R1.
R.
Conti, Experimental Tests of QED in Positronium:
Recent Advances
R2.
K.
Jungmann, Precision Spectroscopy of the Muonium
Atom - Recent Results and Future Possibilities
T1.
G.
S. Adkins, R. N. Fell, and J. Sapirstein, Order
Corrections to the Decay Rate of Orthopositronium
T2.
M. Grosse Perdekamp, V. W. Hughes, D. Kawall, W. Liu, K. Jungmann
and G. zu Putlitz, Test of CPT and Lorentz Invariance
from Muonium Spectroscopy
P20.
A. Czarnecki, K. Melnikov and A. Yelkhovsky, Recent
Results in Positronium Theory
P21.
R.
Ley, Positronium: Theory versus Experiment
P22.
I. Meshkov,
A. Sidorin, A. Smirnov, and E. Syresin, Generation
and Experiments with Positronium in-Flight
P23.
R.S. Vallery, R.S. Conti, J.J. Engbrecht, D.W. Gidley, and M. Skalsey,
Impact
of Positronium Thermalization on High-Precision Experiments
P24.
V.
Yakhontov, K. Jungmann and V. Meyer, Highly
Accurate Theoretical Simulation of the Resonant 2- and 3-Photon Ionization
Processes with Simplest Atoms |
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Experimental
Tests of QED in Positronium: Recent Advances
R.S. Conti
The University of Michigan, Randall Laboratory
of Physics, Ann Arbor, MI 48109-1120, USA
In the past decade several new results have been
published that impact the testing of QED in positronium. These are comparison
between theory and experiment for the decay rates of ortho- (13S1)
and para-positronium (11S0) and for the energy splittings between the hyperfine
states (13S1-11S0), the n
= 2 fine structure (23S1-23PJ,
J = 0, 1, 2; 23S1-21P1), and
the two-photon transition between the n = 1 and n = 2 levels (13S1-23S1).
In the early part of the decade all the experimental values for these quantities
were known to higher precision than the corresponding theoretical values.
In the last few years this trend has been almost completely reversed by
theoretical advances. In the early part of the decade the only clear discrepancy
between theory and experiment was in the decay rate of ortho-positronium.
That discrepancy has persisted, with additional controversy introduced
by further experimental and theoretical results. In light of recent theoretical
calculations, the hyperfine splitting too, shows hints of a discrepancy.
The thermalization of positronium in gases has
systematic effects in some of the measurements of both the ortho-positronium
decay rate and the hyperfine splitting. These systematics will be discussed
in detail in a separate poster. Future prospects for improvements in each
of these measurements will be discussed.
Work of the Michigan positron group is supported
by NSF grant PHY 97-31861 and the University of Michigan. |
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Precision
Spectroscopy of the Muonium Atom - Recent Results and Future Possibilities
Klaus P. Jungmann
Physikalisches Institut, Universität Heidelberg,
D-69120 Heidelberg, Germany
The muonium atom consits of two leptons from two
different generations, a positve muon and an electron1,2. The
absence of any known internal structure for these particles allows to calculate
level energies to very high accuracy within the framework of bound state
Quantum Electrodynamics (QED). In th case of the hyperfine structure the
agreement between theory and experiment is substantially better than for
natural hydrogen where the yet not well known structure of
the proton and dynamics of its charge carrying constituents prevent more
stringent conclusions.
In two recent experiments the hyperfine structure
interval and the Zeeman effect in the ground state3 and the
1s-2s energy splitting4 were measured with microwave respectively
Doppler-free two-photon laser spectroscopy. The results were in good agreement
with theoretical predictions which include the dominant QED part and contributions
from strong and weak interactions. Most accurate values for the muon
magnetic moment, the muon mass, the muon electron charge ratio and a precise
number for fine structure constant were extracted from the measurements2,3,4.
Muonium has proven to be an ideal system for testing
QED and fundamental symmetries in physics5 as well as
for providing accurate values of fundamental constants in the past. It
could continue to do so in the future. Improvements in accuracy can be
expected with higher numbers of muonium atoms as they are expected to be
available from future high flux muon sources such as the PRISM facility
of the Japanese Hadron Facility, the Oak Ridge spallation neutron
source or the front end of a muon collider6,7. An additional
boost in accuracy can then be gained from new techniques like using cw
lasers in the case of the 1s-2s experiment5.
References:
-
V.W. Hughes and G. zu Putlitz, in: Quantum Electrodynamics,
ed. T. Kinoshita, World Scientific, p. 822 (1990).
