calculated using Eq</p><p> jet jet jet</p><p> The second way to dene E uses Eqs and As long as there is</p><p>T</p><p> consistency in comparing theory to exp eriment it is relatively arbitrary howone</p><p> denes E given that all internal variables are calculated consistently However</p><p>T</p><p> b ecause of the dierences b etween p and E the denition in Eq should not</p><p>T T</p><p> b e used in calculating the invariantmassgiven in Eq For such cases only</p><p> the E dened in Eq is appropriate</p><p>T</p><p> </p><p>To see this clearlywe use the relation E p m and write</p><p> </p><p>E sin p m sin p m sin </p><p>T</p><p>We see that this denition gives a systematical ly lower value for the transverse</p><p> energy E than the relativistically correct denition from Eq The dierence</p><p>T</p><p> of course is insignicant in the high energy limit jet velo city and for jets</p><p></p><p> that are pro duced at to the b eam axis socalled central jets</p><p>Wecanquantify the dierence in the two denitions of E through the quantity</p><p>T</p><p> q</p><p></p><p></p><p></p><p> p m sin </p><p>T E sin </p><p> p</p><p> </p><p></p><p></p><p>E</p><p>T p m</p><p>T</p><p> which measures the fractional error in using Eq Expanding Eq for</p><p> </p><p> small mass and keeping only the lowest p owers of m p gives</p><p>T</p><p></p><p></p><p> m tanh </p><p> </p><p></p><p>p T</p><p>Jets and Kinematics in Hadronic Col lisions </p><p>This shows the explicit dep endence of the dierence on p for arbitrary values</p><p>T</p><p></p><p></p><p> of For small tanh and rapidly approac hes zero Coupled with the</p><p> fact that mE for all but the smallestE jets we conclude that typicallyEq</p><p>T T</p><p> and Eq agree at the few p ercentlevel for </p><p>Figure shows the distribution in for the highest E jet in jet events from</p><p>T</p><p> our Sample App endix Figure shows the integrated probability as a function</p><p> of a lower cuto on the p ercen tage of jets that would b e mismeasured if w ere</p><p> greater than the value given on the abscissa The distributions clearly broaden with</p><p></p><p> jet cone size Because is prop ortional to m the broadening can b e attributed</p><p> to the broadening of the mass of a jet due to the increase in the numberofjet</p><p> towers with the cone size including towers that might not b elong in the jet</p><p>Such broadening can also come ab out from the failure to merge twojetsinto one</p><p> where one of the two jets mighthave an energy b elowanE threshold Sucha</p><p>T</p><p> threshold is usually employed by the exp eriments to eliminate the numb er of jets</p><p> found at very low energy</p><p>Fig Distribution in as dened using Eq for jets of Sample required to have j j</p><p>The E dened in Eq also underestimates the true E of the jet as dened</p><p>T T</p><p> using Eq This can b e seen as follows Supp ose there is a cluster with just </p><p> towers then Eq would yield</p><p> </p><p> E E p p E p</p><p> z z </p><p> z</p><p> </p><p> E E E cos E cos </p><p> </p><p> </p><p> E E E E cos cos </p><p> </p><p>T T </p><p></p><p> while equation would yield</p><p> Jets and Kinematics in Hadronic Col lisions</p><p>R R</p><p> </p><p> </p><p> dP where P is the distribution in Figure Jets were dP Fig I </p><p></p><p> </p><p> required to have j j </p><p>X</p><p> </p><p> E E E </p><p>Ti t t</p><p> i</p><p></p><p> E sin E sin </p><p> </p><p> </p><p>E E sin sin E E</p><p> </p><p>T T </p><p></p><p>If we form the dierence of the two expressions weget</p><p>X</p><p> </p><p>E p E E E sin </p><p>Ti </p><p> z</p><p> i</p><p> where We see that this dierence is always positive which means that</p><p> </p><p> using Eq underestimates the true E of a jet</p><p>T</p><p>Again we form the quantity</p><p>P</p><p>E</p><p>Ti</p><p> i</p><p> </p><p>E</p><p>T</p><p> whichshows the fractional