|
November 2, 2011: CERN Experiment and Violation of Newton’s Second
Law Englishview
October 13, 2011: CERN Experiment and Violation of the Newton’s
Second Law Persianview
November 24, 2008: A New Definition of Gravitonview
July 10, 2007: Zero Point Energy and the Dirac Equationview
July 10, 2007: Zero Point Energy and the Dirac Equationview
June 28, 2007: Unification and CPH Theoryview
June 14, 2007: Summary of Physics Conceptsview
June 14, 2007: Strong Interaction and CPH Theory Rview
June 4, 2007: Quantum Electrodynamics and CPH Theoryview
November 30, 2006: Vocabulary of CPH Theoryview
November 17, 2006: Thermodynamic Laws Entropy and CPH Theoryview
November 17, 2006: Time Function and Absolute Black Holeview
October 14, 2006: CPH and Timeview
October 13, 2006: CPH Theory and Newton's Second Lawview
October 13, 2006: Time Function and Work Energy Theoremview
October 13, 2006: CPH Theory and Special Relativityview
October 13, 2006: Properties of CPHview
July 31, 2006: A New Mechanism of Higgs Bosons in Producing Charge
Particlesview
July 31, 2006: A New Mechanism of Higgs Bosons in Producing Charge
Particlesview
May 14, 2006: Speed of Light and CPH Theoryview
May 14, 2006: Speed of Light and CPH Theoryview
April 28, 2006: Color Charges Curve Spaceview
April 28, 2006: Color Charges Curve Spaceview
April 17, 2006: Effective Nuclear Chargeview
April 17, 2006: Effective Nuclear Chargeview
April 12, 2006: Maxwell's Equations in a Gravitational Fieldview
April 12, 2006: Maxwell's Equations in a Gravitational Fieldview
April 11, 2006: Realization Hawking - End of Physics by CPHview
April 7, 2006: Questions and Answers on CPH Theoryview
April 7, 2006: Opinions on CPH Theoryview
April 7, 2006: Opinions on CPH Theoryview
April 7, 2006: Questions and Answers on CPH Theoryview
March 23, 2006: Analysis of CPH Theoryview
March 23, 2006: Analysis of CPH Theoryview
March 21, 2006: Logical Foundation of CPH Theoryview
March 21, 2006: Definition Principle and Explanation of CPH Theoryview
March 21, 2006: Logical Foundation of CPH Theoryview
March 21, 2006: Definition Principle and Explanation of CPH Theoryview
March 21, 2006: Experimental Foundation of CPH Theoryview
March 21, 2006: Experimental Foundation of CPH Theoryview
March 19, 2006: Color Charge/Color Magnet and CPHview
March 19, 2006: Sub-Quantum Chromodynamicsview
|
|
|
|
|
|
A Fascinating New Higgs Boson Search By The DZERO
Experiment |
|
| |
|
A Fascinating New Higgs Boson Search By The
DZERO Experiment
By Tommaso
Dorigo

Reporting on scientific results to a broad audience is difficult, in
my opinion, not so much because of the need to explain things in a
simple way -which is easy and fun, once you master the matter- as
for the self-discipline you are forced to stick to.
Things that are obvious to you, because you have seen them and
studied them for years, are not obvious to others, not even to
fellow scientist from the other door who practice a just slightly
different sub-field of research, let alone to the larger pool of
smart readers who are drawn to science readings but have never taken
an advanced course on the matter. An alarm bell has to go off every
time you hit on a concept which is likely unfamiliar to most:
maintaining in good operation that alarm bell is by far the hardest
part. At least, that is what my experience tells me.

