The Higgs and Beyond

Excerpt from: The Standard Model of Particle Physics by Tom W.B. Kibble

(Credit: particleadventure.org)

This may seem a very strange theory but it is now well established; QCD and the electroweak theory together constitute the standard model, with spin -½ leptons and quarks and spin – 1 gauge bosons. It has been tested by innumerable experiments over the last forty years and been thoroughly vindicated.

Until recently there was however a gap, the Higgs boson. Back in 1964, the existence of this extra particle was seen as a relatively minor feature; the important thing was the mechanism for giving masses to gauge bosons. But twenty years later, it began to assume a special significance as the only remaining piece of the standard – model jigsaw that had not been found.

Real CMS proton-proton collision events in which 4 high energy muons (red lines) are observed. The event shows characteristics expected from the decay of a Higgs boson but is also consistent with background Standard Model physics processes. (Credit: CERN, for the benefit of the CMS Collaboration)
Real CMS proton-proton collision events in which 4 high energy muons (red lines) are observed. The event shows characteristics expected from the decay of a Higgs boson but is also consistent with background Standard Model physics processes. (Credit: CERN, for the benefit of the CMS Collaboration)

Finding it was one of the principal goals of the large hadron collider (LHC) at CERN. This is the largest piece of scientific apparatus every constructed, a precision instrument built in a huge 27 km – long tunnel straddling the French – Swiss border near Geneva — a truly remarkable piece of engineering. Protons are sent round in both directions, accelerated close to the speed of light, and allowed to collide at four crossing points around the ring. At two of these are large detectors, Atlas and CMS, also marvels of engineering, that over a period of twenty years have been designed, built and operated by huge international teams of physicists and engineers. In 2012 this mammoth effort paid off, with the unequivocal discovery by both teams of the Higgs boson.

Aerial of Cern (Credit: CERN / LHC)
Aerial of Cern (Credit: CERN / LHC)

So is this the end of the story? Surely not. The standard model can hardly be the last word.

It is marvelously successful, but far from simple. It has something like 20 arbitrary parameters, things like ratios of masses and coupling strengths, that we cannot predict and that seem to have no obvious pattern to them. Moreover there are many features for which  we have no explanation. Why for both quarks and leptons are there three generations with very similar properties but wildly varying masses? Why do quarks come in three colours?

One theory is that all these choices are random. There may have been many big bangs, each producing a universe with its own set of parameters. Most of those universes would probably be devoid of life. But that is for many a profoundly unsatisfactory answer; we certainly hoped for a more predictive theory!

Grand Rebound (Credit: Unknown)
Grand Rebound (Credit: Unknown)

On the observational side, there are still many things we cannot explain. What is the nature of the dark matter in the universe? Why does the universe contain more matter than antimatter — leptons and quarks rather than antileptons and antiquarks? Moreover there are a few points on which the standard model definitely does not agree with observation. In particular, in the standard model the neutrinos are strictly massless. But we now know that do in fact have non-zero, albeit very tiny, masses. We really have no idea why.

The slight difference in the gravity of Earth in different locations illustrated. (Credit: NASA)
The slight difference in the gravity of Earth in different locations illustrated. (Credit: NASA)

Finally, there is the elephant in the room: gravity, which does not appear at all in the standard model. It is in fact very difficult to reconcile our best theory of gravity, Einstein’s general theory of relativity, with quantum theory. That is a problem we have been struggling with for the best part of a century. There are hopes that string theory, or its more modern realization, M-theory, may successfully unite the two, but that effort has been going on for decades without as yet reaching a conclusion. At any rate it does appear that there is a lot more for theoretical physicists to do!

Excerpt from: The Standard Model of Particle Physics by Tom W.B. Kibble. Blackett Laboratory, Imperial College London  arXiv:1412.4094 (PDF)

Physics in the News

Saturday, October 11, 2014

Leaky galaxies lead researchers to better understand the universe

 This is Sanchayeeta Borthakur, assistant research scientist in the Department of Physics and Astronomy at the Johns Hopkins University. (Photo Credit: JHU)
Sanchayeeta Borthakur, an assistant research scientist in the Department of Physics and Astronomy in the university’s Krieger School of Arts and Sciences, reports in a paper published online Oct. 9 in the journal Science that an indicator used for studying star-forming galaxies that leak radiation is an effective measurement tool for other scientists to use. (Credit: JHU)
via sciencecodex