-
K. Jungmann, in: Muon Science, eds. S.L. Lee, S.H.
Kilcoyne and R. Cywinsky, Inst. of Physics Publ., p. 405 (1999).
-
W. Liu et al., Phys. Rev. Lett. 82, 711 (1999).
-
V. Meyer et al., Phys. Rev. Lett. 84, 1136
(2000).
-
L. Willmann et al., Phys. Rev. Lett. 82, 49
(1999).
-
K. Jungmann, in: Proceedings of the HISMUS99 Workshop,
ed. Y. Kuno, World Scientific, in print (2000).
-
M.G. Boshier et al., Comm. At. Mol. Phys. 33,
17 (1996).
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Order
Corrections to the Decay Rate of Orthopositronium
G.S .Adkins1,
R. Fell2, and J. Sapirstein3
1 Department of Physics and Astroomy,
Franklin & Marshall Colege, P.O. Box 3003, Lancaster, PA, 17604, USA,
Email: g_adkins@acad.fandm.edu
2 Brandeis University, Waltham,
MA, 01742 USA
3 Department of Physics, University
of Nore Dame, Nore Dame, IN, 46556 USA
The discrepancy between theory and experiment
for the decay rate of orthopositronium has long been one of the outstanding
problems in precision QED. The calculated decay rate is [1-3]
,
where the lowest order contributionis
[4]. The one-loop correction is known to be A = -10.286606(10) [5]. The
result of the present calculationis a value for the two-loop correction
B.
Our calculation was done in the context of Nonrelativistic
Quantum Electrodynamics (also knownas NRQED) [6] following the approach
outlined by Labelle, Lepage, and Magnea [7].This method allows the highenergy
part of the calculation to be treatedas an onshell scattering process.
The highenergy calculationis part of a "matching" procedure in which a
set of nonrelativistic interaction operators is defined. These operators
are used to work out the boundstate aspects of the problem. Our calculation
of the highenergy process followed by a boundstate calculation using
the effective interaction operators allowed us to complete the determination
of B [8].
Acknowledgments. The work of GA was partially
supported by NSF grants PHY9711991 and PHY9722074, and that of JS by
PHY9870017. Useful conversations with P. Labelle, G.P. Lepage, and R.
Hill are acknowledged.
References:
-
W.E. Caswell, G.P. Lepage, and J. Sapirstein, Phys.
Rev. Lett. 38, 488 (1977).
-
W.E. Caswell and G.P. Lepage, Phys. Rev. A 20,
36 (1979).
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S.G. Karshenboim, Zh. Eksp. Teor. Fiz. 103,
1105 (1993) [JETP 76, 541 (1993)].
-
A. Ore and J.L. Powell, Phys. Rev. 75, 1696
(1949).
-
G.S. Adkins, Phys. Rev. Lett. 76, 4903 (1996).
-
W.E. Caswell and G.P. Lepage, Phys. Lett. 167B
, 437(1986).
-
P. Labelle, G.P. Lepage, and U. Magnea, Phys. Rev.
Lett. 72, 2006 (1994).
-
G.S. Adkins, R. Fell, and J. Sapirstein, hepph/0003028.
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Test
of CPT and Lorentz Invariance from Muonium Spectroscopy
M. Grosse Perdekamp,
V. W. Hughes, D. Kawall, and W. Liu,
Yale University
K. Jungmann and G.
zu Putlitz
University of Heidelberg
Following a suggestion of A. Kostelecký et al.
[1], we are evaluating a test of CPT and Lorentz invariance from the microwave
spectroscopy of muonium [2]. Precise measurements have been reported for
the transition frequencies
and
for ground state muonium in a magnetic field H of 1.7 T. These frequencies
depend on both the hyperfine interaction and Zeeman effect. Hamiltonian
terms beyond the standard model which violate CPT and Lorentz invariance
would contribute
and .
The nonstandard theory indicates that
and
should oscillate with the earth's sidereal frequency and indeed
and
would be anticorrelated.
We are analyzing our muonium data and expect to
report results at the Hydrogen II Conference.
References:
-
D. Calladay and V.A. Kostelecký, Phys. Rev. D 55,
6760 (1997) ; R. Bluhm, V.A. Kostelecký and C.D. Lane, CPT and Lorentz
Tests with Muons, submitted to Phys. Rev. Lett.