So let me try and check how rusty that alarm bell is today, as I
make an attempt at reporting in hopefully simple terms on a new
particle physics search by the DZERO experiment (see right), one for
a subatomic process that I find extremely interesting, and which,
once found, will make manifest the hard core of our theory of
electroweak symmetry breaking, a fundamental pillar of our current
understanding of the subnuclear world. This process is the
associated production in hadron collisions of three of the fanciest
building blocks that Nature (the bitch, not the magazine) has
provided our playground with: a top-antitop quark pair, and a Higgs
boson.
This, by the way, is a good point for you to jump ahead by a couple
of sections in this long post, if you are curious about the new
DZERO result but know about, or are not interested in, some
underlying basic facts about hadron collisions.
Some background on hadronic collisions
In the case of the result I report today the hadron collider at hand
is not the LHC, the fast-asleep giant sitting underground below the
border between Switzerland and France, but rather the quite awake
Tevatron collider of Batavia, Illinois, which is traversed daily by
a few micrograms worth of protons and antiprotons, all rigorously
traveling at 99.9 and something percent of the speed of light.
As protons and antiprotons hit each other at that fantastic speed,
they often just bounce off each other retaining their integrity:
physicists call that process "elastic scattering", but they are not
interested in it, because it tells them about as much on the inner
structure of matter as a glance at a glass of wine can tell you
about its tannins.
In closer encounters the protons may break apart, but still nothing
much happens. It is only in those rarer instances when one of the
most energetic quarks or gluons making up a proton hit directly one
of their kin from the antiproton that things become interesting. The
collision is then hard enough that the two constituents -we call
them "partons"- kick each other off their envelopes, the parent
proton and antiproton: they then materialize in the form of streams
of subatomic particles, energetic sprays that we call hadronic
jets; in still rarer instances, their interaction instead gives
rise directly to new states of matter.
(I have explained elsewhere why quarks
can only be seen as jets, and I will avoid repeating myself
here. Suffices to say that quarks cannot exist isolated, and they
must "dress up" in the form of hadrons. Hadrons are composed of
pairs or triplets of quarks: it is them, and not individually their
constituent quarks, the particles that make up the jets we observe
in energetic collisions.)
Doing business with a hadron collider -a proton-antiproton collider
like the Tevatron, for instance- is a frustrating experience: you
spend your money and wits to build a machine that accelerates those
particles at incredibly high energies, and then as you turn it on
would like to see that energy materialize into fantastically
energetic jets, or even better, new exotic, massive particles that
can only be produced by exchanging the projectiles' kinetic energy
into mass. Instead, you have to accept the fact that most of the
collisions you get release way less energy than the total
theoretically available.
That is because what is colliding are not really the proton and
antiproton that you launched one against the other -or more
precisely, one each among a trillion of the former and a hundred
billion of the latter. What really collides is a (anti)quark or a
gluon inside one projectile and a (anti)quark or a gluon inside the
other. And, since these constituents of the proton only carry a
small fraction of the total kinetic energy of their parent
"envelope", the total energy release is smaller than the sum of
proton and antiproton kinetic energy.

Particle physicists learn this fact in their playground years. Parton
Distribution Functions(PDF) have been devised to describe what
is the probability that a quark or a gluon is found with a given
fraction of their envelope's total energy. The graph on the left
shows their density as a function of the fraction x the partons
carry, for different parton species: g labels gluons, u are up-type
quarks, d are down-type quarks, etcetera. Needless to say, these
functions get vanishingly small as the fraction approaches unity: at
the Tevatron for instance you will never, ever, get a collision
releasing 1.96 TeV, which is the sum of the proton and antiproton
energies provided by the superconducting, 4-mile-long accelerator.
The same, of course, goes for the LHC: 14 TeV will never be actually
reached by that machine; nope: not even if its currently ongoing
repairs exceed expectations!
How energetic can a collision be at the Tevatron, then ? That
depends: the larger the number of collisions you observe, the higher
is the chance to see a very energetic one. The most energetic
collisions recorded by CDF and DZERO, the two experiments built
around the points where the Tevatron proton and antiproton beams
intersect, have a total energy release of about 1 TeV, but they are
exceedingly rare. Below is a 2-D bar chart of the energy read out by
the DZERO detector for two high-energy jets: the detector is like a
cylinder surrounding the collision point, and it has been cut along
one side and unrolled on the plane you see, to display the localized
energy deposits of the streams of hadrons which hit it. Such events
are spectacular: they are as close as you can get to actually
"seeing" two quarks.

Enter the production process
Now, the above introduction served one important purpose besides
sorting out the few of you who really want to get personal with
elementary particles: it provides important input to figure out why
the production of a top-antitop quark pair AND a Higgs boson is so
rare and special. It is only a part of the whole story, but let me
use the acquired knowledge at once. Top quarks are the heaviest ones
in the lot of six we have figured out matter can be made of. They
weigh about 173 GeV each, which is the total weight of about 184
hydrogen atoms! As for the Higgs boson, we may assume it weighs 120
GeV here for the sake of argument: existing experimental hints point
to a
value not too far from the one above.
Let us make a simple addition: two top quarks, plus a Higgs boson,
already make a rest mass of 470 GeV. This is about a quarter of the
total kinetic energy of a proton-antiproton pair at the Tevatron,
and it is an energy which is only reached once in a million
collisions or so. Those PDF are indeed functions steeply peaking
when the fractional energy is close to zero, as I noted above.

