High Magnetic Fields for Fundamental Physics
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Gammev: Fermilab Axion-Like Particle Photon Regeneration Results
GammeV: Fermilab Axion-like Particle Photon Regeneration Results William Wester Fermilab, MS222, Batavia IL, USA presented on behalf of the GammeV Collaboration DOI: http://dx.doi.org/10.3204/DESY-PROC-2008-02/wester william GammeV is an axion-like particle photon regeneration experiment conducted at Fermilab that employs the light shining through a wall technique. We obtain limits on the cou- pling of a photon to an axion-like particle that extend previous limits for both scalar and pseudoscalar axion-like particles in the milli-eV mass range. We are able to exclude the axion-like particle interpretation of the anomalous PVLAS 2006 result by more than 5 standard deviations. 1 Introduction The question, What are the particles that make up the dark matter of the universe?, is one of the most fundamental scientific questions today. Besides weakly interacting massive particles (WIMPs) such as neutralinos, axion-like particles or other weakly interacting sub-eV particles (WISPs) are highly motivated dark matter particle candidates since they have properties that might explain the cosmic abundance of dark matter. The milli-eV mass scale is of particular interest in modern particle physics since that mass scale may be constructed with a see-saw between the Planck and TeV mass scales, and may be related to neutrino mass differences, the dark energy density expressed in (milli-eV)4, and known dark matter candidates such as gravitinos and axion-like particles. In 2006, the PVLAS experiment reported [1] anomalous polarization effects in the presence of a magnetic field including polarization rotation and el- lipticity generation that could be interpreted as being mediated by an axion-like particle in the milli-eV mass range with a unexpectedly strong coupling to photons. -
Circular and Linear Magnetic Birefringences in Xenon at =1064 Nm
Downloaded from orbit.dtu.dk on: Oct 06, 2021 Circular and linear magnetic birefringences in xenon at =1064 nm Cadene, Agathe; Fouche, Mathilde; Rivere, Alice; Battesti, Remy; Coriani, Sonia; Rizzo, Antonio; Rizzo, Carlo Published in: Journal of Chemical Physics Link to article, DOI: 10.1063/1.4916049 Publication date: 2015 Document Version Publisher's PDF, also known as Version of record Link back to DTU Orbit Citation (APA): Cadene, A., Fouche, M., Rivere, A., Battesti, R., Coriani, S., Rizzo, A., & Rizzo, C. (2015). Circular and linear magnetic birefringences in xenon at =1064 nm. Journal of Chemical Physics, 142(12), [124313]. https://doi.org/10.1063/1.4916049 General rights Copyright and moral rights for the publications made accessible in the public portal are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. Users may download and print one copy of any publication from the public portal for the purpose of private study or research. You may not further distribute the material or use it for any profit-making activity or commercial gain You may freely distribute the URL identifying the publication in the public portal If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Circular and linear magnetic birefringences in xenon at λ = 1064 nm Agathe Cadène, Mathilde Fouché, Alice Rivère, -
Strategies for the Detection of Dark Matter
Bernard Sadoulet Dept. of Physics /LBNL UC Berkeley UC Institute for Nuclear and Particle Astrophysics and Cosmology (INPAC) Strategies for the Detection of Dark Matter What do we know? What have we achieved so far? Strategies for the future Strategies for the Detection f Dark Matter Hanoi 10 Aug 06 1 B.Sadoulet 1. What do we know? 2. What has been achieved? 3. Strategies for the future Standard Model of Cosmology A surprising but consistent picture Non Baryonic Λ Dark Matter Ω Ωmatter Not ordinary matter (Baryons) Nucleosynthesis Ω >> Ω = 0.047 ± 0.006 from m b WMAP Mostly cold: Not light neutrinos≠ small scale structure mv < .17eV Large Scale structure+baryon oscillation + Lyman α Strategies for the Detection f Dark Matter Hanoi 10 Aug 06 2 B.Sadoulet 1. What do we know? 2. What has been achieved? 3. Strategies for the future Ongoing Systematic Mapping dark matter and energy non baryonic Λ Quintessence baryonic clumped H2? ? gas Primordial Black Holes VMO Mirror branes ? exotic particles dust Energy in bulk MACHOs thermal non-thermal SuperWIMPs Light Neutrinos WIMPs Axions Wimpzillas Most baryonic forms excluded (independently of BBN, CMB) Particles: well defined if thermal (difficult when athermal) Additional dimensions? Strategies for the Detection f Dark Matter Hanoi 10 Aug 06 3 B.Sadoulet 1. What do we know? 2. What has been achieved? 3. Strategies for the future Standard Model of Particle Physics Fantastic success but Model is unstable Why is W and Z at ≈100 Mp? Need for new physics at that scale supersymmetry additional dimensions Flat: Cheng et al. -
