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@article{ ISI:A1980JM13300003,
Author = {MOHAPATRA, RN and SENJANOVIC, G},
Title = {{NEUTRINO MASS AND SPONTANEOUS PARITY NON-CONSERVATION}},
Journal = {{PHYSICAL REVIEW LETTERS}},
Year = {{1980}},
Volume = {{44}},
Number = {{14}},
Pages = {{912-915}},
Publisher = {{AMERICAN PHYSICAL SOC}},
Address = {{ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA}},
Type = {{Article}},
Language = {{English}},
Affiliation = {{MOHAPATRA, RN (Reprint Author), CUNY CITY COLL,DEPT PHYS,NEW YORK,NY 10031, USA.
UNIV MARYLAND,DEPT PHYS \& ASTRON,COLLEGE PK,MD 20742.}},
DOI = {{10.1103/PhysRevLett.44.912}},
ISSN = {{0031-9007}},
Research-Areas = {{Physics}},
Web-of-Science-Categories = {{Physics, Multidisciplinary}},
Number-of-Cited-References = {{31}},
Times-Cited = {{4003}},
Usage-Count-Last-180-days = {{2}},
Usage-Count-Since-2013 = {{41}},
Journal-ISO = {{Phys. Rev. Lett.}},
Doc-Delivery-Number = {{JM133}},
Unique-ID = {{ISI:A1980JM13300003}},
DA = {{2020-01-24}},
}
@article{ ISI:000275024000019,
Author = {Rueter, Christian E. and Makris, Konstantinos G. and El-Ganainy, Ramy
and Christodoulides, Demetrios N. and Segev, Mordechai and Kip, Detlef},
Title = {{Observation of parity-time symmetry in optics}},
Journal = {{NATURE PHYSICS}},
Year = {{2010}},
Volume = {{6}},
Number = {{3}},
Pages = {{192-195}},
Month = {{MAR}},
Abstract = {{One of the fundamental axioms of quantum mechanics is associated with
the Hermiticity of physical observables(1). In the case of the
Hamiltonian operator, this requirement not only implies real
eigenenergies but also guarantees probability conservation.
Interestingly, a wide class of non-Hermitian Hamiltonians can still show
entirely real spectra. Among these are Hamiltonians respecting
parity-time (PT) symmetry(2-7). Even though the Hermiticity of quantum
observables was never in doubt, such concepts have motivated discussions
on several fronts in physics, including quantum field theories(8),
non-Hermitian Anderson models(9) and open quantum systems(10,11), to
mention a few. Although the impact of PT symmetry in these fields is
still debated, it has been recently realized that optics can provide a
fertile ground where PT-related notions can be implemented and
experimentally investigated(12-15). In this letter we report the first
observation of the behaviour of a PT optical coupled system that
judiciously involves a complex index potential. We observe both
spontaneous PT symmetry breaking and power oscillations violating
left-right symmetry. Our results may pave the way towards a new class of
PT-synthetic materials with intriguing and unexpected properties that
rely on non-reciprocal light propagation and tailored transverse energy
flow.}},
Publisher = {{NATURE PUBLISHING GROUP}},
Address = {{MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND}},
Type = {{Article}},
Language = {{English}},
Affiliation = {{Kip, D (Reprint Author), Tech Univ Clausthal, Inst Energy Res \& Phys Technol, Leibnizstr 4, D-38678 Clausthal Zellerfeld, Germany.
Rueter, Christian E.; Kip, Detlef, Tech Univ Clausthal, Inst Energy Res \& Phys Technol, D-38678 Clausthal Zellerfeld, Germany.
Makris, Konstantinos G.; El-Ganainy, Ramy; Christodoulides, Demetrios N., Univ Cent Florida, CREOL, Sch Opt, Orlando, FL 32816 USA.
