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Posts Tagged ‘detector’

for B physics?


The title of today’s post is obviously a rhetorical question, because the answer is naturally LHCb. *winks* However I thought I would take some time to prove it with a particular \(B\) meson decay…

One of the most interesting \(B_s^0\) meson decays is that into a \(J/\psi\) and a \(\phi\) meson, shown below. This is because one of the quantities we can derive from this decay has a very small Standard Model prediction, so any measured excess would be a clear indication of new physics.[*]

This decay mode is so interesting that both ATLAS and CMS as well as LHCb are trying to detect it. Hence giving me the opportunity to directly compare the performance of the detectors. So without further ado, here are the results:So what are we looking at here? These are the invariant mass distributions of the identified \(B_s^0 \rightarrow J/\psi + \phi\) decays in each detector. In every event, we look for the products of the particular decay we are interested in. In this case, we need to identify two muons from the decay of the \(J/\psi\) and two kaons from the decay of the \(\phi\). We then take these four particles and add their four-momenta together, if they did originate from the decay of a \(B_s^0\) meson, we should see a peak around the \(B_s^0\) mass of 5366.3 MeV / c\(^2\). This is represented by the data points in the three plots from each of the experiments. The lines on each of the graphs are fits to the data using a normal distribution for the signal and a straight line for the background. [**]

So what do we look for in these graphs to learn about the performance of each detector? Actually, before we do any comparisons, we need to look the size of the datasets used in each analyses. Luckily for us, the datasets are fairly similar, with LHCb reporting results using 36 pb\(^{-1}\) of data, CMS using 39 pb\(^{-1}\) and ATLAS using 40 pb\(^{-1}\). This means we can basically do a direct comparison of the graphs, though with the caveat that each of the analyses used different selection criteria to select their \(B_s^0\) candidates. However, we can assume that they have been optimised to select as much signal as possible while rejecting as background as possible.

Okay, now we have established we can compare the graphs, let’s do so. The first thing you might notice is that the graphs look fairly similar. Each experiment has been able to reconstruct a nice \(B_s^0\) peak from its decay products. Looking closer however, the results have some notable differences, despite each of the experiments looking for the same decay in very similar sized datasets and using the same signal and background distribution shapes.

I’m emphasising the fact that the datasets are similar sizes because you may notice that the number of signal events is fairly different between the three experiments, with 877 events in the signal peak for LHCb, while ATLAS and CMS only see 358 and 377 events respectively. This may not be immediately obvious looking at the height of the signal peaks, but if you notice that each experiment uses different mass binning, it becomes clearer.

So LHCb sees more \(B_s^0 \rightarrow J/\psi + \phi\) decays than ATLAS and CMS. This is actually expected from the geometry of the detectors. As I mention in my very first post, \(B\) meson production peaks in the forward region, shown below, where LHCb has coverage while ATLAS and CMS don’t.

Interesting, even though LHCb sees more signal events than ATLAS and CMS, it sees many less background events. This can be seen in the plots above by see how high above 0 the linear background fit is. We can see that LHCb sees less background then ATLAS, which see less background than CMS. The reason for this is that LHCb is much better at identifying kaons and muons at these energies thanks to the RICH subdetectors.

What else can we learn? If we look at the width of the signal fits of the \(B_s^0\) mass peaks from each experiment, we can see that these are also quite different. The LHCb peak is very narrow at 7 MeV, while the CMS peak is a little wider at 16 MeV and the ATLAS peak is wider again at 27 MeV. These numbers tell us how accurately the momenta of the kaons and muons are measured, and how well the \(B_s^0\) decay vertices are reconstructed. So we see that LHCb is better at measuring the kaon and muon momenta and reconstructing displaced decay vertices.

In summary, LHCb sees more signal, less background and better at measuring the particles involved in \(B_s^0 \rightarrow J/\psi + \phi\) decays compared to CMS and ATLAS. It is therefore clearly the best detector to use for these types of decays. An obvious conclusion, since these decays are what the detector was designed and built to measure, but it is nontheless reassuring to see that the results confirm our hypothesis.

 

[*] I know that this really isn’t a satisfactory explanation of why this particular decay is interesting, but I didn’t want to get too sidetracked here. I’ll save the details for a future post. This one is long enough already!

