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1983, Physics Letters B
We discuss the pair production of massive photinos +or other neutral gauginos in e e annihilation. We present +-cross sections for e e +--+ yy and e e -t yyy including finite mass effects for both the selectron and the gaugino. * Work supported by the Department of Energy, contract DE-AC03-76SF00515. § On leave of absence from Theory Division,
Physics Letters B, 1982
We evaluate cross sections for the two processes e÷e-~ .,/-photino-antiphotino, e÷e -~ .y-gravitino-antiphotino. In the local limit approximation they are proportional to a3s/m 4 (spin-0 electron) and GNewton ~2s/m2 (gravitino), respectively. If spin-0 electrons have masses between 16 and 40 GeV/c 2, the -r-photino-antiphotino production cross section would be of the order of 0.4 to 0.1 pb at x/-~ = 40 GeV, with the cuts indicated in the text. Detecting this process is within the range of possibilities at PETRA. If no such signal is found the existence of light photinos coupled to spin-0 electrons lighter than ~40 GeV/c 2 , or to gravitinos lighter than ~ 10 -6 eV/c 2, would be excluded.
Zeitschrift für Physik C Particles and Fields, 1989
Differential cross sections fore + e –$$e^ + e^ - \to \tilde \gamma \tilde \gamma $$ . No candidate events were found and a new limit on the photino mass is obtained.
Nuclear Physics B, 1986
We study in detail production and decay of neutralinos in e ÷ e annihilation. Formulae for the cross sectiom the single lepton, lepton pair, and missing energy spectra are given. Particular attention is paid to the mixing of gauginos and higgsinos. In order to illustrate its importance numerical results for four different mixing scenarios are presented.
Physics Letters B, 1996
A study of e'e-annihilations into final states containing a single energetic photon with no accompanying particles is made at a center of mass energy of 57.8 GeV. The measured cross section is consistent with expectations from standard model processes and is used to set limits on the masses of the scalar electron and photino particles predicted by supersymmetry theories. If the photino is assumed to be massless, the 90% confidence level lower limit on the mass of the degenerate scalar electron is 65.5 GeV. If the results of all the single photon experiments are combined, this lower limit increases to 79.3 GeV.
Nuclear Physics B, 1988
We treat in detail the production of selectrons and squarks in ep collisions, e + p ---, E + ~ + X. In particular we also study their most important decays. General mixing of gauginos and higgsinos is included. Formulae for the cross section, the energy and the angular distribution of the decay electron are given. We also calculate the cross section asymmetry when using polarized electron beams. Numerical results for three different mixing scenarios and various squark and selectron masses are presented. * Supported in part by "Fonds zur FBrderung der wissenschaftlichen Forschung in (3sterreich", project number P5444.
Physics Letters B, 1997
A search for pair-production of long-lived, heavy, singly-charged particles has been performed with data collected by the ALEPH detector at a centre-of-mass energy of 172 GeV. Data at p s = 161, 136, and 130 GeV are also included to improve the sensitivity to lower masses. No candidate is found in the data. A model-independent 95% condence level upper limit on the production cross section at 172 GeV of 0.2{0.4 pb is derived for masses between 45 and 86 GeV/c 2 . This cross section limit implies, assuming the MSSM, a l o w er limit of 67 (69) GeV/c 2 on the mass of right-(left-) handed long-lived scalar taus or scalar muons and of 86 GeV/c 2 on the mass of long-lived charginos.
European Physical Journal C, 1999
The events with two photons and missing (transverse) energy collected by the DELPHI detector at centre-of-mass energies between 130 GeV and 183 GeV have been studied to search for processes of the type e+e- → YY with the subsequent decay Y → X7, where X is an undetectable neutral particle. Reactions of this kind are expected in supersymmetric models, where the Y particle can be either the lightest neutralino, decaying to a photon and a gravitino, or the next-to-lightest neutralino, decaying to a photon and the lightest neutralino. To study the case of long-lived Y particles, a search for single-photon events with the reconstructed photon axis pointing far from the beam interaction region has also been performed. No evidence for a deviation from Standard Model expectations has been observed in the data and upper limits have been derived on the signal cross-section as a function of the the X and Y masses and of the Y mean decay path.
