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Physics Focus and Fiscal Forces

Physics Focus and Fiscal Forces
Physics Focus and Fiscal Forces

a r X i v :h e p -t h /9111019v 1 8 N o v 1991HUTP-91/A057

Physics Focus and Fiscal Forces

Sheldon L.Glashow Lyman Laboratory of Physics Harvard University Cambridge,MA 02138Two items are reproduced herein:my ‘Outlook’talk,an amended version of which was presented at the 1991joint Lepton–Photon and EPS Conference in Geneva,and an Open Letter addressed to HEPAP.One is addressed primarily to the European high–energy physics community,the other to the American.A common theme of these presentations is a plea for the rational allocation of the limited funds society provides for high–energy physics research.If my ‘loose cannon’remarks may seem irresponsible to some of my colleagues,my silence would be more so.

11/91

1.OUTLOOK

Just a few months after CERN’s triumphant observations of Z0and W±bosons, Harvard celebrated the centenary of its Je?erson Physical Laboratory.Carlo Rubbia,then one of our most illustrious faculty members,described these discoveries and more:he spoke with gusto of certain curious events—monojets—which could not be explained with the standard model of particle physics.We have learned a great deal since then.There are no inexplicable monojets and there has not been one demonstrable failure of the standard model.QCD and the electroweak theory reign supreme.They o?er a complete,correct and consistent description of all known elementary–particle phenomena.Rubbia is now the director–general of a laboratory that seems forever destined to con?rm the predictions of what we must now call the standard theory.His punishment is?t as a modern–day myth.

Some physicists look upon the current situation as a triumph of human ingenuity, since many of the most puzzling problems of the past are solved.The rich and complex spectroscopy of hadrons is‘understood’at last in terms of the energy levels of a system of two or three interacting quarks,much as the spectroscopy of nuclei is understood in terms of constituent nucleons and that of atoms in terms of electrons.(The quotes are needed since we cannot as yet perform as precise calculations with QCD as we might wish to do.)Similarly,all of the wealth of weak–interaction phenomena is resolved in terms of the gauge interactions of three intermediate vector bosons,whose properties have been found to agree with the predictions of the electroweak theory.

Many questions lie beyond the ken of the standard theory.They remain to be answered and suggest the existence of a more powerful theory.Why are there three fermion families? Why do particles have the masses and mixings they do?Why did nature choose the gauge group SU(3)×SU(2)×U(1)?Look to history,say the optimists.The secrets of the outer atom were exposed at energies of a few eV.Those of the inner atom by X ray studies at energies of a few KeV.The nucleus was explored at MeV energies and evidence for quarks appeared at some GeV.Each great breakthrough required a leap in energy by a factor of 1000.Thus,the next great discovery to be made—the nature of electroweak symmetry breaking and the origin of mass—will be revealed in the multi–TeV domain:at the next great hadron collider.

Other physicists interpret the manifold empirical successes of the standard theory as a tragedy marking the end of an era of exciting discovery.Aside from one missing quark and

the Higgs boson,nothing is left to discover at the high–energy frontier.All that remains is the measurement of the next decimal place.Although we have heard this refrain before, the pessimists also consult the history of our discipline.They point to the great surprising discoveries of the past century,which until recently have sprung upon us every few years: 1890s X rays,rare gases,radioactivity and the electron.

1900s Planck’s h,half–lives,photoelectric e?ect,special relativity.

1910s Cosmic rays,nuclei,the Bohr atom and the bending of starlight.

1920s Hubble shift,quantum theory,spin and the Pauli principle.

1930s Positrons,muons,neutrons,?ssion,continuous beta spectra.

1940s Pions,strange particles,the Lamb shift and the atomic bomb.

1950s Parity violation,pion–nucleon resonance,neutrinos,V?A.

1960s Muon neutrinos,scaling behavior,CP violation,hadrons aplenty.

1970s J/Ψ,neutral currents,tau leptons,charm and beauty quarks.