[**] I have obviously simplified the selection and analysis process immensely. If you do want to find out more information about each of the analyses, and where I got the graphs and numbers, details can be found here for LHCb, here for ATLAS and here for CMS.

Don’t Stop Me Now…

Friday, July 29th, 2011

Today I’m going to describe the last, but definitely not least LHCb subdetector, the muon subsystem, which unsurprisingly from the name, is designed to detect muons. Just in case you’ve all forgotten what the LHCb detector looks like, I’ve included a schematic below. The muon subsystem is the rightmost one, with alternating layers of light and dark green.

So why is a completely separate subsystem required to detect muons on top of the previously described vertex location, tracking, particle identification and calorimeter subsystems?

It all comes down to how muons interact with matter. In my last post, I said that the goal of the LHCb calorimeter subsystem is to stop particles in the detector and measure how much energy is produced through interactions with the detector material. However, I left out the important fact that different particles interact differently with detector material. In particular, muons pass through the calorimeters almost without any energy loss. Flip has a very nice explanation about why in this post, where he compares electron interactions to muon interactions… which he hopefully won’t mind if I borrow…

Electrons are light, so let’s imagine that they’re ping pong balls. On the other hand, muons are heavy, so let’s imagine them as bowling balls. As you probably know, the LHC detectors are big and full of stuff… by that I mean atoms, which in turn are made up of a nucleus and a cloud of electrons. We can thus imagine a sea of ping pong balls (kind of like an IKEA ball pit). When electrons hit this ball pit, they end up distributing all of their energy into the other balls. Muons on the other hand, are so massive that they just barrel straight through the ball pit to reach the other side.

Why go to all this effort just to detect muons?

Apart from muons being the only particle you can make farm jokes about, the fact that muons are the only known particles which the calorimeters don’t stop is quite useful. It means that if any signals are seen in a detector that is located behind the calorimeters, they must originate from a muon. This makes searching for decays involving muons much simpler than searching for decays involving other particles, such as electrons. An example of such a decay is the rare \(B_s \rightarrow\mu\mu\) decay which may reveal new physics, as discussed previous by both Ken and Flip.

So how does LHCb detect muons?

The muon subsystem comprises five rectangular ‘stations’, gradually increasing in size and covering a combined area of 435 square metres. Each station contains chambers filled with a combination of three gases – carbon dioxide, argon, and tetrafluoromethane. The passing muons react with this mixture, and wire electrodes detect the results. In total, the muon subsystem contains around 1,400 chambers and some 2.5 million wires.

Here is a nice photo taken between two of the stations…

So now you know all about the LHCb detector, you should be able to understand the following event display of a \(B_s \rightarrow\mu\mu\) event. If not, don’t fear, because there’s a very good explanation here.

And that ends my series of posts describing the LHCb detector… I hope you all enjoyed reading them as much as I enjoyed writing them.

Stop right there, particle!

Tuesday, July 26th, 2011

Looking back over my previous posts, I noticed that I forgot to describe the calorimeter and muon systems before jumping straight to the trigger. The subject of today’s post will thus be the calorimeters and my next post will probably be about the muon system.

So what is a calorimeter? I vaguely remember that in high school chemistry, we performed a calorimetry experiment to measure the energy change in a chemical reaction by measuring the heat released (for those who are enjoy their etymology, calorimeter derives from the Latin word, calor, which means heat).

It is slightly different in particle physics, where the main function of the calorimeter detector subsystems is to measure the energy of produced particles. The materials and techniques vary, however the basic principle of all calorimeter systems is the same: to stop particles in the detector and measure how much energy is produced through interactions with the detector material.

On my very first post, I mentioned that LHCb contains two calorimeters; the electromagnetic calorimeter is responsible for measuring the energy of electrons and photons, while the hadron calorimeter samples the energy of protons, neutrons and other particles containing quarks. The calorimeters provide the main way of identifying particles that possess no electrical charge, such as photons and neutrons.

Both calorimeters have a sandwich-like structure, with alternating layers of metal and plastic plates. The metal plates are to stop particles, while the plastic plates are to measure the energy released. More technically, when particles hit the metal plates, they produce showers of secondary particles. These, in turn, excite molecules within the plastic plates, emitting ultraviolet light, which is then guided to photomultiplier detectors. The amount of light produced is proportional to the energy of the particles entering the calorimeter.