The European Physical Journal C, 2002
In the context of the Minimal Supersymmetric extension of the Standard Model, we analyze the production at future high-energy e + e − colliders of second and third generation scalar leptons as well as scalar quarks in association with neutralinos and charginos, e + e − → ff χ. In the case of third generation squarks, we also discuss the associated production with gluinos. We show that the cross sections for some of these three-body final state processes could be significant enough to allow for the detection of scalar fermions with masses above the kinematical two-body threshold, √ s = 2mf. We then discuss, taking as a reference example the case of scalar muons, the production cross sections in various approximations and make a comparison with the full four-body production process, e + e − → ff χχ, in particular around the two-sfermion threshold.
Physical Review D, 1996
In a class of low-energy supersymmetry models the photino is a natural dark matter candidate. We investigate the effects of post-freeze-out photino annihilations which can generate electromognetic cascades and lead to photo-destruction of 4 He and subsequent overproduction of D and 3 He.
Physics Letters B, 1982
…, 1976
We present the properties of 103 events of the form e+ + -t-e--+e-+p + missing energy, in which no other charged particles or photons are detected.
Nuclear Physics B, 1995
We study the production and decay of heavy selectrons in the e − γ mode of a linear collider of the next generation. The standard model backgrounds can be substantially reduced by appropriate kinematical cuts. As a consequence, selectrons far heavier than the kinematical threshold for pair production are shown to be easily discoverable for large portions of the supersymmetry parameter space. We also describe a model-independent kinematical measurement of the mass of the lightest neutralino.
The European Physical Journal C - Particles and Fields, 2002
We investigate selectron pair production and decay in e − e − scattering and e + e − annihilation with polarized beams taking into account neutralino mixing as well as ISR and beamstrahlung corrections. One of the main advantages of having both modes at disposal is their complementarity concerning the threshold behaviour of selectron pair production. In e − e − the cross sections at threshold forẽ RẽR andẽ LẽL rise proportional to the momentum of the selectron and in e + e − that forẽ RẽL. Measurements at threshold with polarized beams can be used to determine the selectron masses mẽ L/R precisely. Moreover we discuss how polarized electron and positron beams can be used to establish directly the weak quantum numbers of the selectrons. We also use selectron pair production to determine the gaugino mass parameter M 1. This is of particular interest for scenarios with non-universal gaugino masses at a high scale resulting in |M 1 | |M 2 | at the electroweak scale. Moreover, we consider also the case of a nonvanishing selectron mixing and demonstrate that it leads to a significant change in the phenomenology of selectrons.
Nuclear Physics B, 1978
We have observed events of the form e + + e---, e + + e-and e + + e-~ ~+ + #-in which there are no other detected particles and there is substantial missing energy; and which cannot be explained by conventional electromagnetic interactions. We show that these events can be explained as the decay products from the pair production, e + + e---* r + + r-, of a new charged lepton, r -+, of mass ~1800 MeV/c 2. Some properties of these events are presented. In particular, this production cross section is inconsistent with the r being an electron-related paralepton.
The European Physical Journal C, 1999
The events with two photons and missing (transverse) energy collected by the DELPHI detector at centre-of-mass energies between 130 GeV and 183 GeV have been studied to search for processes of the type e + e ! YY with the subsequent decay Y ! X , where X is an undetectable neutral particle. Reactions
Physical Review D, 2004
We study two CP sensitive triple-product asymmetries for neutralino production e + e − →χ 0 iχ 0 j and the subsequent leptonic two-body decayχ 0 i →l ℓ,l →χ 0 1 ℓ, for ℓ = e, µ, τ . We calculate the asymmetries, cross sections and branching ratios in the Minimal Supersymmetric Standard Model with complex parameters µ and M 1 . We present numerical results for the asymmetries to be expected at a linear electronpositron collider in the 500 GeV range. The asymmetries can go up to 25%. We estimate the event rates which are necessary to observe the asymmetries. Polarized electron and positron beams can significantly enhance the asymmetries and cross sections. In addition, we show how the two decay leptons can be distinguished by making use of their energy distributions. *
Physical Review Letters, 2005
Physics Letters B, 1976
We present the properties of 103 events of the form e+ + -t-e--+e-+p + missing energy, in which no other charged particles or photons are detected.
