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INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS: 9th Conference CIPAN2006 Date: 30 May-3June 2006 Location: Rio Grande, Puerto Rico (USA) ISBN: 978-0-7354-0368-0 Editor(s): Tony M. Liss

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Parity‐Violating Electron Scattering: New Results and Future Prospects

Krishna S. Kumar

AIP Conf. Proc. 870, pp. 1-9; doi:http://dx.doi.org/10.1063/1.2402591 (9 pages)

Online Publication Date: 28 November 2006

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We discuss the status and prospects of an experimental program of parity‐violating asymmetry measurements in the scattering of longitudinally polarized electrons off unpolarized fixed targets. One thrust is the measurements of nucleon neutral weak form factors at intermediate four‐momentum transfer (0.1 < Q2 < 1) (GeV/c)2 which provide information about the role of virtual strange quarks on the charge and current distributions inside nucleons. A new topic is the elastic neutral weak amplitude from scattering off a heavy spinless nucleus, which is sensitive to the presence of a neutron skin. Finally, we discuss the neutral current elastic amplitude at very low Q2, which allows precision measurements of the weak mixing angle at low energy and is thus sensitive to new physics at the TeV scale. The physics implications of recent results, potential measurements from experiments under construction as well as new ideas at future facilities are discussed. © 2006 American Institute of Physics
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11.30.Er Charge conjugation, parity, time reversal, and other discrete symmetries
13.60.-r Photon and charged-lepton interactions with hadrons
12.15.Mm Neutral currents

Beauty in the Standard Model and Beyond

Gabriella Sciolla

AIP Conf. Proc. 870, pp. 10-16; doi:http://dx.doi.org/10.1063/1.2402592 (7 pages)

Online Publication Date: 28 November 2006

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The study of CP violation in the B system allows us to perform quantitative tests of the CP symmetry in the Standard Model. Many precise measurements of the sides and angles of the Unitarity Triangle used to test the theory are made possible by the abundant experimental data accumulated at the B factories and the Tevatron. I review the Standard Model description of CP violation and the key measurements which allow us to use CP violation studies as a probe for New Physics. © 2006 American Institute of Physics
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11.30.Er Charge conjugation, parity, time reversal, and other discrete symmetries
12.60.-i Models beyond the standard model

QCD and Matter at Extreme Conditions

Xin‐Nian Wang

AIP Conf. Proc. 870, pp. 17-24; doi:http://dx.doi.org/10.1063/1.2402593 (8 pages)

Online Publication Date: 28 November 2006

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Nuclear matter is predicted to undergo a phase transition and become a plasma of quarks and gluons (QGP) at high temperature and density. Recent experimental results from high‐energy heavy‐ion collisions at the Relativistic Heavy‐ion Collider (RHIC) indicate the production of a strongly interacting quark‐gluon matter with fluid‐like properties. I will discuss some expected features of QCD at high temperature and density, theoretical interpretations of experimental observations and challenges in unraveling some of the basic properties of dense matter in the strongly interacting regime. © 2006 American Institute of Physics
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25.75.Nq Quark deconfinement, quark-gluon plasma production, and phase transitions
24.85.+p Quarks, gluons, and QCD in nuclear reactions
21.65.-f Nuclear matter

New results from BLAST on the nucleon electromagnetic form factors

Haiyan Gao and BLAST Collaboration

AIP Conf. Proc. 870, pp. 25-32; doi:http://dx.doi.org/10.1063/1.2402594 (8 pages)