Above is a photo of the two calorimeters, the one labeled with LHCb ECAL is unsurprisingly the electromagnetic one, while the hadronic one is behind it. It is a little hard to get a sense of scale from the photo, but the electromagnetic calorimeter wall is approximately 6.3 metres by 7.8 metres and 0.5 metres thick, while the hadronic calorimeter wall is around 8.4 metres by 6.8 metres and 1.7 metres thick.

I think that’s all I have to say about the LHCb calorimeters, except to leave you all with this random fact. The specific design of the electromagnetic calorimeter, its alternate layers of scintillator and lead, readout by plastic fibres which run parallel to the plates, is called shashlik, which is also a type of shish kebab… mmm…

Magnets magnets everywhere…

Tuesday, May 17th, 2011

In my previous posts, I’ve mentioned that LHCb contains a dipole magnet to help measure particle momenta. Particles normally travel in straight lines, but in a magnetic field the paths of charged particles curve, with positive and negative particles moving in opposite directions.
By examining the curvature of the path, it is possible to calculate the momentum of a particle. Particles with greater momentum bend less than those lesser momentum. This is because a particle with greater momentum will spend less time in the magnetic field and thus be affected less.Note that both the above images are from The Particle Adventure which is a fantastic website to learn the basics of particle physics.

Here is an image of the LHCb dipole magnet with some people for size comparison. The magnet is essentially a very large horseshoe magnet with the upper coil being one polarity (N for example) and the lower coil the opposite (S) where the magnetic field is the strongest between them.

Of the major LHC experiments (ALICE, ATLAS, CMS and LHCb), the only other that uses a dipole magnet to bend charged tracks is ALICE. Actually, ALICE has quite an interesting magnet configuration, which you can see from the following schematic. There is a large solenoid magnet (coloured red which was used in the L3 experiment at LEP) in the central region, and a dipole magnet on the single arm forward muon detector.

What’s a solenoid magnet? Here is a schematic of one from physics animations. This type of coil configuration generates a nearly uniform field inside the windings and a comparably weak and divergent field outside. It is the preferred type of magnet within cylindrically symmetric detectors. In fact both ATLAS and CMS use solenoid magnets.

Actually, solenoid is part of the CMS acronym, Compact Muon Solenoid. At 12.9 meters long with an inner radius of 2.95 metres, an outer radius of 3.8 metres, and weighting 12,000 tonnes, the experiment contains the world’s largest superconducting solenoid magnet.

ATLAS on the other hand is named after its other magnet system, A Toroidal LHC ApparatuS. One of the key design features of the ATLAS detector is the unique hybrid superconducting magnet system. It is an arrangement of a central solenoid surrounded by a system of three large air-core toroids, measuring 26 m in length and 20 m in diameter.

What’s a toroidal magnet field? Again, thanks to physics animations, here is a schematic. As you can see, coils are oriented so that the magnetic field goes around in a doughnut type shape. (Toroidal is just a fancy mathematical description for a doughnut shaped object.)

Of course, the LHC experiments aren’t the only uses of magnets at the LHC. The accelerator system is full of them. Dipole magnets are used to steer the protons around the ring, quadrupole magnets are used to focus the beam, sextupole magnets are used to correct chromaticity, octupole magnets are used to correct field errors. What are all these magnets? Here is a nice diagram from some lecture slides I found. As you can see, they are named after the number of magnetic poles they contain (2, 4, 6 and 8, the n in the diagram counts the number of pole pairs). The arrows on the diagram shows the direction of the magnetic fields that each of the magnets produces.

In terms of beam acceleration, dipoles and quadruples are the most important. In fact, if you look carefully at the Fermilab logo below, you might notice the superposition of a quadrupole and a dipole magnet…

I could continue, but this post is getting very long. I hope this very brief introduction illustrates how important magnets are in experimental particle physics. Personally, I wish I had known this when I was taking electromagnetism and electrodynamics in my undergraduate studies, which were actually my worse physics subjects in terms of marks. I really should have paid more attention!

What made those tracks?

Sunday, May 8th, 2011

Last post I discussed how we reconstruct tracks in LHCb. The next logical step is to talk about how we identify what sort of particle left which track. Continuing with my analogy about animal tracking, animals leave very distinctive tracks related to their paw prints and how they move. You can basically tell what animal left a track by examining it carefully…

The above image was taken from this webpage.