L.A. Museum Adds the Last Payload to Shuttle Endeavour

141010-shuttle_c92e33917bf64aaa38d9790b47f34c7f.nbcnews-ux-1240-800
During an event titled “Go for Payload,” the California Science Center in Los Angeles hoisted a Spacehab module into the open hold of the retired space shuttle Endeavour. The logistics module’s addition, together with several other real and replica parts, marked a major milestone towards the center’s plans to display the NASA winged orbiter in a vertical, launch-ready configuration. (Pearlman, CollectSpace.com)
via nbcnews

Topological defects in the fabric of space and time

A cosmic string is a very long (possibly as long as the diameter of the visible universe), very thin (less than the width of a proton) high-density object formed during the early moments of the big bang. (Credit: Stae Trek,  Paramount Pictures)
A cosmic string is a very long (possibly as long as the diameter of the visible universe), very thin (less than the width of a proton) high-density object formed during the early moments of the big bang. (Credit: Stae Trek, Paramount Pictures)
via phys.org

The Moon and the Oh-My-God Particle

Close up artist rendition. Image of the Australian SKA LFAA (Low Frequency Aperture Array) instrument. These dipole antenna which will number in their hundreds of thousands will survey the radio sky in frequencies as low at 50Mhz (Credit: SKA Organisation)
Close up artist rendition. Image of the Australian SKA LFAA (Low Frequency Aperture Array) instrument. These dipole antenna which will number in their hundreds of thousands will survey the radio sky in frequencies as low at 50Mhz (Credit: SKA Organisation)
via popularmechanics

On the front lines of the Higgs boson search

Prof. Butterworth, leading physicist on the ATLAS experiment at CERN and head of physics and astronomy at University College London, said the two colliding proton beams at CERN were the highest energy particle beams ever used in a laboratory. In order for the high momentum beams to be bent into a circle, its curvature had to be gentle enough for superconducting magnets to be able to control the beams. (Credit: hep.ucl.ac.uk/~jmb/publications)
Prof. Butterworth, leading physicist on the ATLAS experiment at CERN and head of physics and astronomy at University College London, said the two colliding proton beams at CERN were the highest energy particle beams ever used in a laboratory. (Credit: hep.ucl.ac.uk/~jmb/publications)
via phys.org

Peering backward to the big bang with the CTC and COSMOS

(NASA, Shellard,)
Recent analysis of CMB observations confirm predictions that a period of enormously fast exponential expansion, which cosmologists call inflation, occurred in the early universe. During inflation, very small changes, or quantum fluctuations, were imprinted into the fabric of space-time. (NASA, Shellard,)
via hpcwire

Answers to questions posed by cosmology to philosophy

 the philosophy of cosmology. He commented that the field is not well formulated yet, and proposed that one way to build a sound foundation for the field would be to identify the key questions worthy of its attention. Carroll nominated 10 such questions. Credit: Carroll)
Sean Caroll purposes 10 questions regarding the ‘not well formulated’ Philosophy of Cosmology. (Credit: Carroll)
via sciencenews

Getting sharp images from dull detectors

Coherent light passes through a pair of slits (top center).  The two resulting concentric trains of waves will interfere, resulting in a fixed pattern when measured by a detector (top right).  Non-coherent thermal light passes through slits and meets with a beam splitter (green plane), which reflects half the waves toward one detector and the other half toward a second detector (lower left).  Each of the detectors records a temporary interference pattern (lower right).  (Credit: JQI/Kelley )
Coherent light passes through a pair of slits (top center). The two resulting concentric trains of waves will interfere, resulting in a fixed pattern when measured by a detector (top right). Non-coherent thermal light passes through slits and meets with a beam splitter (green plane), which reflects half the waves toward one detector and the other half toward a second detector (lower left). Each of the detectors records a temporary interference pattern (lower right). (Credit: JQI/Kelley )
via umd

NASA: More spacewalks for ISS crew

via floridatoday

This Week’s Sky at a Glance, October 10 – 18

The waning Moon and Orion tip to the southwest as dawn brightens. (The Moon in these scenes is always shown three times its actual apparent size.. (Credit: Sky and Telescope)
The waning Moon and Orion tip to the southwest as dawn brightens. (The Moon in these scenes is always shown three times its actual apparent size.. (Credit: Sky and Telescope)
via skyandtelescope