1980s SN1987a,voids and walls of the universe.

While new and wonderful things are being found out about the universe,there hasn’t been a big surprise in our discipline since the establishment of the third family of quarks and leptons in1977.True,W and Z were?rst produced and detected in the1980s,but their reality came as no surprise.Not for well over a century has there been such an insipid interregnum.So be it.While optimists glory in the success of the standard theory and pessimists bemoan their fate,there remains much to be done:

?Let us not be hasty in assuming its absolute validity:the standard theory must be tested as best we can.With a million Z0events in hand,the theory works just?ne.Will agreement persist when we have ten times that number?Will the deduced value of the muon’s g?2survive the next experimental onslaught?Is the Kobayashi–Maskawa matrix truly unitary?And so on.

?We must learn to exploit the standard model better.Theorists and experimenters must work together to devise more and better ways to extract the consequences of a recalcitrant theory and confront them with experiment.

?We must hope for more surprises and search for them.Nature is not the enemy; complacency is.No physicist should be so arrogant as to believe that her bag of tricks is exhausted,lest the great desert of particle physics become a self–ful?lling prophecy.

?We must worry the weak points of the standard theory.CP violation is surely among them.Another generation of experiments is needed to pin down the fundamental

CP–violation parameters in K0decay.The search for a neutron electric dipole moment must go on.Most importantly,the world needs one(and only one!)B factory powerful enough to explore the question of CP violation in B decay.

?We must extend the burgeoning non–accelerator frontier and not forget that much of what we know about elementary particles once came,and will come again,from disciplines far removed from accelerator–based high–energy physics:

(a)The existence of an alleged17KeV neutrino is?atly inconsistent with the standard

theory.Does it exist or does it not?Discussions at this meeting were inconclusive.

Many experiments,some of them solid,see evidence for it.Many experiments,some of them solid,claim to exclude it.Here is an exciting dilemma!

(b)Does resolution of the solar–neutrino problem demand the existence of mixed and

massive neutrinos?These e?ects lie beyond the minimal17–parameter standard the-ory.However,the case for MSW oscillations as a cure to the problem is far from iron clad.Morrison,for example,is led to conclude that there is no solar neutrino problem.Decisive results from the gallium experiments are awaited with fervor,as are those from future experiments now being planned.

(c)Astronomers have come to the dreadful conclusion that they cannot detect anything

beyond the gravitational in?uences of the dominant form of matter in the universe.

The dark matter may be non–baryonic and unconventional.If so,its identi?cation and investigation lies within the realm of high–energy physics.

The near–term future of elementary–particle physics,largely if not exclusively,de-pends on those large accelerators that are now or soon operating:the?xed target facilities at Fermilab,Brookhaven’s kaon beam,the Tevatron collider,LEP,HERA and the mini B factory at Cornell.I have not the gall to write a guide for the experimenter.Our discipline is open–ended,in the sense that the new and pro?table directions are almost certainly not those that we anticipate.Surprises may lie in wait for experimenters at all of these facilities.

For the long term,our community is almost unanimous in its belief that the next great accelerator must be a hadron collider.SSC is approved and partially funded while an LHC proposal is soon to be put to the CERN council.At the risk of alienating many friends and colleagues,let me consider this issue.?

Giant accelerators,their enormous detectors,and their continuing operations are enor-mously expensive enterprises.We all agree that the world needs one great hadron collider, but two such machines makes no sense at all.The world’s governments,if they knew what we know,should not fund the construction and instrumentation of both machines.There are too many other interesting and important things to do!Although well–intentioned ar-guments have been presented for each accelerator from each side of the Atlantic,the course that is set seems bound for disaster.

Should we prove ingenious(and irresponsible)enough to convince our governments to begin building the two comparable behemoths,these endeavors are likely to starve ongoing research programs in all of physics,and especially in high–energy physics.Money is more–or–less conserved:CERN needs extra support(from member or non–member)nations to build LHC expeditiously,and SSC may not be built without substantial external support. The majority of our colleagues—those who do physics in real time and choose not to live at the very fringe of the high–energy frontier—will need and deserve funds that are almost certainly to be pre¨e mpted by our preoccupation with bigness.