Online Publication Date: 28 November 2006

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Recently, a new experiment was carried out in the South Hall Ring at the MIT‐Bates Accelerator Laboratory. This experiment utilized a polarized electron beam, a pure hydrogen (deuterium) internal polarized gas target, and the symmetric Bates Large Acceptance Spectrometer Toroid (BLAST) detector. The proton electric to magnetic form factor ratio, math at Q2= 0.15 – 0.65 (GeV/c)2 has been determined from the experiment by measuring the spin‐dependent ep elastic scattering asymmetry in both sectors simultaneously. This is the first experiment to measure math using a polarized proton target, which is complementary to recoil polarimetry experiments. The neutron magnetic form factor GMn has been extracted from the measurement of the spin‐dependent asymmetry from the inclusive d⃗(e⃗,e) process in a similar Q2 with a vector polarized deuterium target, and the neutron electric form factor GEn has been extracted by measuring the spin‐dependent asymmetry from the coincidence d⃗(e⃗,e′n) process simultaneously. Preliminary results on the nucleon form factors from the BLAST experiment are presented. © 2006 American Institute of Physics
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13.40.Gp Electromagnetic form factors
14.20.Dh Protons and neutrons
29.25.Bx Electron sources
29.25.Pj Polarized and other targets
29.30.Aj Charged-particle spectrometers: electric and magnetic

Nuclear Astrophysics

W. C. Haxton

AIP Conf. Proc. 870, pp. 33-43; doi:http://dx.doi.org/10.1063/1.2402595 (11 pages)

Online Publication Date: 28 November 2006

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I review progress that has been made in nuclear astrophysics over the past few years and summarize some of the questions that remain. Topics selected include solar neutrinos, supernovae (the explosion and associated nucleosynthesis), laboratory astrophysics, and neutron star structure. © 2006 American Institute of Physics
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26.65.+t Solar neutrinos
26.50.+x Nuclear physics aspects of novae, supernovae, and other explosive environments
26.30.-k Nucleosynthesis in novae, supernovae, and other explosive environments
97.60.Jd Neutron stars

Precision Studies of Dark Energy with LSST

J. Anthony Tyson and LSST Collaboration

AIP Conf. Proc. 870, pp. 44-52; doi:http://dx.doi.org/10.1063/1.2402596 (9 pages) | Cited 3 times

Online Publication Date: 28 November 2006

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Starting around 2013, data from the Large Synoptic Survey Telescope (LSST) will be analyzed for a wide range of phenomena. By separately tracing the development of mass structure and rate of expansion of the universe, these data will address the physics of dark matter and dark energy, the possible existence of modified gravity on large scales, large extra dimensions, the neutrino mass, and possible self interaction of dark matter particles. © 2006 American Institute of Physics
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95.36.+x Dark energy
95.35.+d Dark matter (stellar, interstellar, galactic, and cosmological)
14.60.Pq Neutrino mass and mixing

The Renaissance of Charm Physics

Roy A. Briere

AIP Conf. Proc. 870, pp. 53-62; doi:http://dx.doi.org/10.1063/1.2402597 (10 pages)

Online Publication Date: 28 November 2006

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A review of charm physics is presented, with an emphasis on decays of open‐charm particles. An ongoing renaissance is in progress, with charm playing an important role in weak flavor physics. It is the unique venue among up‐like quarks to perform precision tests to complement K and B physics. Charm also proves to be a useful test‐bed for verifying theoretical methods, such as Lattice QCD, which are required to interpret precision B physics data. © 2006 American Institute of Physics
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13.20.Fc Decays of charmed mesons
13.25.Ft Decays of charmed mesons

Hadron Spectroscopy in 2006

Jonathan L. Rosner

AIP Conf. Proc. 870, pp. 63-83; doi:http://dx.doi.org/10.1063/1.2402598 (21 pages) | Cited 1 time

Online Publication Date: 28 November 2006

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New results on hadron spectra have been appearing in abundance in the past few years as a result of improved experimental techniques. These include information on states made of both light quarks (u, d, and s) and with one or more heavy quarks (c, b). The present review, dedicated to the memory of R, H. Dalitz, treats light‐quark states, glueballs, hybrids, charmed and beauty particles, charmonium, and bb̄ states. Some future directions are mentioned. © 2006 American Institute of Physics
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14.65.Bt Light quarks
12.39.Mk Glueball and nonstandard multi-quark/gluon states

Top, Higgs and Electroweak Physics

Paul L. Tipton

AIP Conf. Proc. 870, pp. 84-92; doi:http://dx.doi.org/10.1063/1.2402599 (9 pages)