Unfortunately is is not possible with particle tracks. Only given the parameters of a reconstructed track, there is no way to determine what type of particle left that track. More information is required and that is where the RICH1 and RICH2 detectors come in.

The identity of a particle can be determined from its mass. The mass of a particle can be determined from its momentum and speed. The momentum of a charged particle is measured by its deflection in a magnetic field. The purpose of the RICH detectors is to match this information with a measurement of the particle’s speed.

RICH detectors work by measuring emissions of Cherenkov radiation. A charged particle traveling faster than the local speed of light in a medium emits Cherenkov radiation in the form of light, in a cone at an angle which depends on the speed of the particle. The RICH detectors focus the cone of Cherenkov light into a ring using mirrors onto an array of detectors. The radius of this ring provides information about the particle’s speed. Here are a few of the rings seen in RICH2 from an early LHC event.

The system of RICH detectors consists of an upstream detector (RICH1) which uses silica aerogel and \(C_{4}F_{10}\) gas as Cherenkov media located just behind the VELO, and a downstream detector (RICH2) using \(CF_{4}\) positioned after the magnet and tracking system. The use of silica aerogel allows the detector to identify low momentum particles (order of a few GeV), the use of \(C_{4}F_{10}\) allows the identification of higher momentum particles (between 10 GeV to around 65 GeV), while the use of \(CF_{4}\) allows the identification of even higher momentum particles (between 15 GeV to around 100 GeV).

Here is a schematic of the RICH1. Particles will enter the detector from the VELO on the left, then travel through the Cherenkov media, producing Cherenkov light which are reflected by the mirrors into the photon detectors. RICH2 is fairly similar.

The two RICH detectors are responsible for identifying a range of different particles that result from the decay of B mesons. Particle identification is crucial to reduce background in selected final states. For example, in the plots below, we are searching for the decay of a \(B_s\) meson into two \(K\) mesons. On the left, you can see that without the RICH it would be very hard to separate the signal, shown in red, from the backgrounds, since we would have no way of accurately differentiating \(K\) mesons from \(\phi\) mesons and \(\rho\) mesons. We would also have problems differentiating between \(B_s\) mesons and \(B_d\) mesons. On the right, using the RICH detectors, you can see that the signal is much much cleaner. They are very nice, useful detectors!

Are those tracks?

Sunday, May 1st, 2011

Today’s post is a continuation of my description of the LHCb detector. From my other post on identifying vertices using the VELO, we naturally progress to tracking charged particles. As I mentioned in my first post, the VELO along with the TT, T1, T2, and T3 stations are used to reconstruct particle tracks inside LHCb.

Particle tracking is somewhat akin to animal tracking. The first thing you need is some material where particle tracks will leave a trace. It is very hard to find animal tracks on concrete, but very easy on sand or snow…

This where the VELO along with the TT, T1, T2 and T3 come in. When charged particles pass though these detector components, they leave hits. Two different types of technology are used to measure particle interactions. The VELO, TT and the inner sections of the T stations are made of layers of silicon strips while the outer sections of the T stations consist of straw tubes filled with a mixture of argon and carbon dioxide gas. The layout of the TT and T stations is shown below. The silicon sections are coloured purple, while the drift tube sections are coloured blue.

Depending on which detector components register hits, tracks can be classified into four different groups:

  1. Long tracks which pass through all parts of the tracking system, from the VELO, through the TT to the outer T stations;
  2. Upstream tracks which only pass through the VELO and TT stations;
  3. Downstream tracks which only pass though the TT and T stations;
  4. VELO tracks which only pass through the VELO; and
  5. T tracks which only pass through the T stations.

Each of these track types is shown in the image below:

All of these types of tracks are useful for reconstructing B meson events. An example of a reconstructed event is displayed below. The average number of successfully reconstructed tracks in fully simulated B meson events is about 72, which are distributed among the track types as follows: 26 long tracks, 11 upstream tracks, 4 downstream tracks, 26 VELO tracks and 5 T tracks.

You may notice that in the images above, the tracks are curved. This is due to the LHCb dipole magnet. The experiment contains what essentially is a very large horseshoe magnet, which produces a field of 4 Tesla between its two large coils. Particles normally travel in straight lines, but in a magnetic field the paths of charged particles curve, with positive and negative particles moving in opposite directions.

