Physics

Galaxy Song

Intro:
WHENEVER LIFE GETS YOU DOWN, MRS. BROWN, AND THINGS SEEM HARD OR TOUGH, AND PEOPLE ARE STUPID, OBNOXIOUS OR DAFT AND YOU FEEL THAT YOU'VE HAD QUITE ENOUGH...

Just remember that you're standing on a planet that's evolving.
And revolving at 900 miles an hour,
That's orbiting at 19 miles a second, so it's reckoned,
A sun that is the source of all our power.
The sun and you and me and all the stars that we can see,
Are moving at a million miles a day
In an outer spiral arm, at 40,000 miles an hour,
Of the Galaxy we call the Milky Way.

Our Galaxy itself contains 100 billion stars
It's 100,000 light years side to side,
It bulges in the middle, 16,000 light years thick
But out by us it's just 3,000 light years wide
We're 30,000 light years from the galactic central point,
We go round every 200 million years
And our galaxy is only one of millions of billions
In this amazing and expanding Universe.

The Universe itself keeps on expanding and expanding
In all of the directions it can whizz
As fast as it can go, at the speed of light you know,
12 million miles a minute, and that's the fastest speed there is.
So remember when you're feeling very small and insecure
How amazingly unlikely is your birth
And pray that there's intelligent life somewhere up in space
Because there's bugger all down here on Earth.

Composer: Eric Idle/John de Prez
Author: Eric Idle
Performed by: Monty Python's Flying Circus

MY WRITINGS

A Measurement of

in Fermilab E791

(.pdf - "diamonds" are arrows to the right! Gotta love pdf!)

High Energy Physics Group, Department of Physics, Kansas State University, Manhattan, Kansas 66506

The above product of the ratios of the branching fractions in Fermilab E791 is measured. A gaussian curve is fit to the invariant mass plots of K+ K- p ± to identify the Ds ±. Invariant mass plots of K+ K- are fit with a Breit-Wigner curve to identify the j and the WA76 parameterization of f0(980) is used to identify the f0(980). In order to determine the detector efficiency for the decay f0(980) -> K+ K-, the Monte Carlo mass generation routine, ULMASS.F of Jetset 7.4, is modified to include the WA76 parameterization to generate the appropriate line-shape for the decay f0(980).

In-beam Tests of a Ring Imaging Cerenkov Detector With a Multianode Photomultiplier Readout

Authors: R. Debbe, S. Gushue, B. Moskowitz, J. Norris, J. Olness, F. Videbaek

Brookhaven National Lab, Upton NY 11973

Nuclear Instruments and Methods in Physics Research A 362 (1995) 253-260: text (.ps), figures (.pdf).

A ring-imaging Cherenkov counter read out by a 100-channel PMT of active area 10cmx10cm was operated successfully in a test beam at the BNL AGS with several radiator gases, including the heavy fluorocarbon C4 F10. Ring radii were measured for electrons, muons, pions and kaons over the particle momentum range from 2 to 12 GeV/c, and a best resolution of sigma_r/r=2.3% was obtained.

Velocity dependence of ionization and fragmentation of methane caused by fast-proton impact

Authors: I Ben-Itzhak, K. D. Carnes, D. T. Johnson, P. J. Norris, O. L. Weaver

James R Macdonald Laboratory, Department of Physics, Kansas State University, Manhattan, Kansas 66506

Physical Review A, Vol 49, Num 2, February 1994, pg 881-888 (.pdf)

The velocity dependence of methane ionization and fragmentation have been studied using a coincidence time-of-flight technique. The relative yields of single-ion, ion-pair, and ion-triple channels have been determined for 1 - to 12-MeV proton impact. The multiple-ionization cross sections have been determined and are in accord with our model semiclassical Coulomb approximation calculations. The single-ion channels resulting from the breakup of CH4+* were found to be independent of the collision velocity. Good agreement with previous proton-impact measurements and with electron-impact measurements is observed. On the other hand, the ion-pair breakup channels of CH4++* show surprising dependence on the collision velocity. The ion-pair data are in reasonable agreement with fast-electron-impact measurements at 10 keV while differing significantly with a lower, 1-KeV, electron-impact measurement.

Direct Determination of recoil ion detection efficiency for coincidence time-of-flight of molecular ragmentation

Authors: I. Ben-Itzhak, K. D. Carnes, S. G. Ginther, D. T. Johnson, P. J. Norris, and O. L. Weaver

James R Macdonald Laboratory, Department of Physics, Kansas State University, Manhattan, Kansas 66506

Nuclear Instruments and Methods in Physics Research B79(1993) 138-141.

Molecular fragmentation of diatomic and small polyatomic molecules by fast ion impact has been studied. The evaluation of the cross sections of the different fragmentation channels depends strongly on the recoil ion detection efficiency, er (single ions proportional to er, and ion pairs to er2, etc.). A method is suggested for the direct determination of this detection efficiency. This method is based on the fact that fast H2 + CH4 collisions produce C2+ fragments only in coincidence with H+ and H+2 fragments in which the H+m of the H+2 + C2+ ion pair was not detected and thus is proportional to 1 - er. Methane fragmentation caused by 1 MeV proton impact is used to evaluate directly the recoil ion detection effeciency and to demonstrate the method of deriving the cross sections of all breakup channels.

Fragmentation of CH4 caused by fast-proton impact

Authors: I. Ben-Itzhak, K. D. Carnes, S. G. Ginther, D. T. Johnson, P. J. Norris, and O. L. Weaver

James R Macdonald Laboratory, Department of Physics, Kansas State University, Manhattan, Kansas 66506

Physical Review A, Vol 47, Num 5, May 1993, pg 3784-3757 (.pdf)

The cross sections of the different breakup channels of CH4, produced by 4-MeV proton impact, have been measured using the coincidence time-of-flight technique. The relative abundances of the different breakup channels were evaluated for collisions in which the molecule broke into two charged fragments as well as for collisions where only a single charged molecular ion or fragment was produced. These relative abundances are compared to the ones measured for photodissociation, and for electron and proton impact. Only the CH4+ ion survives long enough to be detected as a molecular ion, while the doubly charged CH42+ ion dissociates rapidly. The most probable final product of the fragmentation of doubly charged methane as formed by fast-proton impact is H+ + CH2++H. The abundance of Hm+ + CHn+ (m+n <= 4) ion pairs decreases rapidly with increasing m, as suggested by Siegbahn [Chem. Phys. 66, 443(1982)]. The momentum of neutral fragments, in channels where they are produced, is small in comparison with the momentum of the charged fragments so that two-body breakup holds approximately. The deviation from two-body breakup increases with increasing number of neutral hydrogen atoms produced. The sensitivity of the experimental method enabled us to extend the study of the fragmentation pattern of CH42+ to include small breakup channels such as CH42+ --> H3+ + CH+. Furthermore, some breakup channels of the triply charged CH43+ have been detected as triple coincidences.

If you have any comments (praise or criticism), please send email to:

jnorris@wamego.net

Copyright: James Norris

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Last modified on R17 Feb 2000