Online Publication Date: 28 November 2006

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Hadron colliders are, and will continue to be, an excellent venue for testing the standard model of particle physics. We describe the status of top‐quark physics and the direct search for a standard model Higgs boson. We briefly describe the use of Tevatron and LEP data to indirectly infer the standard model Higgs mass through precision electroweak measurements. © 2006 American Institute of Physics
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14.65.Ha Top quarks
14.80.Bn Standard-model Higgs bosons

Deeply Virtual Compton Scattering and Nucleon Structure

M. Garçon

AIP Conf. Proc. 870, pp. 93-101; doi:http://dx.doi.org/10.1063/1.2402600 (9 pages) | Cited 1 time

Online Publication Date: 28 November 2006

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Deeply Virtual Compton Scattering (DVCS) is the tool of choice to study Generalized Parton Distributions (GPD) in the nucleon. After a general introduction to the subject, a review of experimental results from various facilities is given. Following the first encouraging results, new generation dedicated experiments now allow unprecedented precision and kinematical coverage. Several new results were presented during the conference, showing significant progress in this relatively new field. Prospects for future experiments are presented. The path for the experimental determination of GPDs appears now open. © 2006 American Institute of Physics
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13.60.Fz Elastic and Compton scattering
14.20.Dh Protons and neutrons

Selected Spin Physics Results From COMPASS, HERMES AND RHIC

Klaus Rith

AIP Conf. Proc. 870, pp. 102-111; doi:http://dx.doi.org/10.1063/1.2402601 (10 pages)

Online Publication Date: 28 November 2006

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This review summarizes recent experimental results in polarized lepton‐nucleon and proton‐proton scattering. © 2006 American Institute of Physics
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13.88.+e Polarization in interactions and scattering
13.60.-r Photon and charged-lepton interactions with hadrons
13.75.Cs Nucleon-nucleon interactions (including antinucleons, deuterons, etc.)

Supersymmetry without Naturalness: Detection Prospects and Sensitivities

James D. Wells

AIP Conf. Proc. 870, pp. 112-115; doi:http://dx.doi.org/10.1063/1.2402602 (4 pages)

Online Publication Date: 28 November 2006

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It is often stated that supersymmetry solves the hierarchy problem. However, if one tries to give a precise statement about what that means, controversy ensues. In this talk, I dismiss solving the hierarchy as a relevant goal for supersymmetry, and ask what remains. Some of the answers we find are that the light Higgs boson, dark matter and gauge coupling unification all remain attractive features of supersymmetry. Several implications for future experiment are presented, which constitute the detection prospects and sensitivities of supersymmetry without naturalness as a primary consideration. © 2006 American Institute of Physics
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11.30.Pb Supersymmetry
12.60.Jv Supersymmetric models
14.80.Ly Supersymmetric partners of known particles

Measurement of the Bs0 Oscillation Frequency

Matthew Jones and CDF collaboration

AIP Conf. Proc. 870, pp. 116-123; doi:http://dx.doi.org/10.1063/1.2402603 (8 pages) | Cited 4 times

Online Publication Date: 28 November 2006

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The precise determination of the Bs0/maths0 oscillation frequency provides a powerful constraint on parameters in the CKM matrix. While previous experiments have only had sufficient sensitivity to set limits, the CDF and DØ experiments have recently presented independent analyses in which the results are interpreted as the direct observation of Bs0 oscillations. The recent results from CDF and DØ are presented, emphasizing key aspects of the CDF analysis that have significantly enhanced its sensitivity to oscillations in the existing data sample from pp̄ collisions recorded at the Fermilab Tevatron. © 2006 American Institute of Physics
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14.40.Nd Bottom mesons (|B|>0)
12.15.Hh Determination of Cabibbo-Kobayashi & Maskawa (CKM) matrix elements

Neutrinoless double beta decay

Petr Vogel

AIP Conf. Proc. 870, pp. 124-131; doi:http://dx.doi.org/10.1063/1.2402604 (8 pages) | Cited 1 time