1998
For the process e+e-+ p+p-(n) , the cross section and forward-backward charge asymmetry are measured at the highest ever center of mass energies which ranged from 130 to 183GeV. The data originates from 85pb-1 of integrated luminosity collected with the L3 detector at LEP. The measured muon pair cross section and forward-backward asymmetry agree with the Standard Model prediction with a XMI /N = .61 with 10 degrees of freedom. A mass limit on an additional heavy, neutral gauge boson of Mz, > 315GeV is set using muon pair production alone, rising to Mz, > 805GeV when all final states are considered. A search for an excited lepton decaying via p*-+ fy excludes such objects with electromagnetic coupling up to 183GeV.
Physics Letters B, 1993
We have studied the production of charged D* mesons m e+e -annxhflaUon at an average center-of-mass energy of 58.0 GeV. Charged D* mesons were identified using two independent methods; the mass-difference method and the detection of the low transverse-momentum plon The forward-backward asymmetry of the charm quark producUon was measured to be Ac= -0 61 +_0.13(stat )+0 08(syst.). The cross section of reclusive D* production was found to be e(e+e---,D*+-+X)=24.5+ 5.3 (star) + 3.0 (syst.) pb. If we assume the standard model prediction for the charm quark production, we obtain the branching ratio for the charm quark to produce a charged D* meson to be Br(c-.D °÷ + X) = (22 + 5 (stat) + 3 (syst.) )%.
Physical Review D, 1989
European Physical Journal C, 1987
Mass limits are presented for various supersymmetric particles: scalar partners of electrons, muons, taus and quarks; photinos, winos and zinos. They were obtained from the analysis of an exposure of 48.6 pb−1 of the CELLO detector at the PETRAe + e − storage ring up to a center of mass energy of 46.8 GeV. Special attention has been given to the case where the photino is assumed to be the lightest supersymmetric particle, but other possibilities have also been considered.
Physics Letters B, 1988
Physical Review D, 1997
We explore two possible interpretations for the CDF eeγγ + E T / event in the context of a recently proposed one-parameter no-scale supergravity model with a light gravitino. We delineate the region in parameter space consistent with the kinematics of the event interpreted either as selectron pair-production (pp →ẽ +ẽ− X,ẽ =ẽ R ,ẽ L ) or as chargino pair-production (pp → χ + 1 χ − 1 X). In the context of this model, the selectron interpretation requiresẽ =ẽ R and predicts comparable rates for ℓ ± γγ + E T / , whereas the chargino interpretation predicts comparable rates for (ℓ ± ℓ ′ + ℓ ′ − , ℓ + ℓ − , ℓ + ℓ − jj) γγ + E T / . We also consider the constraints from LEP 1.5 and the expectations for LEP 2. We point out that one of the acoplanar photon pairs observed by the OPAL collaboration at LEP 1.5 may be attributable to supersymmetry in the present model via e + e − → χ 0 1 χ 0 1 → γγ + E T / . We also show how similar future events at LEP 2 may be used to deduce the neutralino mass.
Physical Review D, 2008
We study the production of the lightest neutralinos in the radiative process e + e − →χ 0 1χ 0 1 γ in low energy supersymmetric models for the International Linear Collider energies. This includes the minimal supersymmetric standard model as well as its extension with an additional chiral Higgs singlet superfield, the nonminimal supersymmetric standard model. We compare and contrast the dependence of the signal cross section on the parameters of the neutralino sector of the minimal and nonminimal supersymmetric standard model. We also consider the background to this process coming from the Standard Model process e + e − → ννγ, as well as from the radiative production of the scalar partners of the neutrinos (sneutrinos) e + e − →νν * γ, which can be a background to the radiative neutralino production when the sneutrinos decay invisibly. In low energy supersymmetric models radiative production of the lightest neutralinos may be the only channel to study supersymmetric partners of the Standard Model particles at the first stage of a linear collider, since heavier neutralinos, charginos and sleptons may be too heavy to be pair-produced at a e + e − machine with √ s = 500 GeV.