Segev, Mordechai, Technion Israel Inst Technol, Dept Phys, IL-32000 Haifa, Israel.}},
DOI = {{10.1038/NPHYS1515}},
ISSN = {{1745-2473}},
EISSN = {{1745-2481}},
Keywords-Plus = {{REAL; EIGENVALUES}},
Research-Areas = {{Physics}},
Web-of-Science-Categories = {{Physics, Multidisciplinary}},
Author-Email = {{[email protected]}},
ResearcherID-Numbers = {{Makris, Konstantinos G/G-3421-2017
Kip, Detlef/C-7021-2013
}},
ORCID-Numbers = {{Kip, Detlef/0000-0001-7923-0113
MacDonald, Allan/0000-0003-3561-3379}},
Funding-Acknowledgement = {{German-Israeli Foundation for Scientific Research and
DevelopmentGerman-Israeli Foundation for Scientific Research and
Development}},
Funding-Text = {{d This research was supported by the German-Israeli Foundation for
Scientific Research and Development.}},
Number-of-Cited-References = {{29}},
Times-Cited = {{1684}},
Usage-Count-Last-180-days = {{37}},
Usage-Count-Since-2013 = {{320}},
Journal-ISO = {{Nat. Phys.}},
Doc-Delivery-Number = {{562BN}},
Unique-ID = {{ISI:000275024000019}},
OA = {{Green Published}},
DA = {{2020-01-24}},
}
@article{ ISI:A1978FM48800025,
Author = {PRESCOTT, CY and ATWOOD, WB and COTTRELL, RLA and DESTAEBLER, H and
GARWIN, EL and GONIDEC, A and MILLER, RH and ROCHESTER, LS and SATO, T
and SHERDEN, DJ and SINCLAIR, CK and STEIN, S and TAYLOR, RE and
CLENDENIN, JE and HUGHES, VW and SASAO, N and SCHULER, KP and BORGHINI,
MG and LUBELSMEYER, K and JENTSCHKE, W},
Title = {{PARITY NON-CONSERVATION IN INELASTIC ELECTRON-SCATTERING}},
Journal = {{PHYSICS LETTERS B}},
Year = {{1978}},
Volume = {{77}},
Number = {{3}},
Pages = {{347-352}},
Publisher = {{ELSEVIER SCIENCE BV}},
Address = {{PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS}},
Type = {{Article}},
Language = {{English}},
Affiliation = {{PRESCOTT, CY (Reprint Author), STANFORD UNIV,STANFORD LINEAR ACCELERATOR CTR,STANFORD,CA 94305, USA.
YALE UNIV,NEW HAVEN,CT 06520.
CERN,CH-1211 GENEVA 23,SWITZERLAND.
RHEIN WESTFAL TH AACHEN,D-5100 AACHEN,FED REP GER.
UNIV HAMBURG,INST,EXPTL PHYS 2,D-2000 HAMBURG,FED REP GER.}},
DOI = {{10.1016/0370-2693(78)90722-0}},
ISSN = {{0370-2693}},
Research-Areas = {{Astronomy \& Astrophysics; Physics}},
Web-of-Science-Categories = {{Astronomy \& Astrophysics; Physics, Nuclear; Physics, Particles \&
Fields}},
Number-of-Cited-References = {{24}},
Times-Cited = {{627}},
Usage-Count-Last-180-days = {{2}},
Usage-Count-Since-2013 = {{5}},
Journal-ISO = {{Phys. Lett. B}},
Doc-Delivery-Number = {{FM488}},
Unique-ID = {{ISI:A1978FM48800025}},
DA = {{2020-01-24}},
}
@article{ ISI:000245302600004,
Author = {Djouadi, Abdelhak and Kneur, Jean-Loic and Moultaka, Gilbert},
Title = {{SuSpect: A Fortran code for the Supersymmetric and Higgs particle
spectrum in the MSSM}},
Journal = {{COMPUTER PHYSICS COMMUNICATIONS}},
Year = {{2007}},
Volume = {{176}},
Number = {{6}},
Pages = {{426-455}},
Month = {{MAR 15}},
Abstract = {{We present the FORTRAN code SuSpect version 2.3, which calculates the
Supersymmetric and Higgs particle spectrum in the Minimal Supersymmetric
Standard Model (MSSM). The calculation can be performed in constrained
models with universal boundary conditions at high scales such as the
gravity (mSUGRA), anomaly (AMSB) or gauge (GMSB) mediated supersymmetry
breaking models, but also in the non-universal MSSM case with R-parity
and CP conservation. Care has been taken to treat important features
such as the renormalization group evolution of parameters between low
and high energy scales, the consistent implementation of radiative
electroweak symmetry breaking and the calculation of the physical masses
of the Higgs bosons and supersymmetric particles taking into account the
dominant radiative corrections. Some checks of important theoretical and
experimental features, such as the absence of non-desired minima, large
fine-tuning in the electroweak symmetry breaking condition, as well as
agreement with precision measurements can be performed. The program is
simple to use, self-contained and can easily be linked to other codes;
it is rather fast and flexible, thus allowing scans of the parameter
space with several possible options and choices for model assumptions
and approximations.}},
Publisher = {{ELSEVIER SCIENCE BV}},
Address = {{PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS}},
Type = {{Review}},
Language = {{English}},
Affiliation = {{Djouadi, A (Reprint Author), Univ Montpellier 2, Lab Phys Theor \& Astroparticules, CNRS, UMR 5207, F-34095 Montpellier 5, France.