Online Publication Date: 28 November 2006

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Present status of the search for 0νββ decay and of the related theoretical questions is reviewed. The mechanism of the decay, and how to recognize it, is discussed first, followed by the relation of the effective neutrino Majorana mass and the oscillation parameters, and the problems of nuclear matrix elements. The planned ∼ 100 kg experiments are briefly described. © 2006 American Institute of Physics
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23.40.Hc Relation with nuclear matrix elements and nuclear structure
14.60.Pq Neutrino mass and mixing

Neutron Lifetime Measurements

J. S. Nico

AIP Conf. Proc. 870, pp. 132-138; doi:http://dx.doi.org/10.1063/1.2402605 (7 pages) | Cited 1 time

Online Publication Date: 28 November 2006

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Precision measurements of neutron beta decay address basic questions in nuclear and particle physics, astrophysics, and cosmology. As the simplest semileptonic decay system, the free neutron plays an important role in understanding the physics of the weak interaction, and improving the precision of the neutron lifetime is fundamental to testing the validity of the theory. The neutron lifetime also directly affects the relative abundance of primordial helium in big bang nucleosynthesis. There are two distinct strategies for measuring the lifetime. Experiments using cold neutrons measure the absolute specific activity of a beam of neutrons by counting decay protons; experiments using confined, ultracold neutrons determine the lifetime by counting neutrons that remain after some elapsed time. The status of the recent lifetime measurements using both of these techniques is discussed. © 2006 American Institute of Physics
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23.40.Bw Weak-interaction and lepton (including neutrino) aspects
26.35.+c Big Bang nucleosynthesis

Fundamental Symmetries and CKM — summary of the parallel sessions

T. Chupp, A. El‐Khadra, and S. Prell

AIP Conf. Proc. 870, pp. 139-147; doi:http://dx.doi.org/10.1063/1.2402606 (9 pages)

Online Publication Date: 28 November 2006

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Recent progress in the tests of fundamental symmetries and the CKM structure of the violation of CP symmetry in the quark mixing sector, as presented in the relevant parallel sessions of this conference, is summarized. © 2006 American Institute of Physics
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12.15.Hh Determination of Cabibbo-Kobayashi & Maskawa (CKM) matrix elements
11.30.Er Charge conjugation, parity, time reversal, and other discrete symmetries

CIPANP 2006 Low Energy Hadron Physics Summary

Reinhard A. Schumacher

AIP Conf. Proc. 870, pp. 148-151; doi:http://dx.doi.org/10.1063/1.2402607 (4 pages)

Online Publication Date: 28 November 2006

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Recent results in the areas of hypernuclear physics, exotic atoms, photo‐ and electro‐production of light mesons and baryons, and medium modifications of meson properties were presented at this conference. Facility highlights presentations were given for five laboratories: the ELSA complex at Bonn, the LEPS facility at SPring‐8, the CLAS facility at Jefferson Lab, the MAMI complex at Mainz, and the COSY complex at Jülich. These talks collectively showed remarkably active programs at all these laboratories, as well as at BNL, KEK, PSI, and Frascati. No “brand new” results were reported at this conference. © 2006 American Institute of Physics
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13.75.-n Hadron-induced low- and intermediate-energy reactions and scattering (energy ≤ 10 GeV)
21.80.+a Hypernuclei
13.60.Le Meson production
13.60.Rj Baryon production

Nuclear Structure at the CIPANP Conference — Summary

John Arrington, Ed Kinney, and Feng Yuan

AIP Conf. Proc. 870, pp. 152-159; doi:http://dx.doi.org/10.1063/1.2402608 (8 pages)

Online Publication Date: 28 November 2006

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We present a brief summary of the nuclear structure parallel sessions. © 2006 American Institute of Physics
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21.60.-n Nuclear structure models and methods

Summary of Quark Matter and Heavy Ion Parallel Session, CIPANP06

J. C. Dunlop

AIP Conf. Proc. 870, pp. 160-167; doi:http://dx.doi.org/10.1063/1.2402609 (8 pages)

