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| Issue 4, 2024 |
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Extracts from the Internet | ||
Having evidence for the Higgs boson?1 November 2000Higgs bosons H are quanta of a scalar field which was introduced by P Higgs in 1964 to secure the renormalization property of the weak interaction in elementary particle physics. The experimental proof of the existence of H is one of the challenges facing high- energy physics. Now the ALEPH experiment conducted at the LEP accelerator at CERN in Geneva, Italy, has provided indirect evidence for the presence of H in reaction products. The search for H was done by studying four-jet events resulting from simultaneous decays of H and Z bosons, with two jets of particles being produced in either. For three of such events, the observed signal was found to be above the background by an amount which indicated H with mass of 114 GeV to be involved. However, because neither this result is statistically significant enough nor alternative explanations can be excluded, a definitive conclusion about the detection of H is not possible, and a decision was therefore made to continue with the ALEPH experiment. Source: http://press.web.cern.ch/ The Lamb shift1 November 2000According to quantum theory, vacuum is a polarizable medium: an electric charge in vacuum is surrounded by a cloud of virtual pairs which partially screen the charge. An electron approaching the atomic nucleus penetrates this cloud, which increases the effective nucleus-electron interaction - an experimentally observable effect underlying the so-called Lamb shift of the atomic energy levels. For the hydrogen atom, the Lamb shift has been measured to 0.01% and is found to agree well with theory. An electromagnetic interaction even stronger than that seen in the hydrogen atom takes place between the electrons and nuclei of heavy atoms. Researchers at the GSI Laboratory in Darmstadt, Germany, passed a beam of uranium-92 atoms through a foil with the result that the atoms were stripped of all but one of their electrons and thus turned into 91+ ions. In such ions, an electric field as high as 1016V cm-1 operates between the nucleus and the remaining electron. The Lamb shift in such ions was measured to be 468(±13) eV, in agreement with quantum electrodynamics predictions. The team hopes, an accuracy of 1 eV will soon be achieved. Source: http://prl.aps.org Bremsstrahlung photons1 November 2000When high-energy, heavy atomic nuclei collide head-on, in addition to their fission products such as neutrons and lighter nuclei, many other particles are produced. Some of these decay by emitting gamma photons, and these photons were detected in many experiments. The cloud of particles that forms around the location of a collision has properties very similar to those of hot plasma, and this latter is known to emit bremsstrahlung radiation. The first detection of this additional radiation has now been accomplished at CERN in collisions between lead nuclei, and based on the characteristics of this radiation, some theorists believe quark gluon plasma might have been produced in such collisions. Source: Physics News Update, Number 505 Melting of atomic clusters1 November 2000The traditional view is that a small solid particle has a lower melting point than a large one: in the former, relatively more atoms are close to the surface and so have fewer neighbour atoms to interact with - hence a lower binding energy per unit mass of the particle. However, A A Shvartsburg and M F Jarrold found the reverse to occur in their experiments on the melting of Si and Ge clusters as small as 15-30 atoms. They studied the motion of cigar-shaped clusters through a drift chamber filled with gaseous helium, and their idea was that when assuming a spherical shape upon melting, such clusters would experience more elastic resistance to their motion, and this would affect the amount of time they take to traverse the chamber. As it was, however, the clusters did not melt up to temperatures 50 K above the melting point of the bulk material. The theoretical explanation for this effect is still lacking. Source: Phys.Rev.Lett. 85 2530 (2000) Optical interferometer1 November 2000Cepheids are a special class of variable stars which, due to the stable nature of their brightness-pulsation period dependence, form convenient `standard candles' for distance determination purposes. Knowing distances to and the redshifts of Cepheid- containing galaxies makes it possible to determine the expansion rate and age of the Universe, but to do this it is necessary first to calibrate the brightness of the Cepheids, for which purpose distances to the closest of them must be very accurately measured. Because the physical diameter of the Cepheids is known from other data, the measurements of the distance reduces to measuring the Cepheid's angular diameter, which is about 0.001 arcseconds for even the closest Cepheids. However, even the resolving power of the Hubble telescope does not exceed 0.1 arcs, let alone ground-based telescopes subject to the degrading effect of the atmosphere. This problem can be overcome by pooling observations from several ground-based telescopes united into one optical interferometer. Attempts at such a system date back to the 1920s, but only recently, with advances in computer and optical technologies, has a real progress been made in this area. The optical interferometer constructed at Palomar Observatory in California, US, has a resolution of 0.001 arcs, equivalent to a single telescope with a mirror 110 m in diameter. The distance to one of the Cepheids has already been found with high accuracy using the new interferometer, and this will enable a cosmic distance scale and the age of the Universe to be determined. Source: Nature 407 485 (2000) |
The Extracts from the Internet is a section of Uspekhi Fizicheskih Nauk (Physics Uspekhi) — the monthly rewiew journal of the current state of the most topical problems in physics and in associated fields. The presented News is devoted to the fundamental discoveries of physics and astrophysics. Permanent editor is Yu.N. Eroshenko. It is compiled from a multitude of Internet sources. | |
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