Univ Montpellier 2, Lab Phys Theor \& Astroparticules, CNRS, UMR 5207, F-34095 Montpellier 5, France.
Univ Paris 11, Lab Phys Theor Orsay, CNRS, UMR 8627, F-91405 Orsay, France.}},
DOI = {{10.1016/j.cpc.2006.11.009}},
ISSN = {{0010-4655}},
EISSN = {{1879-2944}},
Keywords = {{supersymmetry; renormalization group equations; loop calculations}},
Keywords-Plus = {{GRAND UNIFIED THEORIES; RENORMALIZATION-GROUP EQUATIONS; ANOMALOUS
MAGNETIC-MOMENT; LEADING QCD CORRECTIONS; SOFTLY BROKEN SUPERSYMMETRY;
ELECTROWEAK RHO-PARAMETER; LOW-ENERGY SUPERGRAVITY; NEUTRALINO
DARK-MATTER; QUANTUM-FIELD THEORY; ONE-LOOP CORRECTIONS}},
Research-Areas = {{Computer Science; Physics}},
Web-of-Science-Categories = {{Computer Science, Interdisciplinary Applications; Physics, Mathematical}},
Author-Email = {{[email protected]}},
Number-of-Cited-References = {{256}},
Times-Cited = {{583}},
Usage-Count-Last-180-days = {{0}},
Usage-Count-Since-2013 = {{10}},
Journal-ISO = {{Comput. Phys. Commun.}},
Doc-Delivery-Number = {{151PK}},
Unique-ID = {{ISI:000245302600004}},
DA = {{2020-01-24}},
}
@article{ ISI:000245020600005,
Author = {Belanger, G. and Boudjema, F. and Pukhov, A. and Semenov, A.},
Title = {{micrOMEGAs 2.0: A program to calculate the relic density of dark matter
in a generic model}},
Journal = {{COMPUTER PHYSICS COMMUNICATIONS}},
Year = {{2007}},
Volume = {{176}},
Number = {{5}},
Pages = {{367-382}},
Month = {{MAR 1}},
Abstract = {{micrOMEGAs 2.0 is a code which calculates the relic density of a stable
massive particle in an arbitrary model. The underlying assumption is
that there is a conservation law like R-parity in supersymmetry which
guarantees the stability of the lightest odd particle. The new physics
model must be incorporated in the notation of CalcHEP, a package for the
automatic generation of squared matrix elements. Once this is done, all
annihilation and coannihilation channels are included automatically in
any model. Cross-sections at v = 0, relevant for indirect detection of
dark matter, are also computed automatically. The package includes three
sample models: the minimal supersymmetric standard model (MSSM), the
MSSM with complex phases and the NMSSM. Extension to other models,
including non-supersymmetric models, is described.