If and when the twin supercolliders begin to do real physics research—which may not happen until the next millenium—there may no longer exist enough of a community of experienced and dedicated high–energy physicists to use them.It is not for reasons of national pride that I believe that SSC is the preferred machine if we have the vision,the scienti?c integrity,and especially,the?scal responsibility to build only one.

?There are technical obstacles in the path of the construction and exploitation of LHC. It requires novel two–in–one magnets operating at nearly ten tesla.Can reliable and ade-quate magnets can be industrially produced at reasonable cost?The physics reach of the LHC is extended by exchanging a compromised collision energy for an intense luminosity, but can appropriate detectors be designed and built to make use of such luminosities?

?There are operational di?culties associated with the construction of LHC.LEP has made a glorious start in its ambitious and exciting program.It has both a higher–luminosity and a higher–energy phase to look forward to.It would be tragic for physics if LHC deployment would hamper,delay or constrain these essential projects.

?There is a serious scienti?c risk associated with the exploitation of LHC.Its collision energy is severely constrained by its need to?t within the LEP tunnel.What if the new physics is accessible at40TeV but not at20TeV?

My dream is of a‘new world order’of cooperation rather than competition for which high–energy physics can lead the way.Let SSC evolve into a truly international project: in funding,instrumentation and administration.CERN is an enormously successful and enviable model.Let SSC?y the?ags of all interested and committed nations and be administered by a representative council much as CERN is.Let it be a machine in America but of the world.My dream is certainly naive,unrealistic and all but impossible to realize. Until recently,the DOE has insisted that SSC be an essentially American enterprise.CERN needs a new initiative to ensure its continued vitality.Nonetheless,I cherish the hope—for the sake of our discipline—that my dream may come true.

Much has been said at this conference about grand uni?cation.Strong,weak and electromagnetic forces are each mediated by gauge bosons.The hypothesis that there is a simple underlying gauge group is irresistably attractive.In minimal SU(5),the curi-ous charges of quarks and leptons are forced upon us and each family corresponds to an anomaly–free representation.Neutrinos are automatically massless and neutral.The ob-served disparity in strength between strong and electric forces sets the symmetry–breaking scale,makes protons practically stable,and evaluates the weak mixing angle.The trouble is in the details:protons are not stable enough and sin2θcomes out a bit too small.

There are many ways in which minimal SU(5)may be modi?ed so as to patch up the problems,?t the data,and save the notion of grand uni?cation.The First Fix:A decade ago,several theorists pointed out that supersymmetrized SU(5)could do the trick[1]. The Second Fix:Both empirical problems could be dealt with by adding to the standard theory one or more split SU(5)fermion multiplets[2].The Third Fix:Perhaps there is an intermediate stage of symmetry breaking involving a semisimple gauge group lying between the unifying group and the group of the standard theory.An intersesting example of such a hierarchy is:

O(10)→SU(3)×SU(2)×SU(2)→SU(3)×SU(2)×U(1).

The intermediate mass scale can be chosen to?t the low–energy values ofα,αs and cosθ[3].For this case,the uni?cation scale is comparable to the Planck energy(neat,but no observable proton decay),and left–right symmetry is restored at roughly a million TeV (useful to generate sensible neutrino masses,but not for new phenomena at LHC or SSC).

Now that LEP data has provided us with an accurate determination ofαs,many workers have refocussed on the rescue of grand uni?cation and the intriguing possibility

that lots of new particles lie almost within reach[4].The results of their analyses are remarkable(and have received lots of attention in the semi–popular press).