There is at least another important thing to consider. Not all
collisions above 470 GeV produce a top, an antitop, and a Higgs
boson! Quite on the contrary, that piece of magic is a rare
occurrence regardless of the energy release. The rules for computing
the probability of subatomic production processes like the one we
are discussing are enshrined in Feynman diagrams, graphs which
describe the space-time propagation of the colliding and produced
particles. On the left you can see one such diagram: time is taken
to flow from left to right here, and only one space dimension is
drawn, on the vertical axis.
As you see, the way a reaction
occurs works by first producing a top-antitop pair, and then letting
the duo (in the case shown) "radiate off" a Higgs particle. Such a
feat is predicted to occur because the Higgs boson couples to
any particle if the latter possesses a mass, and that is for sure
something that top quarks are good at -they are the heaviest
elementary bodies known to us. Just as a photon can be emitted by
any electrically charged body, and it does so more readily if the
charge of the latter is higher, a Higgs boson will happily be
emitted by any mass-endowed particle. The difference, however, is
that Higgs bosons are very heavy themselves, and you cannot produce
mass out of nothing: the top quark originating the Higgs boson has
better be very energetic to enable Higgs radiation.
Computing precisely the rate of tth production is beyond my
decidedly experimental expertise, but from the few hints I provided
above you can probably accept that such rate is seriously dampened
by asking for a very specific way of spending the 500 or more GeV of
energy we have already dearly paid for (a one-in-a-million chance,
give or take a cow or two). The easiest way to release that energy
for a proton-antiproton collision would be to produce two 250-GeV
jets like the ones pictured above: any quark pair would do, and even
a pair of gluons would be a very probable solution. Asking for top
quarks makes this much less probable because most of the energy has
to go into the mass of the two fat guys; and asking that one top
quark spits out a Higgs boson makes this a real rarity.
(If you need more detail, here is an important piece: the dampening
in part comes from the narrowness of a thing called phase
space. Given a fixed 500 GeV energy budget to materialize a
pair of quarks, Nature way prefers light-mass ones, since almost all
the initial energy may then be allocated to endowing quarks with
large momenta, and large momenta translate in a larger span of
allowed configurations. The more configurations, the more probable a
process is! But in our case it is still worse: we need one of the
top quarks to be produced with a mass much larger than its nominal
173 GeV, since we need the surplus to materialize the Higgs boson
via radiation. Short-lived particles can indeed be created off-mass-shell,
but the probability for this to happen rapidly decreases with the
departure from their rest mass.)
From the above discussion you have certainly gathered that there are
several factors making tth production a very rare process. Well,
that is exactly true. And here is the final result: all in all, at
the Tevatron one expects less than one in ten trillion collisions to
give rise to a ttH final state. Once-in-ten-trillions is roughly as
frequent as a total failure of the "save a parent" strategy some
dads and moms adopt when they have to travel, taking different
flights to reach the same destination: once in ten trillion times,
both planes crash (I am purposedly neglecting correlated
catastrophes such as 9/11 here, but you get the point). That is what
I call pretty darn rare, what do you think ?
...And they still search for those!
Despite the rarity of associated production of a top-antitop pair
and a Higgs boson -or maybe because of that!-, the CDF and DZERO
experiments at the Tevatron have started to look for it. That does
not mean the physicists in these collaborations are desperate: a
search for a new physical process predicted by your theory is
intrinsically interesting and worth pursuing even if you predict
your experimental setting cannot reach the required sensitivity to
observe the process, because of a couple of facts.
One: particle theory -the so-called Standard
Model- has reached a high level of refinement, but putting it
to the test in new ways, such as searching for a process that is
predicted to be unobservable in a particular environment, might
eventually spot an otherwise unnoticed breach in the theory, opening
the way to the unknown. Two: by studying peculiar and rare final
states of particle collisions one might stumble in some unexpected,
unpredicted new process, again resulting in a disclosure of new
physics.
Also, please consider: measuring something which is predicted to be
very small or even better, exactly zero (or undiscernible from zero)
is a very effective way to probe your theory, much better than
checking whether physical quantity A is equal to seven hundred
gudungoons or seven hundred and twelve gudungoons. The reason for
this is that zero is a quite peculiar number: any
departure from zero sticks out as a lamppost, while a departure
from a non-zero quantity can at most be as significant as the
prediction is precise. Or if you prefer, a rare unknown effect may
only be seen by checking if zero is exactly zero, rather than if
some non-zero quantity is in the high-gudungoons range or not.
In any case, there one last input I have so far denied you: the
number of collisions that have been produced since 2002 in the core
of CDF and DZERO amounts to about 400 trillions each! If the Higgs
boson exists, a handful of those events have most certainly been
popping up: maybe once a year, but they must have! Now, go tell the
needle hiding in the haystack that DZERO searches for a few events
in 400 trillions, and you'll see it rolling away in laughter. But
physicists are clever! So let me tell you how clever they have been
now.
The DZERO search
DZERO searched for the process
in 2.1 inverse
femtobarns of
collisions, which is little less than a third of what they have
accumulated this far. This delay is due to the gigantic amount of
computing required to reconstruct and analyze the information, as
much as to the complexity of the analyses, which must at some point
"freeze" the datasets they use before performing further steps which
may take months to complete. Inverse femtobarns sound like
complicated things the first time you hear about them, but they
actually simply count the number of projectiles that have crossed a
unit area in the center of the detector. Multiply that by the
"effective area" of their targets, and you get the number of hits.
The first step of the analysis consisted in figuring out the best
way to get rid of most the large number of collision events stored
by the data aquisition system, those which were the least likely to
have originated by the production of the ephemeral trio of heavy
particles and their subsequent disintegration into stable particles
-those actually producing the observable detector signals which
constitute the "event" data.
Here I have to unveil a detail I so far hid: the data stored by
DZERO amount to much fewer than hundreds of trillion events, because
the rate at which collisions occur in the core of the detector
during data taking is about three megahertz -three millions per
second-, which is way too high to allow detector readout and
storage. A online trigger system in fact takes care to neglect those
collisions which resulted in elastic scattering or low-energy
release, and only read out and store the most interesting, energetic
events. The trigger system is one of the most complicated parts of
the detector hardware, but I will not discuss it further here:
suffices to say that the offline analysis starts with a dataset of
only billions of events, ones containing an already pre-selected
signal of high-energy electrons or muons.
Electrons and muons. These are the diamonds collider experiments
mine for. Their presence immediately signals that the original
hadrons gave rise to an electroweak interaction, as opposed to the
much more frequent strong interactions that quarks (and gluons) are
most likely entertain themselves with. A high-energy electron or
muon can only be produced by the decay of a W or Z boson or by a
photon, the carriers of the electroweak interaction. In our case,
these particles signal the decay of top quarks, and DZERO uses their
presence to select a sample of top quark pair decays.
The decay chain of a top quark pair yielding one electron and jets
can be written as follows: .
Here you see that one of the W bosons produced an electron-neutrino
pair, while the other yielded one further quark-antiquark pair. Each
of the quarks (both the bottom quarks duo and the generic ones
labeled by the letter q) produces a energetic jet of hadrons, and
the top-antitop signature one ends up observing in the detector is
called "single lepton", to distinguish it from "all hadronic" and
"dilepton" ones containing respectively only jets or two leptons and
two jets. As for the neutrino accompanying each lepton in the W
boson decay, they leave the detector unseen, but their presence is
inferred by the imbalance in the energy flowing out of the collision
point.
My DZERO colleagues know extremely well how to best select
top-antitop events in the single lepton final state: they have been
doing this since CDF showed the way, in the days prior to the top
quark discovery in 1995. But in the case at hand, a Higgs boson must
be present in the event: this particle, if it is not too heavy,
decays most of the time into an additional pair of b-quark jets. The
total signature DZERO is after is thus one of lepton plus many jets,
nominally six of them. Since, however, jets may be lost in
uninstrumented regions of the solid angle around the collision
point, or overlap to other jets, or fail to have enough energy to
provide a clear identification, DZERO chooses to concentrate on two
different signatures: lepton
plus four jets, and lepton
plus five or more jets.
After selecting the above topologies, the data is still polluted
with processes that have little to do with top quark pair production
(not to mention the exceedingly rare tth events). A further cleanup
is provided by requiring that at least one of the jets contains an
indication of having been originated by a bottom quark. Bottom
quarks are not as heavy as top quarks, and thus are not as rare; but
they are still rare
enough that their
presence is a strong indication of a top decay.
In the end, DZERO applies a technique we might call "Divide et
Impera" (divide and rule): by slicing and dicing the selected
event set into different classes (each consisting in a well-defined
event signature) a small signal is easier to find, even if some
classes will contain a much smaller fraction of it than others.
Below is a table from the preliminary
paper produced by
DZERO: as you can see, electron plus jets and muon plus jets are
separated, and then events with only 4, or 5+ jets, are kept
distinct. Further, the number of b-quark jets identified in the
event (dubbed "b-tags") allows to define a total of 12 exclusive
subsets. To decode them, take "5j2t" as an example: that class
contains events with at least 5 jets (5j), and exactly two b-tags
found in them (2t).