Program summary
Title of program: micrOMEGAs2.0
Catalogue identifier: ADQR\_v2\_0
Program summary URL: http://cpc.cs.qub.ac.uk/summaries/ADQR-v2-0
Program obtainable from: CPC Program Library, Queen's University of
Belfast, N. Ireland
Computers for which the program is designed and others on which it has
been tested: PC, Alpha, Mac, Sun
Operating systems under which the program has been tested: UNIX (Linux,
OSFI, SunOS, Darwin, Cygwin)
Programming language used: C and Fortran
Memory required to execute with typical data: 17 MB depending on the
number of processes required
No. of processors used: 1
Has the code been vectorized or parallelized: no
No. of lines in distributed program, including test data, etc.: 91 778
No. of bytes M distributed program, including test data, etc.: 1306 726
Distribution format: tar.gz
External routines/libraries used: no
Catalogue identifier of previous version: ADQR\_v1\_3
Journal reference of previous version: Comput. Phys. Comm. 174 (2006)
577
Does the new version supersede the previous version: yes
Nature of physical problem: Calculation of the relic density of the
lightest stable particle in a generic new model of particle physics.
Method of solution: In numerically solving the evolution equation for
the density of dark matter, relativistic formulae for the thermal
average are used. All tree-level processes for annihilation and
coannihilation of new particles in the model are included. The
cross-sections for all processes are calculated exactly with CalcHEP
after definition of a model file. Higher-order QCD corrections to Higgs
couplings to quark pairs are included.
Reasons for the new version: There are many models of new physics that
propose a candidate for dark matter besides the much studied minimal
supersymmetric standard model. This new version not only incorporates
extensions of the MSSM, such as the MSSM with complex phases, or the
NSSM which contains an extra singlet superfield but also gives the
possibility for the user to incorporate easily a new model. For this the
user only needs to redefine appropriately a new model file.
Summary of revisions:
Possibility to include in the ppackage any particle physics model with a
discrete symmetry that guarantees the stability of the cold dark matter
candidate (LOP) and to compute the relic density of CDM.
Compute automatically the cross-sections for annihilation of the LOP at
small velocities into SM final states and provide the energy spectra for
gamma, e(+), (p) over bar, nu final states.
For the MSSM with input parameters defined at the GUT scale, the
interface with any of the spectrum calculator codes reads an input file
in the SUSY Les Houches Accord format (SLHA).
Implementation of the MSSM with complex parameters (CPV-MSSM) with an
interface to CPsuperH to calculate the spectrum.
Routine to calculate the electric dipole moment of the electron in the
CPV-MSSM.
In the NMSSM, new interface compatible with NMHDECAY2.1.
Typical running time: 0.2 sec
Unusual features of the program: Depending on the parameters of the
model, the program generates additional new code, compiles it and loads
it dynamically.
(C) 2006 Elsevier B.V. All rights reserved.}},
Publisher = {{ELSEVIER SCIENCE BV}},
Address = {{PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS}},
Type = {{Article}},
Language = {{English}},
Affiliation = {{Belanger, G (Reprint Author), Lab Phys Theor LAPTH, F-74941 Annecy Le Vieux, France.
Lab Phys Theor LAPTH, F-74941 Annecy Le Vieux, France.
Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119992, Russia.