error in using Eq for the transverse energyas</p><p> opp osed to Eqs and for the true E Figure shows the distribution</p><p>T</p><p> in as so dened As can b e seen in the gure the t wo dierent denitions of</p><p> transverse energy give similar results Dierences are not large and in fact Eq</p><p> gives a smaller error than one obtains when using Eq </p><p> The Mass of a Jet</p><p>Jets and Kinematics in Hadronic Col lisions </p><p>Fig Same as Figure E dened using Eq </p><p>T</p><p>The mass of a jet can b e calculated from its transverse momentum and energy using</p><p>Eqs and </p><p> </p><p> p E M</p><p> jet jet jet</p><p> </p><p> E p</p><p>Tjet Tjet</p><p> E p E p </p><p>Tjet Tjet Tjet Tjet</p><p> </p><p>Note that in the ab ove equation we formed the mass by using either E p or</p><p> </p><p>E p One should not confuse the mass of the jet as dened by E p with</p><p>T T T T</p><p> what wehave previously describ ed as the transverse mass In fact the transverse</p><p> mass is only dened when dealing with or more vectors A jet do es not have</p><p> a transverse mass</p><p>In the limit when the jet energy gets large the jet narrows and</p><p> i</p><p> We expand Eq for small and Eq for small yielding</p><p> i i i</p><p></p><p>X</p><p></p><p> i</p><p> E p</p><p>Ti Tjet</p><p></p><p> and</p><p></p><p>X</p><p></p><p> i</p><p>E E </p><p>Tjet Ti</p><p></p><p>Calculating the dierence and sum b etween E and p wehave</p><p>Tjet Tjet</p><p>X</p><p></p><p> </p><p> E p E </p><p>Tjet Tjet Ti</p><p> i i </p><p> Jets and Kinematics in Hadronic Col lisions</p><p>X</p><p></p><p> </p><p>E p E </p><p>Tjet Tjet Ti</p><p> i i</p><p></p><p>X</p><p> E </p><p>Ti</p><p> where wehave ignored the terms in and in the second equation Inserting</p><p> i i</p><p> these relations into Eq gives</p><p>X X</p><p> </p><p>M E E </p><p>Ti Ti</p><p> jet i i</p><p>Nowwe pro ceed to the small angle thin jet limit for largeE jets As in the</p><p>T</p><p>P</p><p> sections ab ove we can use the approximation E E and combine with</p><p>Tjet Ti</p><p>Eq to obtain the relation for the invariant mass of the jet as</p><p>M E </p><p> jet R Tjet</p><p>This equation conrms what we knowintuitively ab out the invariant mass of a</p><p> multiparticle <a href="/tags/System/" rel="tag">system</a> namely that the mass of the system is generated by the</p><p> angles b etween the approximately zero mass particles</p><p> ws the normalized distribution in mass M for jets that were Figure sho</p><p> jet</p><p> reconstructed with cone cutos of and The distributions broaden as</p><p> the cuto increases due to inclusion of more towers further away from the jet center</p><p>Fig Mass distribution for jets of dierent cone size</p><p>In Figure we plot the ratio E M onaneventbyevent basis These</p><p>R Tjet jet</p><p> distributions show that the ratio is well within the few p ercent level of unity for all</p><p> jet cones note the vertical log scale used</p><p> Jet Merging</p><p>Jets and Kinematics in Hadronic Col lisions </p><p>Fig The distribution in the ratio E M for dierent cone sizes</p><p> jet</p><p>R Tjet</p><p>The merging of two jets is usually reected in the value of and of course in</p><p>R</p><p> the size of the elements of the shap e matrix To study merging wehave used data</p><p> from D paying particular attention to whether there is evidence of any merging or</p><p> splitting of jets as controlled by the jet algorithm parameters see section These</p><p> data constitute our samples as describ ed in the app endices</p><p>Figure shows the normalized distributions in for merged and not merged</p><p>R</p><p> jets using our Sample for R and cone sizes We see a marked in</p><p> crease in the width of the merged jets for all cone cutos This sample is somewhat</p><p> biased by the requirement that after merging there must b e and only