-
W. Liu et al., Phys. Rev. Lett 82, 711 (1999).
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Recent
Results in Positronium Theory
Andrzej Czarnecki1,
Kirill Melnikov2 and Alexander Yelkhovsky3
1 Physics Department, Brookhaven
National Laboratory, Upton, NY 11973, USA
2 Stanford Linear Accelerator Center,
Stanford University, Stanford, CA 94080, USA
3 Budker Institute for Nuclear
Physics, Novosibirsk, 630090, Russia
Positronium, an elementary atom which consists
of electron and positron, provides a unique laboratory to test the theory
of weakly bound states in QED. Because of the small value of the
electron mass, the uncertainties due to strong interactions are not important
at the current level of theoretical and experimental precision. This provides
a unique opportunity to confront high precision experiments that study
various properties of positronium with theoretical predictions.
Recently, we have applied dimensionally regularized
non-relativistic QED to positronium spectroscopy and the decay width of
parapositronium. An analytic expressions for
corrections to the ground state positronium hyperfine splitting [1] and
singlet energy level shifts [2] have been obtained. We have also derived
corrections to positronium energy levels [3]. For the most precisely measured
quantity, the positronium ground state hyperfine splitting, we obtain [2,3]
203392(1) MHz, which differs from experimental results by about three standard
deviations.
Another interesting quantity is the parapositronium
decay width into two photons. Since a rather precise measurement of the
parapositronium decay rate is available, the theoretical result becomes
of considerable interest. We obtain [4,5] 
which agrees very well with experimental result.
References:
-
A. Czarnecki, K. Melnikov and A. Yelkhovsky, Phys.
Rev. Lett. 82, 311 (1999).
-
A. Czarnecki, K. Melnikov and A. Yelkhovsky,
Phys. Rev. A 59, 4316 (1999).
-
K. Melnikov and A. Yelkhovsky, Phys. Lett. B 458,
143 (1999).
-
A. Czarnecki, K. Melnikov and A. Yelkhovsky, Phys.
Rev. Lett. 83, 1135 (1999).
-
A. Czarnecki, K. Melnikov and A. Yelkhovsky, Phys.
Rev. A 61, 052502 (2000).
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Positronium:
Theory versus Experiment
Richard Ley
Institute for Physics, University of Mainz,
D-55099 Mainz, Germany
Positronium (Ps) is the bound state of an electron
and its antiparticle the positron. Both components are structureless and
pointlike leptons, thus avoiding the difficulties encountered with the
proton structure in hydrogen. The advantage, compared with muonium, is
the absence of an additional free parameter like the muon mass. Moreover
Ps is an eigenstate of the charge conjugation operator, which opens new
channels of real and virtual annihilation. For these reasons Ps is an ideal
test object for bound state QED. Ps is completely described by only two
parameters: the Rydberg constant Ry and the fine structure constant .
QCD effects and the weak interaction play no role at the present state
of accuracy.
The energy levels of Ps have been completely calculated
up to the order .
The theoretical uncertainty results only from uncalculated higher order
terms and is estimated to be 1 MHz for the ground state n = 1. The experimental
accuracy is comparable and there is moderate agreement with theory within
3 standard deviations. In the excited state n = 2 the intervals between
the P-levels can be calculated to an accuracy of 10 kHz. Here the experiments
need the full width of 3 standard deviations (3 × 1 MHz ) to come into
agreement with theory.
The annihilation rate of triplet Ps in the ground
state is completely calculated up to the order .
The contribution from higher orders is only estimated and introduces a
relative theoretical uncertainty of 2×10-4. The experimental situation
is controversial: a measurement at the University of Tokyo is in agreement
with theory, whereas the results from the University of Ann Arbor disagree
with theory by more than 4 standard deviations.
The annihilation rate of singlet Ps in the in
the ground state has been completely calculated up to the order .
The estimated higher order contributions introduce a relative theoretical
uncertainty of 1×10-4. The experiment has comparable accuracy and is in
good agreement with theory. |
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Generation
and Experiments with Positronium in-Flight
I. Meshkov, A. Sidorin,
A. Smirnov, and E. Syresin
Joint Institute for Nuclear Research, Dubna,
Russia
The project of Low Energy Particle Toroidal Accumulator
(LEPTA) [1], which is under construction in the JINR now, is dedicated
to the creation of small positron storage ring with electron cooling of
positrons circulating in the ring. The potential of this device is the
generation of intense streams of electron-positron bound states, known
as positronium, and - together with low energy antiprotons - for the synthesis
of antihydrogen atoms in copious numbers.