Joint Inst Nucl Res, Dubna 141980, Russia.}},
DOI = {{10.1016/j.cpc.2006.11.008}},
ISSN = {{0010-4655}},
EISSN = {{1879-2944}},
Keywords = {{dark matter; relic density; MSSM; Beyond Standard Model}},
Keywords-Plus = {{SUPERSYMMETRIC STANDARD MODEL; ELECTRIC-DIPOLE MOMENTS; PROBE WMAP
OBSERVATIONS; COSMOLOGICAL PARAMETERS; HIGGS MASSES; NEUTRALINO; MSSM;
SEARCHES; PARTICLE; SPECTRA}},
Research-Areas = {{Computer Science; Physics}},
Web-of-Science-Categories = {{Computer Science, Interdisciplinary Applications; Physics, Mathematical}},
Author-Email = {{[email protected]}},
ORCID-Numbers = {{Boudjema, Fawzi/0000-0003-4668-7584}},
Number-of-Cited-References = {{61}},
Times-Cited = {{457}},
Usage-Count-Last-180-days = {{1}},
Usage-Count-Since-2013 = {{24}},
Journal-ISO = {{Comput. Phys. Commun.}},
Doc-Delivery-Number = {{147RR}},
Unique-ID = {{ISI:000245020600005}},
DA = {{2020-01-24}},
}
@article{ ISI:A1979HE74800038,
Author = {PRESCOTT, CY and ATWOOD, WB and COTTRELL, RLA and DESTAEBLER, H and
GARWIN, EL and GONIDEC, A and MILLER, RH and ROCHESTER, LS and SATO, T
and SHERDEN, DJ and SINCLAIR, CK and STEIN, S and TAYLOR, RE and YOUNG,
C and CLENDENIN, JE and HUGHES, VW and SASAO, N and SCHULER, KP and
BORGHINI, MG and LUBELSMEYER, K and JENTSCHKE, W},
Title = {{FURTHER MEASUREMENTS OF PARITY NON-CONSERVATION IN INELASTIC
ELECTRON-SCATTERING}},
Journal = {{PHYSICS LETTERS B}},
Year = {{1979}},
Volume = {{84}},
Number = {{4}},
Pages = {{524-528}},
Publisher = {{ELSEVIER SCIENCE BV}},
Address = {{PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS}},
Type = {{Article}},
Language = {{English}},
Affiliation = {{PRESCOTT, CY (Reprint Author), STANFORD UNIV,STANFORD LINEAR ACCELERATOR CTR,STANFORD,CA 94305, USA.
YALE UNIV,NEW HAVEN,CT 06520.
CERN,CH-1211 GENEVA 23,SWITZERLAND.
RHEIN WESTFAL TH AACHEN,D-5100 AACHEN,FED REP GER.
UNIV HAMBURG,INST EXPT PHYS 2,D-2000 HAMBURG 13,FED REP GER.}},
DOI = {{10.1016/0370-2693(79)91253-X}},
ISSN = {{0370-2693}},
Research-Areas = {{Astronomy \& Astrophysics; Physics}},
Web-of-Science-Categories = {{Astronomy \& Astrophysics; Physics, Nuclear; Physics, Particles \&
Fields}},
Number-of-Cited-References = {{18}},
Times-Cited = {{414}},
Usage-Count-Last-180-days = {{0}},
Usage-Count-Since-2013 = {{5}},
Journal-ISO = {{Phys. Lett. B}},
Doc-Delivery-Number = {{HE748}},
Unique-ID = {{ISI:A1979HE74800038}},
DA = {{2020-01-24}},
}
@article{ ISI:A1991GQ57000001,
Author = {BONNER, WA},
Title = {{THE ORIGIN AND AMPLIFICATION OF BIOMOLECULAR CHIRALITY}},
Journal = {{ORIGINS OF LIFE AND EVOLUTION OF BIOSPHERES}},
Year = {{1991}},
Volume = {{21}},
Number = {{2}},
Pages = {{59-111}},
Publisher = {{SPRINGER}},
Address = {{VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS}},
Type = {{Review}},
Language = {{English}},
Affiliation = {{BONNER, WA (Reprint Author), STANFORD UNIV, DEPT CHEM, STANFORD, CA 94305 USA.}},
DOI = {{10.1007/BF01809580}},
ISSN = {{0169-6149}},
EISSN = {{1573-0875}},
Keywords-Plus = {{ABSOLUTE ASYMMETRIC-SYNTHESIS; CIRCULARLY POLARIZED-LIGHT; VIOLATING
ENERGY DIFFERENCES; QUANTITATIVE ENANTIOMERIC YIELD; PROCHIRAL
CHEMICAL-REACTIONS; OPTICALLY-ACTIVE MOLECULES; PARITY NON-CONSERVATION;
ALPHA-AMINO-ACIDS; GAS-CHROMATOGRAPHIC ANALYSIS; MIRROR
SYMMETRY-BREAKING}},
Research-Areas = {{Life Sciences \& Biomedicine - Other Topics}},
Web-of-Science-Categories = {{Biology}},
Number-of-Cited-References = {{515}},
Times-Cited = {{385}},
Usage-Count-Last-180-days = {{9}},
Usage-Count-Since-2013 = {{117}},
Journal-ISO = {{Orig. Life Evol. Biosph.}},
Doc-Delivery-Number = {{GQ570}},
Unique-ID = {{ISI:A1991GQ57000001}},
DA = {{2020-01-24}},
}
@article{ ISI:000221981700001,
Author = {Ginges, JSM and Flambaum, VV},
Title = {{Violations of fundamental symmetries in atoms and tests of unification
theories of elementary particles}},
Journal = {{PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS}},
Year = {{2004}},
Volume = {{397}},
Number = {{2}},
Pages = {{63-154}},
Month = {{JUL}},
Abstract = {{High-precision measurements of violations of fundamental symmetries in
atoms are a very effective means of testing the standard model of
elementary particles and searching for new physics beyond it. Such
studies complement measurements at high energies. We review the recent
progress in atomic parity nonconservation and atomic electric dipole
moments (time reversal symmetry violation), with a particular focus on
the atomic theory required to interpret the measurements. (C) 2004
Elsevier B.V. All rights reserved.}},
Publisher = {{ELSEVIER SCIENCE BV}},
Address = {{PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS}},
Type = {{Review}},
Language = {{English}},
Affiliation = {{Flambaum, VV (Reprint Author), Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia.
Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia.}},
DOI = {{10.1016/j.physrep.2004.03.005}},
ISSN = {{0370-1573}},
EISSN = {{1873-6270}},
Keywords-Plus = {{ELECTRIC-DIPOLE-MOMENT; NONCONSERVING OPTICAL-ROTATION; PARITY
NON-CONSERVATION; NUCLEAR ANAPOLE MOMENTS; BODY PERTURBATION-THEORY;
WEAK NEUTRAL CURRENTS; HIGH-ACCURACY CALCULATION; TIME-REVERSAL
INVARIANCE; HARTREE-FOCK-CALCULATION; P-ALPHA-SCATTERING}},
Research-Areas = {{Physics}},
Web-of-Science-Categories = {{Physics, Multidisciplinary}},
Author-Email = {{[email protected]}},
ResearcherID-Numbers = {{Ginges, Jacinda/O-7169-2016}},
ORCID-Numbers = {{Ginges, Jacinda/0000-0003-0390-0891}},
Number-of-Cited-References = {{384}},
Times-Cited = {{384}},
Usage-Count-Last-180-days = {{1}},
Usage-Count-Since-2013 = {{26}},
Journal-ISO = {{Phys. Rep.-Rev. Sec. Phys. Lett.}},
Doc-Delivery-Number = {{828OD}},
Unique-ID = {{ISI:000221981700001}},
DA = {{2020-01-24}},
}
@article{ ISI:000245922000052,
Author = {Ibanez, Luis E. and Uranga, Angel M.},
Title = {{Neutrino Majorana masses from string theory instanton eff ects}},
Journal = {{JOURNAL OF HIGH ENERGY PHYSICS}},
Year = {{2007}},
Number = {{3}},
Month = {{MAR}},
Abstract = {{Finding a plausible origin for right- handed neutrino Majorana masses in
semirealistic compactifications of string theory remains one of the most
difficult cult problems in string phenomenology. We argue that right-
handed neutrino Majorana masses are induced by non-perturbative
instanton effects ects in certain classes of string compactifications in
which the U(1) B-L gauge boson has a Stuckelberg mass. The induced
operators are of the form e(vRvR)(-U) where U is a closed string modulus
whose imaginary part transforms appropriately under B-L. This mass term
may be quite large since this is not a gauge instanton and ReU is not
directly related to SM gauge couplings. Thus the size of the induced
right- handed neutrino masses could be a few orders of magnitude below
the string scale, as phenomenologically required. It is also argued that
this origin for neutrino masses would predict the existence of R-parity
in SUSY versions of the SM. Finally we comment on other phenomenological
applications of similar instanton effects, like the generation of a
mu-term, or of Yukawa couplings forbidden in perturbation theory.}},
Publisher = {{SPRINGER}},
Address = {{233 SPRING ST, NEW YORK, NY 10013 USA}},
Type = {{Article}},
Language = {{English}},
Affiliation = {{Ibanez, LE (Reprint Author), Univ Autonoma Madrid, Dept Fis Teor 111, Madrid 28049, Spain.