Although the failure of minimal SU(5)is now established beyond any possible doubt, its supersymmetrized version is still very much alive.Furthermore,the super–partners of known particles may lie~1TeV and be accessible to the next great hadron collider; and proton decay may be detectable at super–Kamioka.A careful and current analysis of the data[5]is dramatically summarized in?gure(1).?However,the second?x(which does not please supersymmetry fans,but involves many fewer hypothetical and perhaps accessible particles)is also in the running,as?gure(2)demonstrates.The?rst and second ?xes suggest—the input data are not precise enough as yet to use a stronger verb—the possible existence of new physics at soon–to–be accessible energies.However,the third ?x also preserves grand uni?cation with an intermediate mass scale lying well beyond experimental reach.And,there may be other?xes as well.We shall learn more about the various possibilities as data improve,and we cannot emphasize too strongly the importance of those‘pedestrian’experiments,at LEP or HERA,that serve to measure the value of the strong coupling constant.

In summary,let me quote a countryman,‘The game ain’t over’til it’s over.Particle physics is very much alive,both at and away from the highest energies,both at and away from accelerators.Our colleagues who lean toward astrophysics and cosmology have given us a solar neutrino headache and various costly medicines to cure it,gravitational lenses,an indirect con?rmation of gravitational radiation and a hoped–for(but unfunded) search for such waves,supernova neutrinos,a weird large–scale structure to the universe coupled with a perfectly smooth era of recombination,inexplicable burster phenomena, the possibility of unconventional dark matter,and many more surprises and dilemmas to come.Our low–energy colleagues give us monopole constraints,axion searches,an alleged 17KeV neutrino,an exorcism of the?fth force,a precision test of the electroweak theory, and again,more to come.

At the accelerator frontier,there are many important experiments to do and surprises to uncover.Indeed,there is far more to do than we can easily a?ord,especially with the burden of building and instrumenting supercolliders in two continents.The Fermilab collider must be upgraded so that it may do its best to?nd the top,which will be a

primary background to experiments at larger hadron colliders.Fixed–target experiments are needed to measure?′and to search for rare decays and neutrino oscillations.HERA may?nd leptoquarks,but it will certainly lead to precision tests of QCD.LEP,in its present and future avatars,may yield wonderfully inexplicable events,but it o?ers the best tests of the electroweak theory and the best constraints on its variations.A B factory is essential if we are to clarify our understanding of quark mixing and CP violation,while smaller factories which are dedicated to physics at1GeV and at3GeV have important r?o les to play as well.Finally,and in my view most importantly,we must learn how to build a powerful linear electron–positron collider with which to study the TeV domain in a relatively clean environment.

Many of our best theorists are all wrapped up in strings and conformal?eld theory. They believe that a new mathematical framework is needed that lies beyond tried and trusted quantum?eld theory.They are almost certainly right in their belief:the most puzzling‘why questions’cannot even be posed in the standard theory or any of its con-ventional modi?cations.However,their early optimism is gone:most string theorists no longer believe that a theory of everything lurks around the corner.They should not be discouraged.The new theory will come in its time,and today’s theorists may lead us to it kicking and screaming.In the meanwhile,particle physics remains,as it traditionally has been,primarily an exciting and rewarding experimental science.

2.AN OPEN LETTER TO HEPAP

Esteemed colleagues:Some years ago,I became a member of HEPAP.For all I know,I may yet be.I attended the?rst two meetings during my tenure,and no others. The reasons include time pressure and my own irresponsibility,but the primary cause for my delinquency is a strong impression that HEPAP(unlike the CERN Science Policy Committee,in which I served honorably for six years)does not adequately address the needs of the community.Due to the open nature of its meetings,a constituency that re?ects the con?icting self–interests of our several national laboratories,the obligation to follow a?rmly orchestrated agenda,the absence of prior discussions and the lack of executive sessions,di?cult issues are rarely faced and sad truths are withheld or sloughed over.I am led to write this letter—rather than play–act at HEPAP—because of my love for and concern about the discipline of accelerator–based high–energy experimental physics in the United States.