The focusing system with longitudinal magnetic
field and electron cooling of positrons are essential features of the LEPTA.
The single turn injection of positrons is performed by special kicker coil.
At the first stage of the LEPTA operation we plan to use a positron source
on the base of radioactive isotope 22Na. Nearest prototype of
the injection system is the positron trap of the ATHENA project. Special
septum coils and centrifugal drift of the electrons are used for superposition
and separation of the cooling electron beam and the circulating positron
one. The positronium is generated in collisions of positrons with free
electrons of the cooling electron beam that have velocities very close
to the positron ones. This permits obtaining a high positronium flux with
small angular and velocity spreads of the atoms and provides a significant
advantage for proposed arrangements of experiments, so-called positronium-in-flight
set-ups [2], as compared with traditional approaches in which positronium
is generated in targets. In particular, the precision in measuring positronium
parameters can be enhanced by several orders of magnitude. Moreover, some
experiments, that are unrealistic within traditional schemes, becomes feasible
with the proposed facility. The ring circumference is about 18 m, magnetic
field value is 400 G, positron energy is of the order of 10 keV. Expected
angular and relative energy spreads of positronium flux are 2×10-3
and (1 - 5)×10-4 correspondingly. At 109 positrons
circulating in the ring the flux value is about 104 atoms per
second.
Presently the design of the storage ring and the
elaboration of the technology of the ring elements manufacturing are completed.
The vacuum chamber of the ring was constructed and tested. Solenoid of
electron cooling system was constructed, tested and adjusted. Other general
elements of the magnetic system are under construction. In very beginning
of the LEPTA ring operation the following problems have to be experimentally
investigated: dynamics of circulating beam; measurements of the friction
force components due to electron cooling of positrons, investigation of
the equilibrium state after finishing of the cooling process; measurements
of the e+e- recombination rate. Their solution will
give a base for detail elaboration of the first physical experiments with
positronium in-flight, namely o-Ps life-time measurements and precise comparison
of positron and electron electric charges.
This work is supported by Grant RFBR 99-02-17716.
References:
-
Yu.V. Korotaev, I.N. Meshkov, S.V. Mironov, A.O.
Sidorin, and E. Syresin, 6th European Particle Accelerator Conference,
Stockholm, 1998, p. 853.
-
I.N. Meshkov, Fiz. El.Ch.A.Yad. 28 , 495 (1997);
Phys. Part. Nucl. 28, 198 (1997).
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Impact
of Positronium Thermalization on High-Precision Experiments
R.S. Vallery, R.S.
Conti, J.J. Engbrecht, D.W. Gidley, and M. Skalsey
The University of Michigan, Randall Laboratory
of Physics, Ann Arbor, MI 48109-1120, USA
Positronium (Ps) is an excellent system to study
QED, with gases often being the formation medium used. At an initial energy
of several eV when formed in gases, Ps then collides with the gas atoms
and approaches thermal equilibrium. It has been recently found1
that the rate of thermalization is significantly slower than previously
believed. Corrections used to remove gas related collisional effects in
high-precision experiments must include the non-thermal nature of the Ps
population. Examples of affected experiments include orthopositronium (o-Ps)
vacuum decay rate measurements2 ( )
and ground state singlet-triplet splitting3 ( ).
The latter contains gas pressure (Stark) shifts and the former gas collisional
quenching effects ( ).
To experimentally investigate the effect of thermalization
on ,
a measurement of the temperature dependence4 of
in the gases used in Ref. 2 (isobutane, neopentane, Ne, and N2)
was made. It was found that
increases linearly with temperature rather than remaining constant as was
previously assumed. In light of the previous two experiments, a systematic
reanalysis of was then performed. The 1989 data have been refitted
to an elastic thermalization model in which the effective thermalization
rate of positronium near room temperature is a freely fitted parameter.
The corrections remove the observed overdispersive nature of the data and
results in a correction downward of about .
This brings the data in good agreement with a measurement of
in vacuum5. Both measurements remain in disagreement with the
QED theoretical value6 and another measurement using low-density
SiO2 powders7.
Measurements3,8 of ,
which are each in
disagreement with recent theory, may also suffer from systematic effects
due to thermalization. Data in Ref. 3 are acquired at sufficiently low
gas densities where it cannot be assumed that the o-Ps was thermalized.
However, there are no data on the temperature dependence of the
pressure shift and thus the exact impact of thermalization on
cannot be determined at this time. Implications of this effect will be
considered.