Physics Letters B, 1996
A study of e'e-annihilations into final states containing a single energetic photon with no accompanying particles is made at a center of mass energy of 57.8 GeV. The measured cross section is consistent with expectations from standard model processes and is used to set limits on the masses of the scalar electron and photino particles predicted by supersymmetry theories. If the photino is assumed to be massless, the 90% confidence level lower limit on the mass of the degenerate scalar electron is 65.5 GeV. If the results of all the single photon experiments are combined, this lower limit increases to 79.3 GeV.
Fortschritte der Physik/Progress of Physics, 1994
Rare kaon processes appear to be particularly suitable to study the extensions of the standard model, especially if the possibility for eventual direct evidence becomes unlikely. In this review, we discuss processes that are important as a test of either the standard model or supergravity. Moreover, some of these are important even for both the standard model and for supergravity. Particular attention is paid to the reduction of uncertainties in the calculation, especially the ones coming from the confinement effects. Recent approaches, such as chiral perturbation theory, the large N c -expansion, QCD sum rules and lattice QCD, are discussed. This is found to be the best strategy in view of the fact that supersymmetric effects are rather tiny.
Physical Review D, 2000
It has been shown that unless the tri-linear R-parity violating coupling λ i33 (i = 1, 2) is small enough (λ i33 < 10 −2 for MSSM and 10 −3 for GMSB model), the partial decay width of photino decaying into 'photon + ν e,µ ', both in supergravity motivated (MSSM) and gauge mediated (GMSB) supersymmetric models are larger than the partial decay width of photino decaying into 'photon + goldstino' in R-parity conserving GMSB model including one loop supersymmetric QED correction.
Modern Physics Letters A, 2011
We examine the single-photon processes in the frame work of supersymmetric models at future e + e − linear colliders. According to recent experimental achievement, optimistic polarization degrees for both electron and positron beams are taken into account to enhance the signal-to-noise ratio revealing the observable difference between supersymmetry breaking models. The minimal supergravity model and the minimal SU(5) grand unified model in gaugino mediation have been examined as examples. We see that after several years of accummulating data, the difference of the number of single-photon events between the two models received from the collider would be in excess of three times the statistical error, providing us the possibility to probe which model would be realized in nature. The result is well suitable for the future running of the International Linear Collider.
Physics Letters B, 1985
We argue that an observation of e+e ~-f + missing energy in the longitudinally polarized e+e-beam with the total helicity zero will be a signal for N = 2 supersymmetry. In a certain range of parameters, the above process can be interpreted as e~e r (or e~el)~ ~' + two unobserved paraphotini (with DiD t ~ 10-2 pb), along with the assumption about the conservation of mirror parity (M) and that the paraphotino is the lightest M-odd particle. The observation cannot be understood within the minimal SU(3)×SU(2)×U(I) theory whether it is N = 1 supersymmetric or not.
Modern Physics Letters A, 2008
We study signals for beyond standard model physics and consider the virtues of single photon signals or associated photons in the final states in identifying different scenarios of new physics models in a very efficient and novel way.
Nuclear Physics B, 1986
In this paper we study the antiproton, positron and gamma-ray fluxes resulting from the aniaihilation of supersymmetric dark matter in our galactic halo. We show that the requirement of closure imposed by inflationary cosmologies constrains the supersymmetric dark matter to be either a relatively pure photino eigenstate or a relatively pure higgsino eigenstate, or possibly a scalar neutrino with a mass less than 4 GeV. The photino choice can lead to observable p fluxes when sfermion masses are < 50 60 GeV. Such a scenario is testable via the radiative production of photinos at PEP and PETRA. The higgsino scenario leads to observable p fluxes independent of sfermion masses, provided (0[H~ I0)/(0SH~]0) = vl/v2-> 2. In contrast, sneutrino dark matter annihilates ahnost entirely into neutrinos, resulting in a monochromatic neutrino flux that is probably unobservable.
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