I apologize for this hurried and distraught communication,but I am alarmed by the precipitous decline of a discipline that Americans created and,until recently,dominated. There is not reason nor sense for continuing American domination of the?eld,but we should at least remain as major players.We spend a lot of money on HE physics,but seem to get too little physics done per dollar spent.If we are to argue,as I think we should,for more funding—or even for continuing funding at present levels—we must demonstrate more of a sense of?scal responsibility than we have in the past.At the price of alienating many colleagues and friends,let me say the unsayable:

?The SLD detector at SLAC has been a sink–hole for funds that could have been spent productively:it is a second detector for a machine that will probably never do useful physics.(CERN has analyzed a million,going on ten million,Z0events.SLC has got a few hundred,and won’t do all that better,polarization or no.Face it chums:it’s a brilliant demonstration of a new accelerator technology,but will never be much of a research tool.)Years ago,when the SLD project was initiated,its proponents may have had sound arguments for it.Very soon,however,it became clear to much of the community that the device was pointless.However,once the great bureaucratic ship sets its sails,no agent on Earth can correct its course.Physicists lucky enough to be on board cling blindly to to their challenging tasks no matter that the cruise is to nowhere.For all I know,money is being spent on this useless toy even as I write.

?When the Soudan proton decay detector was?rst proposed,it seemed a good idea. If the larger IMB and Kamioka could detect proton decay,a smaller but more highly instrumented device would have been an invaluable facility.As it turned out many years ago,there was no such signal.It became clear that the Soudan initiative was pointless,as far as its original primary goal is concerned.No matter.The ship plows on.

?Although PEP was in many ways a better instrument than PETRA,its timing was a disaster.Aside from a few physics gems,it came on line far too late to succeed as a forefront accelerator.As my father taught me,if a job’s worth doing,it’s worth doing right...and when it needs doing!

?Years ago,it seemed a good idea to provide the Fermilab collider with a better and bigger(and very expensive)new detector.But a second detector is useful only when there is the potential to exploit the accelerator at which it is to be used.However,we have hardly begun to exploit the CDF detector.With collider runs as far apart as they are, who needs another detector?It’s just one more uncontrollable spigot or useless ship.All

that money could have been used to shore up the decaying university–based infrastructure upon which all of physics research depends.

Enough spilt milk and rotten eggs!High–energy physics in America is threatened by dilution(too many sacred laboratories),by dispersion(too many directions,with little foresight and no corrective capacity)and by the reluctance of our community and its sponsors to perform di?cult but necessary triage.In the future,we must focus more tightly and painfully,or abandon ship.

For sound scienti?c and technical reasons,we all agree that a proton super–collider is our?rst priority.However,SSC will not come on line for physics for a decade.If things continue as they are,there aren’t going to be any American experimenters around who are ready,willing and able to use it.All other priorities are irrelevant and immaterial unless we properly attend to numero uno!

As I talk to my experimentalist friends,I?nd that almost all groups–from the brilliant to the merely sound—are being squeezed out of the business of high–energy physics.Hardly any American graduate students care to board our sinking ships.Yet,if we are to build SSC,we must keep HE physics,especially hadron–collider physics,healthy in the meantime—and there’s lots of good physics remaining to do at the World’s Highest Energy but Rarely Running Accelerator.The training ground for a large hadron collider is a large hadron collider,and we’ve got the only one.We’ve got to‘?nd the top’because it’s likely to be the background to really interesting SSC events.Can anyone doubt that part and parcel of the SSC initiative must be the maximum exploitation of the Fermilab collider.This means that we must have more collider runs sooner and a Main Injector too!

One last word about the SSC,whose balance sheet I’ve never quite understood.It seems that we are depending on massive foreign support for the construction of both the machine and its enormous detectors.We don’t have committments for such support,and we may never do if Europe commits to the LHC and Japan joins their action.Furthermore, it is international lunacy to build and instrument both behemoths.Arguments based on physics goals and technical obstacles convince me that SSC is the better machine to build: LHC is just too small,too hard to build and too hard to instrument.Is the federal govern-ment?nally reaching the sensible conclusion that SSC must be truly internationalized,not only in funding but in management,so that it becomes a facility in America but of and for the World?The search for the secrets of matter and the universe is both glorious and costly.Surely,we must cooperate rather than compete—it’s the way to go,and perhaps the only way.

