1.1. Phase Space Volume

1.1. Phase Space Volume

<p>International Journal of Mo dern <a href="/tags/Physics/" rel="tag">Physics</a> A�</p><p> f</p><p> cWorld Scienti�c 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 colliding�b 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 � �K�e���and</p><p>� s forming clusters of energy dep osition in calorimeters� In this pap er we outline howto</p><p> de�ne 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 center�of�mass 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 di�erent energy results in a center�of�</p><p> momentum that do es not necessarily coincide with the lab oratory frame� A lackof</p><p> knowledge of the center�of�mass energy guides the choice of kinematic variables�</p><p>���� Phase SpaceVolume</p><p>We start with the de�nition 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>De�ning 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 �z�invariance 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 re�ect the Lorentz</p><p> invariance of the phase space elementis�p �y���m�� 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� de�ned 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 � � p�E � and � is� as ab ove� the p olar pro duction angle relativetothe�z</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 e�ect 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 di�erentiate 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 simpli�es 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 rapidity�y � should b e distributed uniformly in y � This is the origin of the</p><p></p><p>�rapidity plateau� for single�particle 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 sub�sections� 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 de�ne 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 �z�we 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 de�ned 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 de�ned 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 de�ned 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 m�variables� 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>���� Pseudo�Rapidity</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 rapidity�However� 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 rapidity�We therefore de�ne 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 pseudo�rapidity � � de�ned 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 tanh�x� is monotonic� the pseudo�rapidity</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> di�erence 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� j�jy j ����� corresp onding to the size of the calorimeter</p><p></p><p> readout pad at D� � Rapidity and pseudo�rapidity are equal to within ��� for pion</p><p> p of � ��� GeV�c� and proton p of � ��� GeV�c� 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 � � p�E � 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� j�jy j�wewould 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 e�ect</p><p> would b e esp ecially large for particles with low p and signi�cant 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� ����� di�erentiating 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 ��� � GeV�c 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 ���� GeV�c�</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>GeV�c� 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>Non�interacting particles such as neutrinos can b e detected only via an apparent</p><p> imbalance of momentum in an event� In p p �or pp�interactions� 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 su�ciently 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 non�interacting 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 insigni�cant� 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 lepton�neutrino 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 �� de�ned 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 de�nition� the transverse mass is de�ned 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 zero�mass 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 �forward�backward� in the lab</p><p> frame� Distributions in M will therefore have a tail at low M �forward�backward��</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 de�ned using Eq�</p><p>T</p><p> as E sin � � They are equivalent only in the limit m�p � �� 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 di�erence b etween E and p b ecomes insigni�cant�</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� b�or c sp eci�cally 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 right�hand side of Eq� ����� Because �� is the di�erence 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>���� De�nition of a Jet</p><p>There are various ways to de�ne jets� For instance� most of the LEP�PEP�and</p><p>�</p><p>PETRA e e exp eriments de�ne jets using information just from tracking cham�</p><p> bers � One of the less ambiguous ways to de�ne 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 parentparton�q � 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� ��� MeV�c at SPEAR s � ��GeV �� increasing</p><p>T</p><p>�</p><p> to hk i��GeV �c at SppS energies� We de�ne � 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 de�ned 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 de�ne 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 de�ned 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 de�nes 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� de�ned 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> di�erence 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 de�ning 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 havea��vector �E � p �that</p><p> jet jet</p><p> corresp onds to an ob ject of some �nite mass� We can de�ne the angles of our jet in</p><p> the lab oratory�asfollows�</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 self�consistent 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 eci�c 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 quantity�E 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 ��xed�cone� 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>�proto�clusters��</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 proto�cluster �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 re�combined 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 �nearest�neighb 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 small�angle 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 de�ned 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 de�ne 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 moment�variance� 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 de�ne � 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 eci�c R we �rst de�ne</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 higher�order</p><p>QCD e�ects 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> cuto�s of R ����� ���� and ���� The p oints are D� data� The e�ect 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 cuto�s� 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 e�ects� 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 � de�ned as the smaller of the angles b etween the semi�ma jor axis and either</p><p> the � or � axis� The angle � can b e calculated from the variance in � and ��as</p><p> de�ned in Eq� ��� and from the corresp onding correlation term � � de�ned 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 semi�ma jor ��</p><p></p><p> and semi�minor �� � 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� R�The</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� Semi�ma 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 de�ned 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 o��diagonal term � do es not a�ect � �</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 de�ne 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 de�ne 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> de�nes E �given that all internal variables are calculated consistently�� However�</p><p>T</p><p> b ecause of the di�erences b etween p and E � the de�nition 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 de�ned in Eq� ��� is appropriate�</p><p>T</p><p>  </p><p>To see this clearly�we 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 de�nition gives a systematical ly lower value for the transverse</p><p> energy E than the relativistically correct de�nition from Eq� ���� The di�erence�</p><p>T</p><p> of course� is insigni�cant 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 �so�called �central jets���</p><p>Wecanquantify the di�erence in the two de�nitions 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 di�erence ��� 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 m�E � for all but the smallest�E jets� we conclude that� typically�Eq�</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 de�ned using Eq� ���� for jets of Sample �� required to have j� j�����</p><p>The E de�ned in Eq� ���� also underestimates the true E of the jet �as de�ned</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 di�erence 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 di�erence 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 energy�as</p><p> opp osed to Eqs� ��� and ���� for the �true� E � Figure �� shows the distribution</p><p>T</p><p> in �as so de�ned� As can b e seen in the �gure� the t wo di�erent de�nitions of</p><p> transverse energy give similar results� Di�erences 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 de�ned 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 de�ned 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 de�ned 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 di�erence 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 large�E 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 con�rms 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 cuto�s 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 di�erent 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 di�erent cone sizes�</p><p> jet</p><p>R Tjet</p><p>The merging of two jets is usually re�ected 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 cuto�s� �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 de�ning cone sizes��</p><p>Figure �� shows the normalized distributions in � using jets with cone cuto�s</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 ����������Figure��shows 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 non�merged 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>Finally�weinvestigate 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 Gaussian�distributed 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 di�erent 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 non�merged 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 cuto�s 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� i�e� 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� etc��were 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 cuto�s 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 cuto�s 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 e�g� 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 de�ne 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 classi�ed in this manner�</p><p>�� V� Barger and R� Phillips� Col lider Physics �Addison�Wesley� Reading� MA� ������</p><p>�� D� Perkins� Introduction to High Energy Physics� �rd Edition �Addison�Wesley� Reading� MA� ������ pp� ��������</p><p>�� Jets and Kinematics in Hadronic Col lisions</p><p>�� H� B�ggild 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 byD�Wo 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> http���sbhep��physics�sunysb�edu � hadrons�pro ceedin gs�html�</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 Proton�Antiproton 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 Scienti�c� ������ 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 Scienti�c� ������ Vol I I� p� �����</p><p>��� Herb ert Goldstein� <a href="/tags/Classical_mechanics/" rel="tag">CLASSICAL MECHANICS</a> ��nd Edition�� �Addison�Wesley�</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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