Online Publication Date: 28 November 2006

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This is clearly an exciting time to be working in the field of relativistic heavy ions, due to RHIC, a running facility dedicated to the study of quark matter at high energy density. Collective phenomena in collisions of ions at high energy indicate that the medium behaves as a liquid with extremely low viscosity, as an essentially perfect liquid. Talks during the session addressed progress in testing this hypothesis and measuring the viscosity. New progress in constituent quark number scaling at intermediate pT, which may identify the relevant degrees of freedom at hadronization, was reported. There has also been significant progress towards full jet emission tomography of the collision zone, using the physical phenomenon of jet quenching, discovered at RHIC. Finally, possible thermometers of the collision zone have been identified and promising measurements towards their use have been made. © 2006 American Institute of Physics
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25.75.Dw Particle and resonance production
21.65.-f Nuclear matter
24.85.+p Quarks, gluons, and QCD in nuclear reactions

Surveying The TeV Sky With Milagro

G. P. Walker and Milagro Collaboration

AIP Conf. Proc. 870, pp. 171-173; doi:http://dx.doi.org/10.1063/1.2402610 (3 pages)

Online Publication Date: 28 November 2006

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A wide field of view, high duty factor TeV gamma‐ray observatory is essential for studying TeV astrophysical sources, because most of these sources are either highly variable or are extended. Milagro is such a TeV detector and has performed the deepest survey of the Northern Hemisphere sky. In addition to detecting the Crab Nebula and Mrk 421, which are known TeV sources, Milagro has made the first detection of diffuse TeV emission from the Galactic plane. The Milagro data has been searched for unknown point sources and extended sources. A new extended TeV source is seen and is coincident with an EGRET unidentified source. Based on the success of Milagro, a second generation water Cherenkov gamma‐ray observatory is planned which will give an increase in sensitivity of more than an order of magnitude. © 2006 American Institute of Physics
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95.55.Ka X- and γ-ray telescopes and instrumentation
95.85.Pw γ-ray
29.40.Ka Cherenkov detectors

Observing nuclear gamma‐ray lines from the Galaxy with SPI/INTEGRAL

Karsten Kretschmer

AIP Conf. Proc. 870, pp. 174-177; doi:http://dx.doi.org/10.1063/1.2402611 (4 pages)

Online Publication Date: 28 November 2006

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Gamma rays in the MeV energy range offer a unique opportunity to study the hot interstellar medium and its dynamics by way of measuring gamma‐ray lines emitted during the decay of radioactive isotopes. Current instrumentation like the spectrometer SPI on board of the INTEGRAL satellite observatory is able to measure the width and position of MeV lines like the 1 808.63 keV line from the decay of 26Al spatially resolved to a precision corresponding to several tens of km s−1 This accuracy allows to deduce the location of the emitting radioactive material within the Galaxy and thereby to determine the total amount of 26Al present and from that the Galactic star formation rate. © 2006 American Institute of Physics
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95.55.Ka X- and γ-ray telescopes and instrumentation
98.70.Rz γ-ray sources; γ-ray bursts
95.85.Pw γ-ray

Upward Showering Muons in Super‐Kamiokande

Shantanu Desai and Super‐Kamiokande Collaboration

AIP Conf. Proc. 870, pp. 178-180; doi:http://dx.doi.org/10.1063/1.2402612 (3 pages)

Online Publication Date: 28 November 2006

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A small subset of neutrino‐induced upward going muons in the Super‐Kamiokande detector consists of high energy muons that undergo radiative energy losses through bremsstrahlung, e+e− pair production and photo‐nuclear interactions. The mean energy of the parent neutrinos of these showering upward muons is approximately 1 TeV, allowing the selection of a high energy sample of neutrinos. We present physics(mainly oscillation analysis) as well as astrophysical results with the upward showering muon dataset using about 1680 days of Super‐K‐I data. © 2006 American Institute of Physics
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95.55.Vj Neutrino, muon, pion, and other elementary particle detectors; cosmic ray detectors
13.15.+g Neutrino interactions
13.66.-a Lepton-lepton interactions
25.20.-x Photonuclear reactions