Acknowledgements

We gratefully acknowledge communications with P.Frampton and U.Amaldi.This work was supported in part by NSF grant PHY-87-14654and by TNRLC grant RGFY9106.

References

[1]S.Dimopoulos and H.Georgi,Nucl.Phys.B193(1981)150.S.Dimopoulos,S.Raby

and F.Wilczek,Phys.Rev.D24(1981)1681.L.E.Ibanez and G.G.Ross,Phys.Lett.

B105(1981)439.

[2] E.g.,P.Frampton and S.L.Glashow,Phys.Lett.B135(1983)340.

[3]H.Georgi and D.V.Nanopoulos,Nucl.Phys.B159(1979)16.H.Georgi ans S.Dawson,

Nucl.Phys.B179(1981)477.

[4] E.g.,U.Amaldi,W.de Boer,H.F¨u rstenau,Phys.Lett.B260(1991)447.A.Giveon,L.

J.Hall and U.Sarid,Berkeley preprint.F.Anselmo,L.Cifarelli,A.Petermann and

A.Zichichi,CERN https://www.doczj.com/doc/6917046648.html,ngacker and M.Luo,Univ.of Penn.preprint.See

also:S.Dimopoulos,S.Raby and F.Wilczek,Physics Today(Oct.1991)25.

[5]U.Amaldi,W.de Boer,P.Frampton,H.F¨u rstenau,and J.Liu,private communica-

tion.

福克斯维修保养使用手册修订版

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图20-4 机油加注口盖2、用10号加长套筒+短接杆 +小飞扳,按照从外向内 对角线的方法拆下发动 机罩盖螺栓(8个),并取 下发动机罩盖,放入零件 车内。 图20-5 发动机罩盖 图20-6发动机罩盖2、向上取下机油反射罩, 并放入零件车内。 注意:机油反射罩有机油应 擦拭干净。

4、向外打开正时齿轮上防护 罩上的两个弹簧钢片卡, 并取下正时齿轮上防护 罩,放入零件车内。 图20-8 弹簧钢片卡 图20-9正时齿轮上防护罩。 5、用5号内六角接头+中飞 扳依次取下正时齿轮中 防护罩上的螺栓(3个), 并取下正时齿轮中防护 罩,放入零件车内。 图20-10 拧松正时齿轮中防护罩上的螺栓

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目录 目录 (1) 1.2自动变速器 (2) 1.2.1 4F27E变速器简介 (2) 1.2.2 4F27E变速器内部结构 (2) 1.2.3 4F27E变速器执行元件工作表 (13) 1.2.4 4F27E变速器电子控制系统 (15) 1.2.5 检查与调整 (18)

福克斯自动变速器的控制原理与常见故障 作者:李超年级:2013级汽车检测与维修技术地址:昆明工业职业技术学院 1.2.1 4F27E变速器简介 4F27E自动变速驱动桥,是一种设计用于前轮驱动车辆的电子控制4速变速驱动桥,目前此款变速器装配在1.8L和2.0L排量的福克斯上。 4F27E代表的是: 4 – 4个前进驱动档位 F –前轮驱动 27 –最大输入扭力365 Nm (270 lb-ft) E –全电子控制。 变速器基本参数 1.2.2 4F27E变速器内部结构 4F27E变速箱的机械传动系统的内部结构为:

一组行星齿轮组—复合式行星齿轮组 一组制动器—低/倒档制动器 一组制动带—2/4档制动带 一组单向离合器—低档单向离合器 三组摩擦片式离合器—前进档离合器/倒档离合器/直接档离合器 输出轴差速装置 复合式行星齿轮组 4F27E采用了一组复合式行星齿轮组,该类型的行星齿轮组的特点是前行星轮架与后齿圈一体运转,而后行星轮架与前齿圈一体运转。前后的行星轮和太阳轮则是互相独立的。基本结构如下图所示。