jets for</p><p> all three dening cone sizes</p><p>Figure shows the normalized distributions in using jets with cone cutos</p><p>R</p><p> of and for events from Sample App endix B This sample was chosen</p><p> to maximize the probability of collecting merged jets unlike Sample whichwas</p><p> chosen to maximize the probability of collecting unmerged jets The crosses and</p><p> the dots are resp ectively sp ectra for the merged and unmerged jets resp ectively</p><p>R</p><p> of Figure It should b e understo o d that each jet with R in Sample</p><p> is required to b e reduced to jets of R Figureshows that</p><p>R</p><p> correlates well on average with whether or not a jet is the result of a merging</p><p>We can therefore use the distributions from Figure to construct a likeliho o d for</p><p> a jet b eing from a merged or unmerged sample Figure shows the ratio of the</p><p> probability distributions for nonmerged and merged jets versus for cones of </p><p>R</p><p> and The p oints indicate the values of for relativelikeliho o ds of equal</p><p>R</p><p> probability of b eing from either distribution these are listed in Table </p><p>Finallyweinvestigate the shap e of jets via correlations in with resp ect to</p><p> </p><p> merging If jets were circular in space wewould exp ect that the quantity </p><p> p p</p><p> would b e Gaussiandistributed around If jets result from merging</p><p> </p><p> then we exp ect the shap e of the jet in space to b ecome elongated forming an</p><p> ellipse and the quantity would deviate from We use the normalized quantity</p><p> Jets and Kinematics in Hadronic Col lisions</p><p>Fig Normalized distributions in for jets that were merged b ottom and those that have</p><p>R</p><p> not b een merged top for dierent cone sizes</p><p>Fig Normalized distributionsof for single jets that are asso ciated with jets found by</p><p>R</p><p> way of a smaller cone cuto see text</p><p>Jets and Kinematics in Hadronic Col lisions </p><p>Fig Relative likeliho o d for a jet b eing nonmerged to a jet b eing merged as a function of </p><p>R</p><p> for three jet cones Relativelikeliho o ds of are indicated by the p oints on the curves</p><p>Table Value for corresp onding to a a relative likeliho o d of unity for jets to b e from non</p><p>R</p><p> merged or merged distributions</p><p>R </p><p>R</p><p> </p><p> </p><p> </p><p> Jets and Kinematics in Hadronic Col lisions</p><p> </p><p> </p><p> </p><p></p><p> </p><p> </p><p> which to rst order should b e indep endent of the cone size for symmetric jets</p><p>This is indeed observed in Figure where weshow for jets from Sample </p><p></p><p> with cones and Figure shows the same distribution from Sample </p><p> </p><p></p><p></p><p>Fig The distribution in using unmerged jets with cone cutos of and</p><p></p><p> </p><p></p><p></p><p> from Sample </p><p>As demonstrated ab ove these jets are broader than pure unmerged jets however</p><p>Figure also shows that the broadening of can b e asso ciated with a broadening</p><p>R</p><p> in either or </p><p> </p><p> Summary</p><p>The ab ove sections are intended to give a p edagogic description of jets towards an</p><p> understanding which is self consistent and illuminating For the particle physicist</p><p> the next step is to learn more ab out the physics of jets ie characteristics of jet</p><p> pro duction which in turn will allow understanding of the fundamental pro cesses</p><p> underlying the physics of interest</p><p>App endix A Events Used in Sample </p><p>A sample of events was used with the following requirements</p><p>i Pathologies Main Ring splash cosmic rays etcwere eliminated</p><p>ii The p osition of the collision vertex was required b e within cm of the</p><p> longitudinal center of the D detector</p><p>iii Eacheventhadtohave and only reconstructed jets for cones of </p><p> and with none of the jets formed from merging of twoormorejetsoflower</p><p>Jets and Kinematics in Hadronic Col lisions </p><p> </p><p></p><p></p><p> using merged jets with cone cutos of and Fig The distribution in </p><p></p><p> </p><p></p><p></p><p> from Sample </p><p> transverse energy by merging we mean that there was no explicit merging</p><p> by the jet cone algorithm as describ ed ab ove</p><p>iv All electron and <a href="/tags/Photon/" rel="tag">photon</a> candidates are rejected by requiring a minimum</p><p> for cluster and dep ending on the cone size The cutos used were</p><p> </p><p> </p><p> and for cones of and resp ectively</p><p>These requirements were chosen to maximize the probability of selecting events with</p><p> only jets at tree level Nevertheless we cannot exclude the presence of events with</p><p> or more jets where jets were merged two at a time a priori due to their extreme</p><p> closeness in space Suchcontamination should b e small In addition there are</p><p>probably small biases due to eg trigger thresholds since the D jet trigger</p><p> starts with a single trigger tower threshold thinner jets are more likely than fat</p><p> jets to pass the trigger requirement and primary vertex cuts item ii ab ove is not a</p><p> very restrictive cut However the results presented here are intended to b e purely</p><p> qualitative in nature</p><p>App endix B Events selected for Sample </p><p>These events were chosen to have a sample of merged jets Events were required to</p><p> satisfy the same criteria and used to dene Sample but only events that had</p><p> jets reconstructed with a cone size of and jets with a cone size of or</p><p> were analyzed guaranteeing the presence of twowell separated clusters of energy</p><p> within a jet Ab out of all events were classied in this manner</p><p> V Barger and R Phillips Col lider Physics AddisonWesley Reading MA </p><p> D Perkins Introduction to High Energy Physics rd Edition AddisonWesley Reading MA pp </p><p> Jets and Kinematics in Hadronic Col lisions</p><p> H Bggild and T Ferb el Inclusive Reactions Annual Review of Nuclear and</p><p>Particle Science </p><p> D Collab oration S Abachi et al NIM A </p><p> As of this submission the most precise published value of the W mass is </p><p></p><p>GeV c from a combination of D CDF and UA data By adding the</p><p></p><p> most recent LEP data the W mass changes to GeV c These re</p><p> sults were presented byDWo o d at the June Hadron Collider Physics con</p><p> ference at Stony Bro ok Pro ceedings for this conference will b e available online at</p><p> httpsbhepphysicssunysbedu hadronspro ceedin gshtml</p><p> D Gross and F Wilczek Phys Rev Lett </p><p> H Politzer Phys Rev Lett </p><p> J Huth and M Mangano QCD Tests in ProtonAntiproton Collisions Ann Rev</p><p>Nucl Part Sci </p><p> S Bethke in Proceedings of the XXIII International Conference on High Energy</p><p>Physics Berkeley ed S Loken World Scientic Volume I I pp </p><p></p><p> G Hanson in Proceedings XIII Rencontre de Moriond ed J Tran Thanh</p><p>Van Vol I I p </p><p> PLUTO Collab oration Ch Berger et al Phys Lett B </p><p> G Thompson in Proceedings of the XXIII International Conference on High En</p><p> ergy Physics Berkeley ed S Loken World Scientic Vol I I p </p><p> Herb ert Goldstein <a href="/tags/Classical_mechanics/" rel="tag">CLASSICAL MECHANICS</a> nd Edition AddisonWesley</p><p> pp The Euler transformation used here is given by equation with</p><p> the condition and </p><p> UA Collab oration Arnison G et al Phys Lett B B </p><p> and B </p><p> CDF Collab oration F Ab e et al Phys Rev Lett </p><p> and p erhaps most imp ortantly Phys Rev D </p><p> D Collab oration S Abachi et al Phys Rev D </p><p> UA Collab oration M Banner et al Phys Lett B </p>
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