Univ Autonoma Madrid, Dept Fis Teor 111, Madrid 28049, Spain.
Univ Autonoma Madrid, Inst Fis Teor 116, Madrid 28049, Spain.
CERN, PHTH Div, CH-1211 Geneva 23, Switzerland.}},
DOI = {{10.1088/1126-6708/2007/03/052}},
Article-Number = {{052}},
ISSN = {{1029-8479}},
Keywords = {{D-branes; superstring vacua; neutrino physics; intersecting branes
models}},
Keywords-Plus = {{STANDARD MODEL; WORLD-SHEET; COMPACTIFICATIONS; SUPERPOTENTIALS;
ORIENTIFOLDS; CONSERVATION; BRANES; VACUA}},
Research-Areas = {{Physics}},
Web-of-Science-Categories = {{Physics, Particles \& Fields}},
Author-Email = {{[email protected]
ORCID-Numbers = {{Uranga, Angel/0000-0002-8203-2545}},
Number-of-Cited-References = {{57}},
Times-Cited = {{224}},
Usage-Count-Last-180-days = {{0}},
Usage-Count-Since-2013 = {{1}},
Journal-ISO = {{J. High Energy Phys.}},
Doc-Delivery-Number = {{160DV}},
Unique-ID = {{ISI:000245922000052}},
OA = {{Bronze}},
DA = {{2020-01-24}},
}
@article{ ISI:A1992HH41900017,
Author = {BLUNDELL, SA and SAPIRSTEIN, J and JOHNSON, WR},
Title = {{HIGH-ACCURACY CALCULATION OF PARITY NONCONSERVATION IN CESIUM AND
IMPLICATIONS FOR PARTICLE PHYSICS}},
Journal = {{PHYSICAL REVIEW D}},
Year = {{1992}},
Volume = {{45}},
Number = {{5}},
Pages = {{1602-1623}},
Month = {{MAR 1}},
Abstract = {{High-precision measurement of atomic parity-nonconserving transitions in
cesium when coupled with calculations of similar accuracy allow for a
precise determination of Q(w), the weak nuclear charge. When expressed
in terms of the Z mass, radiative corrections to Q(w) are insensitive to
the top-quark mass, so such a determination of Q(w) allows a
particularly sensitive probe of radiative corrections depending on new
physics. While the wave function of cesium, the atom in which the most
accurate measurements have been made, is extremely complex, atomic
theory has advanced to a point where predictions accurate to 1\% can be
made. This paper describes such a calculation with particular emphasis
on the question of the reliability of the atomic theory.
Particle-physics implications following from the present state of theory
and experiment are discussed, and prospects for more accurate work
described.}},
Publisher = {{AMERICAN PHYSICAL SOC}},
Address = {{ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA}},
Type = {{Article}},
Language = {{English}},
Affiliation = {{UNIV CALIF LAWRENCE LIVERMORE NATL LAB,LIVERMORE,CA 94550.
UNIV NOTRE DAME,DEPT PHYS,NOTRE DAME,IN 46556.}},
DOI = {{10.1103/PhysRevD.45.1602}},
ISSN = {{0556-2821}},
Keywords-Plus = {{BODY PERTURBATION-THEORY; WEAK NEUTRAL CURRENTS; NUCLEAR ANAPOLE
MOMENTS; FREE GAUGE THEORIES; ATOMIC CESIUM; NON-CONSERVATION;
MATRIX-ELEMENTS; PRECISION-MEASUREMENT; 6S->7S TRANSITION; 6S-7S
TRANSITION}},
Research-Areas = {{Astronomy \& Astrophysics; Physics}},
Web-of-Science-Categories = {{Astronomy \& Astrophysics; Physics, Particles \& Fields}},
Number-of-Cited-References = {{71}},
Times-Cited = {{204}},
Usage-Count-Last-180-days = {{0}},
Usage-Count-Since-2013 = {{6}},
Journal-ISO = {{Phys. Rev. D}},
Doc-Delivery-Number = {{HH419}},
Unique-ID = {{ISI:A1992HH41900017}},
DA = {{2020-01-24}},
}