In the table, top-antitop events are estimated separately from
"non-tt backgrounds", to highlight the power of the DZERO selection:
especially in the 2- and 3-b-tags classes, the top contribution far
exceeds the other annoying processes that pollute the selected
dataset. Also, the observed event counts (shown in the last line for
both electron+jet and muon+jet topologies) match pleasingly the
expected sum of backgrounds, indicating that there are no surprises
and possibly no mistakes. Finally, please notice how the number of
events has been reduced by orders of magnitude by the combination of
requirements on the presence of a lepton and many jets. Still, the
expected signal across the table sums up to less than one event. One
event in 626 ? That is not a needle in the haystack anymore! Kudos
to DZERO for their clever selection then!
The final step of the analysis is different from what has become
common practice in the searches of small signals buried in large
backgrounds nowadays. Rather than relying on the modeling of many
observed characteristics of the quite complicated kinematics these
multi-object final states possess, DZERO uses a single, dumb but
foulproof variable: the HT, which is computed as the sum of
transverse energies of all the jets, the lepton, and the inferred
neutrino. This quantity provides a quite model-independent tool to
discriminate tth from tt events, and its use sidesteps a
theoretically nagging problem: our insufficient understanding of the
main background to the search, the production of top-antitop quark
pairs accompanied by bottom-antibottom pairs.
In the figure below, a HT distribution is shown for the sum of the
two classes most "signal-rich": the ones corresponding to five or
more jets and three or more b-tags. The black points show the
observed data events (a total of five entries), and the red
distribution shows the expectation from known processes (basically
dominated by top-antitop production). The black histogram instead
shows the expected HT distribution that the signal would display, if
it had a production rate exceeding by 100 times the predictions from
theory. The different shape of red and black histogram is the whole
point of using HT as a discriminating variable.