低倒档制动器/单向离合器/行星齿轮组

编号名称编号名称 1 低/倒档制动器活塞11 低档单向离合器 2 低/倒档制动器回位弹簧12 卡环 3 低档单向离合器内座圈13 前齿圈 4 低档单向离合器固定环14 前行星齿轮/后齿圈总成 5 低/倒档制动器波形片15 前行星托架推力轴承 6 低/倒档制动器钢片16 卡环 7 低/倒档制动器摩擦片17 前太阳齿轮 8 低/倒档制动器压片18 前太阳齿轮推力轴承 9 低/倒档制动器卡环19 后行星齿轮总成 10 低档单向离合器固定器20 卡环 前进离合器

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来说,风险就更大了,发动机几乎肯定会报废。所以按照厂家的建议及时更换正时皮带是非常重要的。 今天的讲座就先进行到这里,如果大家还有什么不明白的地方,可以随时来查询,我们下期为大家准备的车辆保养小知识是讲一讲汽车保养包括哪些项目,希望在这里可以再次看到您的身影。

伊兰特正时皮带更换方法

一)拆卸 注意:记录正时皮带盖螺栓的不同长度。 1.支撑住发动机。 2.拆卸: 发动机辅助传动皮带 ?水泵皮带轮?曲轴皮带轮螺栓 ?曲轴皮带轮 ?正时皮带盖 3.转动曲轴到1号气缸的上止点。确保曲轴链轮、凸轮轴链轮、机油泵链轮和平衡轴链轮正时标记4、5、6、7对齐。 注意:凸轮轴链轮上的定位销8应面朝上。 拧松张紧器螺栓9。将张紧器移离皮带并稍稍拧紧螺栓。 5.拆卸: ?自动张紧装置螺栓 ?自动张紧装置11 ?正时皮带 ?曲轴中心螺栓12 ?曲轴链轮13 ?曲轴导向垫圈14 拧松平衡轴皮带张紧器螺栓15。将张紧器移离皮带并稍稍拧紧螺栓。 7.拆下平衡轴正时皮带 (二)安装 .确保正时标记5、6、7、22对齐。 注意:凸轮轴链轮上的正时标记应与上气缸盖表面对齐-5。排气链轮标记在凹槽上,但进气链轮标记在齿上。 注意:为检查机油泵链轮是否正确定位:从气缸体拆下塞子23。在孔内插入一个8mm十字螺丝刀。确保螺丝刀从气缸体表面插入60mm。如果螺丝刀只能插入20mm:转动机油泵链轮360°。再次插入螺丝刀。 .拧松平衡轴皮带张紧器螺栓15。顺时针转动张紧器以张紧皮带。拧紧螺栓到15-22N?m。.用手压皮带▼处。皮带应挠曲5-7mm。 .如果不是:重复操作2-5。 .安装: ?曲轴链轮导向垫圈14 ?曲轴链轮13 .将曲轴中心螺栓12拧紧至110-130N?m。 注意:确保曲轴链轮导向垫圈装配正确。装配以前用油涂抹曲轴螺栓螺纹和表面。 .检查张紧器体11是否泄漏或损坏。如有必要,进行更换。 9.检查推杆突出部分16是否为12mm。如果不是:更换自动张紧装置。 10.慢慢将推杆压入张紧器体11,直到孔对齐。应感觉到有阻力。 注意:在张紧器体下放置平垫圈,以免损坏张紧器体端部螺塞。 11.用合适的销子穿过张紧器体内的孔来固定推杆17。 12.将自动张紧装置安装到气缸体。拧紧螺栓到22-27N?m。 13.从张紧轮开始,按逆时针方向装配正时皮带。 14.拧松张紧轮螺栓9。顺时针转动张紧轮以暂时张紧皮带,拧紧螺栓到43-45N?m。

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