So that’s how we measure particle tracks in LHCb and the types of tracks we record. Stay tuned for how we figure out what type of particle left which track…

VELO: it moves!

Sunday, April 17th, 2011

I’m not ashamed to admit that I spend a fair bit of time monitoring what the LHC is doing. Luckily there is a very good set of web pages that allow me to do this, the first of which Brian discusses in this post.

Below I’ve got stills of Page 1 and Page 3 when the beam is in Adjust and Stable modes.

LHC Page 1 - Adjust Mode
Adjust Mode
LHC Page 1 - Stable Beams ModeLHC Page 3 - Stable Beams Mode
Stable Mode

It’s a little hard to see, but I’ve highlighted particular sections of each page. First on Page 1 there’s a small entry titled Movable Devices Allowed In, while on Page 3 there’s a special entry for the LHCb VELO Position.

These two small entries in the LHC status pages are probably all that people outside LHCb know about the VELO, and even then the first entry isn’t an obvious reference.

So what is the VELO? And why does it move?

The VErtex LOcator is the part of the LHCb detector closest to the collisions at the LHC. As I mentioned in my previous post, its job is to measure particle tracks to precisely separate primary and secondary vertices and that this is important to identify B mesons and their decay products.

This is possible through the use of 42 silicon modules which during physics data taking are positioned as close as 5mm from the interaction point.

While it is important for the sensors to be close to the beam during physics data taking for optimal precision; at these small distances, there is a high probability that the modules will sustain damage due to radiation from the high energy proton beam.

To prevent damage, the silicon modules are mounted on custom made bellows, which allow the VELO to retract to the safer distance of 30mm from the beam during periods of beam instability.

Below is a schematic of the silicon modules from the side and from the front, in both open and closed positions, followed by photo of the actual modules during the assembly process.
VELO Schematic

Module assembly

The VELO is a very impressive feat of physics and engineering. It is not an easy task to design a set of silicon chips and associated services to operate so close to a high energy proton beam and its associated electromagnetic effects. And it works! Beautifully, as can be seen from this view of one of the first reconstructed B mesons…


I like to think it is because of Syracuse’s involvement in the subdetector, but Syracuse is just a spoke in the collaboration…

Syracuse LogoNIKHEF LogoLiverpool LogoGlasgow Logo

Greetings and salutations everybody! I’m gratified and honoured to be the first LHCb US LHC blogger. As well being new to US LHC, I’m also new to the LHCb collaboration, so we can all learn about LHCb and B physics together.

Today I thought I would start by introducing the LHCb detector. Here is a schematic:

LHCb DetectorIf you are familiar with the two largest LHC experiments, ATLAS or CMS, this may look a little different to you. LHCb is not a general purpose detector, with the aim of detecting as many different types of physics events as possible; it is especially designed to measure the decays of (B) mesons (more about why we care specifically about (B) mesons in a future post).

ATLAS and CMS are essentially cylindrical in shape, while LHCb is a cone, taking advantage of the strongly forward peaked probability distribution of (B) meson production. This means that while the detector only covers around 4% solid angle, it is able to measure around 40% of (B) meson production.

The decay products of (B) mesons are identified and measured by different detector components:

  • Closest to the proton-proton interaction region is the vertex detector, known as the VELO. Its job is to measure the particle tracks to precisely separate primary and secondary vertices. This is important to identify (B) mesons and their decay products. For example, in the image below, we have been able to identify three vertices: PV, SV and TV, and associate them with particular events: PV – the production of an (B_s) meson, SV – the decay of the (B_s) meson into a muon and a (D_s) meson, and TV – the decay of the (D_s) meson into a (K) and two (pi) mesons. These three vertices could not have been identified without the VELO.Reconstructed multiple=
  • There are two ring imaging Cherenkov detectors, known as RICH1 and RICH2, which are used for particle identification. For example, they can differentiate between the (K) and the (pi) mesons in the decay chain described above.
  • Reconstruction of charged particle tracks and momentum measurement is performed by the tracking system, made up of the TT, T1, T2 and T3 stations in the schematic.
  • Following these are the electromagnetic and hadronic calorimeters (ECAL and HCAL), which measure the energy of electrons, photons and hadrons.
  • Finally, there are there is the muon system (M1, M2, M3, M4 and M5), which identifies and measures muons.