The 12 HT distributions are finally tested by comparing data to the
expectation from the sum of backgrounds (which includes both top
production and non-top processes). A complex, very accurate method
is used to combine the variegated information coming from the twelve
distributions into a single response -the ratio between the
probability that the data contain both signal and background
together, divided by the probability that they contain only
backgrounds. The study of that quantity allows to set a upper limit
on the number of signal events contained in the data, which can then
be converted in a limit on the signal cross-section by suitably
multiplying for the signal detection and reconstruction efficiency,
numbers that can be estimated by Monte Carlo simulation programs.
The whole procedure is repeated for different hypotheses of the
unknown value of the Higgs boson mass, and the limit thus becomes a
function of it. The end result is displayed, as has become
customary, as a curve showing, as a function of the Higgs mass, the
ratio between the resulting upper limit on signal cross section and
the cross section that is predicted by the Standard Model theory.
That is to say, if for a given hypothetical Higgs mass a limit is
set at a value equal 100, that means that DZERO's data exclude the
presence of tth production at a rate exceeding 100 times the
predicted production rate, in case the Higgs has that mass.

As you can check in the graph on the right, the limit is not very
stringent! In fact, an exclusion of a mass range for the Higgs boson
would result if the limit curve assumed values below 1.0 in that
range (the hatched black line). Instead, the red curve (labeled Observed
limit) is floating at values well above 30 times the Standard
Model prediction. This should not be read to imply that the DZERO
search has not been fruitful or successful! The result is, in fact,
quite interesting, for several reasons.
First of all, an anomalous coupling of the Higgs boson to the top
quark might boost the production rate above Standard Model
predictions, and the DZERO limit sets a bound on that occurrence.
Second, the final states investigated by the search had never before
studied in detail at the Tevatron, and it feels good to see we do
understand the production of top quarks in association with
b-quarks. Third, the search provides guidance for future
investigations in the same direction. Fourth, the limit, although
very loose, can be combined with advanced statistical procedures
with the much more stringent ones coming from higher-rate production
processes of the Higgs boson, eventually contributing to advancing
our knowledge of that elusive particle. Elusive is certainly an
appropriate word: Higgs bosons have been hypothesized more than
forty years ago, and we still have to see one of them...
The only remaining taks, at the end of this long article, is for me
to ask you, dear readers, whether the alarm bell I mentioned at the
beginning needs to be serviced!
Further reading:
A call for ideas on how to improve a prospective search for tth
events with the CMS detector
Home page of the DZERO experiment
Home page of the Fermi National Accelerator Laboratory
Real-time display of Tevatron performances
Source: Scientific
Blogging
|
|
|
|
|
|
|

|
|
@2003-2012 The CPH theory, All right reserved
|