First cosmic‐ray grapes ripen in Argentina: Results and progress of the Pierre Auger Observatory

Michael Prouza and Pierre Auger Collaboration

AIP Conf. Proc. 870, pp. 181-185; doi:http://dx.doi.org/10.1063/1.2402613 (5 pages)

Online Publication Date: 28 November 2006

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The Pierre Auger Observatory is the largest detector ever built for the study of ultra‐high energy cosmic rays. The construction of its southern site in Mendoza Province in Argentina is almost complete and the observatory has been acquiring scientific data for more than two years. The cumulative exposure achieved during this period is greater than the exposure of any forerunner experiment. Furthermore, the Pierre Auger Observatory uses the innovative hybrid technique which combines the advantages of fluorescence telescopes (precise and nearly model‐independent energy measurement) and the advantages of surface detector arrays (exact geometrical definition of exposure). A preliminary analysis of this initial data set will be presented, namely the spectrum and the results of anisotropy searches. © 2006 American Institute of Physics
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95.55.Vj Neutrino, muon, pion, and other elementary particle detectors; cosmic ray detectors
95.45.+i Observatories and site testing

Results and status of KASCADE‐Grande

H. Ulrich, W. D. Apel, A. F. Badea, K. Bekk, A. Bercuci, M. Bertaina, J. Blümer, H. Bozdog, I. M. Brancus, M. Brüggemann, P. Buchholz, A. Chiavassa, F. Cossavella, K. Daumiller, F. Di Pierro, et al.

AIP Conf. Proc. 870, pp. 186-189; doi:http://dx.doi.org/10.1063/1.2402614 (4 pages)

Online Publication Date: 28 November 2006

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The KASCADE‐Grande experiment measures extensive air showers induced by cosmic rays in the knee region (with energies between 0.5 PeV and 1 EeV). The principal task of the experiment is to measure precisely the energy and chemical composition of primary cosmic rays to clarify the origin of the knee. The data of the original KASCADE experiment have been used in a composition analysis, which shows the knee is caused by a steepening of the element spectra. The limitations to these conclusions due to the dependence on the high energy hadronic interaction models used in the simulations are also presented. © 2006 American Institute of Physics
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96.50.sd Extensive air showers
96.50.sb Composition, energy spectra and interactions

Ultra High Energy Cosmic Rays in the North: Measurement of UHE Cosmic Rays with the High Resolution Fly’s Eye (HiRes) Detector

J. N. Matthews and HiRes Collaboration

AIP Conf. Proc. 870, pp. 190-197; doi:http://dx.doi.org/10.1063/1.2402615 (8 pages)

Online Publication Date: 28 November 2006

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The High Resolution Fly’s Eye (HiRes) observatory has been collecting Ultra High Energy Cosmic Ray (UHECR) data since 1997. The experiment observes cosmic ray air showers via the air fluorescence technique and consists of two observatory sites separated by 12.6 km in the western Utah desert. The two stations can each measure the cosmic rays in monocular mode. In addition, the data from the two stations can also be combined to form a stereo measurement of the air showers. The experiment measures such properties as the energy spectrum, chemical composition, and p‐air cross‐section of these cosmic rays. It also searches for point sources and other anisotropy. The spectrum is measured above ∼3 × 1017 eV and shows significant structure including the “ankle” and a steep fall off which is consistent with the expectation of the GZK. threshold. The spectrum is inconsistent with a continuing spectrum at the 5σ level. The composition is measured using the Xmax technique. It was found to be predominantly light and unchanging over the range from 1018 to 3 × 1019 eV. Finally, several different styles of searches for anisotropy in the data were performed. There are some tantalizing hints including potential correlation with BL Lac objects and the ‘AGASA triplet”, however these will need to be confirmed with an independent data set. © 2006 American Institute of Physics
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95.55.Vj Neutrino, muon, pion, and other elementary particle detectors; cosmic ray detectors
96.50.sd Extensive air showers
96.50.sb Composition, energy spectra and interactions
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