This research is supported by NSF Grant PHY-9731861
and the University of Michigan.
References:
-
M. Skalsey, R.K. Bithell, J.J. Engbrecht, R.S. Vallery,
and D.W. Gidley, Phys. Rev. Lett. 80, 3727 (1998).
-
C.I. Westbrook, D.W. Gidley, R.S. Conti, and A. Rich,
Phys. Rev. A 40, 5489 (1989).
-
M.W. Ritter, P.O. Egan, V.W. Hughes, and K.A. Woodle,
Phys. Rev. A. 30, 1331 (1984).
-
R.S. Vallery, A.E. Leanhardt, M. Skalsey, and D.W.
Gidley, accepted for publication in J. Phys. B.
-
J.S. Nico, D.W. Gidley, A. Rich, and Zitzewitz, Phys.
Rev. Lett. 65, 1344 (1990).
-
G.S. Adkins, R.N. Fell, and J. Sapirstein, submitted
to Phys. Rev. Lett..
-
S. Asai , S. Orito, and Hinohara, Phys. Lett. B 357,
475 (1995).
-
A.P.Mills, Jr., and G.H. Bearman, Phys. Rev. Lett.
34,
246 (1975).
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Highly
Accurate Theoretical Simulation of the Resonant 2- and 3-Photon Ionization
Processes with Simplest Atoms
V. Yakhontov1,
K. Jungmann2 and V. Meyer2
1 Institut für Physikalische Chemie,
Klingelbergstr. 80, CH4056 Basel, Switzerland
2 Physikalisches Institut, Philosophenweg
12, D69120 Heidelberg, Germany
We present highly accurate ab initio theoretical
study to simulate ionization probabilities and line profiles for a two-step
3-photon resonant ionization process, ,
of the ground state of muonium (or any hydrogen-like atom). The 1S-2S transition
offers unique opportunities for ultra-high precision spectroscopy due to
the narrow natural line width
of 2Sstate. In hydrogen atom, for example, the smallness of
KHz has already allowed the quality factor
Hz be achieved in the measurement of the 1S-2S energy separation [1]. Experimentally,
the 1S-2S transition can be induced Doppler-free by absorbing two photons
from two identical counter-propagating laser beams. These can be generated
by either asufficiently powerful pulsed laser (as with muonium [2]) or
a continuous laser (as with hydrogen [1]). In the new 1S-2S in muonim recently
finalized at the Rutherford Appleton Laboratory, the use of intense pulsed
laser source to induce above 3-photon process has enabled the 1S-2S energy
interval to be determined to the 9.8 MHz accuracy [2].
In the present work we report new results of our
simulations intended to account for most important contributions to the
energy intervals between atomic level involved in the above resonant 3-photon
process, which arise due to a number of systematic spurious effects that
make their appearance whenever an atom is subject to laser radiation of
arbitrary intensity. The relevance and strong motivation of this study
are discussed in more detail in [2,3]. Our present model constitutes a
significant improvement over our obsolete scheme [3] which was lately used
in analyzing experimental 1S to the model on equal footing. Without imposing
any restriction on the strength of the laser field, the model developed
is currently capable of accounting for its arbitrary spatial and temporary
inhomogeneities, non-zero ionization rates of intermediate atomic relay
levels, along with their Stark shifts and appropriate exact fine structure
contributions. In addition, it allows for the second order Doppler shifts
as well, i.e. takes into account the movement of atoms in a media to order
(v/c)2. This enables the model to be efficiently employed
for a highly accurate analysis of either 2- or 3-photon resonant phenomena
with few-particle systems, which are induced by either pulsed or continuous
sources of laser radiation. Although technically difficult to construct,
high-power continuous CW lasers offer nowadays a number of inviting and
unique opportunities for ultra-high precision spectroscopy with simplest
atoms, especially for those containing -muons.
This makes the current work of relevance and use for both current and future
highly precise studies with various fundamental bounded quantum systems.
References:
-
A. Huber, Udem Th., B. Gross, J. Reichert, M. Kourogi
et al., Phys. Rev. Lett. 80, 468 (1998).
-
V. Meyer, S.N. Bagaev, P.E.G. Baird, P. Bakule, M.G.
Boshier et al. Phys. Rev. Lett. 84, 1136 (2000).
-
V. Yakhontov, R. Santra and K. Jungmann, J. Phys.
B: Atom. Mol. Opt. Phys. 32, 1615 (1999).
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