Along with these detector components, there is a dipole magnet to help measure particle momenta. Particles normally travel in straight lines, but in a magnetic field the paths of charged particles curve, with positive and negative particles moving in opposite directions. By examining the curvature of the path, it is possible to calculate the momentum of a particle.

There you have it, a brief overview of the LHCb detector and its components. This is what it looks like in reality:LHCb in realityNote that I’ve flipped the photo horizontally so it is easier to match the detector components in the schematic to their real counterparts.

On ALICE

Thursday, February 3rd, 2011

The electromagnetic calorimeter is now fully installed but there’s still work to do before we start running.  We now have to make sure we’re able to read all of the data.  I’ve spent most of the last week in, on, and next to ALICE troubleshooting (along with several of my colleagues working on the calorimeter.)  Here I am sitting inside the magnet on top of  the support structure next to the front end electronics (the boards that read out the data) for the calorimeter.  I’m on the phone with someone upstairs who’s trying to take a pedestal run to see if we’ve fixed a problem reading out data from one of the new supermodules.  (A pedestal run is a run you take without proton-proton or lead-lead collisions to see what the background in your detector is.  It’s useful for troubleshooting because the detector has to send data.)

Now that we’re getting close to the start of the run, they’re putting the concrete shielding in.  In total 30 or 40 tons of concrete blocks sit above ALICE.  Here you can see one of the last blocks going in:

And just to go along with the preposition theme, here’s a picture under ALICE (in the magnet but under the TPC, TRD, and TOF):

Inside ALICE

Sunday, January 30th, 2011

I am currently at CERN to work on getting the electronics for the electomagnetic calorimeter working now that the rest of it is installed.  I got to see the ALICE detector in person for the first time on Thursday, which was very exciting.

This is a picture of me in front of the detector:

But that was part of a tour and to work in the detector I needed a lot of training.  I needed to take

  • Radiation safety training – there can always be residual radiation from things that have been activated by the beam and there may be radioactive sources in the area.  I have to recognize the appropriate placards and understand any dangers that may be present.
  • Working at heights training – the electromagnetic calorimeter is not at ground level and working on the electronics requires me to work well above ground.  I have to know how to use a harness properly.
  • Confined space training – the doors of the magnet are closed now so that they can start replacing the shielding around ALICE and I need to work inside the magnet.  This is a confined space.  There is a risk of oxygen deficiency – the amount of oxygen can drop rapidly and I have to to be aware of potential dangers and ready to respond.
  • Biocell training – The biocell is a small container of oxygen which I have to carry with me at all times in case the oxygen levels rapidly drop.  I have to be trained to use this properly because I may need to use it to save my life.

I also have to wear a dosimeter (which measures how much radiation I’ve been exposed to), a hardhat with a headlamp (in case the power goes out), and safety (steel-toed) shoes.  No shorts are allowed.  Inside the magnet there are high voltage sources, risks of falling, risks of falling objects, and detectors using flammable and/or toxic gases which could leak.  We are required to have at least two people working inside the magnet at a time – so that if someone gets hurt, the other person knows and can get help – and to have a 3rd person outside the magnet as a watcher keeping track of who is inside and where they are so that if anyone gets hurt or there is an emergency there is someone who can call the fire brigade and tell them how many people are inside and where they are.

I haven’t had the opportunity to take any pictures inside ALICE yet – and safety always has to come first so I may not be able to – but this is the hole we use to enter the magnet:

It is about 60 cm in diameter.  To get down to ALICE, you first have to go through this door:

(This is Soren Sorensen, my boss, coming down to see ALICE.) To go through this door, I have to scan my dosimeter on a card reader.  This says who I am and whether or not I have access to “the cavern” – the space underground where the detector is.  Then the outer doors open, I walk in, and I’m closed inside.  They scan one of my eyes and weigh me to make sure that I really am the person who owns the dosimeter.  Only then am I allowed in.  Inside there’s an elevator that takes us the 70m down to ALICE.  (It is easier to go down to see the cavern as a visitor than to work on the detector – one does not need training but must be supervised.)

This is why we tested as many components of the electromagnetic calorimeter  as possible before the EMCal was installed.  However, there will always be something which doesn’t work quite right and we want to fix it if we can.  It’s really exciting work, but we have to stay alert and stay safe.