Axial Field Permanent Magnet Machines with High Overload Capability for Transient Actuation Applications
THE UNIVERSITY OF SHEFFIELD Axial field permanent magnet machines with high overload capability for transient actuation applications By Jiangnan Gong A Thesis submitted for the degree of Doctor of Philosophy Department of Electronic and Electrical Engineering The University of Sheffield. JANUARY 2018 ABSTRACT This thesis describes the design, construction and testing of an axial field permanent magnet machine for an aero-engine variable guide vane actuation system. The electrical machine is used in combination with a leadscrew unit that results in a minimum torque specification of 50Nm up to a maximum speed of 500rpm. The combination of the geometry of the space envelope available and the modest maximum speed lends itself to the consideration of an axial field permanent magnet machines. The relative merits of three topologies of double-sided permanent magnet axial field machines are discussed, viz. a slotless toroidal wound machine, a slotted toroidal machine and a yokeless axial field machine with separate tooth modules. Representative designs are established and analysed with three-dimensional finite element method, each of these 3 topologies are established on the basis of a transient winding current density of 30A/mm2. Having established three designs and compared their performance at the rated 50Nm point, further overload capability is compared in which the merits of the slotless machine is illustrated. Specifically, this type of axial field machine retains a linear torque versus current characteristic up to higher torques than the other two topologies, which are increasingly affected by magnetic saturation. Having selected a slotless machine as the preferred design, further design optimization was performed, including detailed assessment of transient performance. -
PLL Approach to Mitigate Symmetrical Faults in Weak AC Grid of DFIG Based Wind Turbine for Voltage Stability Analysis
International Journal of Electrical Electronics & Computer Science Engineering Volume 5, Issue 2 (April, 2018) | E-ISSN : 2348-2273 | P-ISSN : 2454-1222 Available Online at www.ijeecse.com PLL Approach to Mitigate Symmetrical Faults in Weak AC Grid of DFIG Based Wind Turbine for Voltage Stability Analysis Cholleti Sriram1, O. Rakesh2, M. Harish3, A. Sridhar4 1Assistant Professor, 2-4UG Scholars, EEE Department, Guru Nanak Institute of Technology, Hyderabad, India [email protected], [email protected] Abstract: Study of Instability issues of the grid-connected of wind turbines (WTs) based on doubly fed induction doubly fed induction generator (DFIG) based wind turbines generators (DFIG) that intends to improve its low- (WTs) during low-voltage ride-through (LVRT) have got voltage ride through(LVRT) capability. The main little attention yet. In this paper, the small-signal behavior of objective of this work is to design an algorithm that DFIG WTs attached to weak AC grid with high impedances would enable the system to control the initial over during the period of LVRT is investigated, with special attention paid to the rotor-side converter (RSC). Firstly, currents that appear in the generator during voltage based on the studied LVRT strategy, the influence of the sags, which can damage the RSC, without tripping it. high-impedance grid is summarized as the interaction As a difference with classical solutions, based on the between phase-looked loop (PLL) and rotor current installation of crowbar circuits, this operation mode controller (RCC). As modal analysis result indicates that the permits to keep the inverter connected to the generator, underdamped poles are dominated by PLL, complex torque something that would permit the injection of power to coefficient method (CTCM), which is conventionally applied the grid during the fault, as the new grid codes demand. -
Arxiv:2101.08781V1 [Hep-Ph] 21 Jan 2021
MI-TH-2135 PASSAT at Future Neutrino Experiments: Hybrid Beam-Dump-Helioscope Facilities to Probe Light Axion-Like Particles P. S. Bhupal Dev,1, ∗ Doojin Kim,2, y Kuver Sinha,3, z and Yongchao Zhang4, 1, x 1Department of Physics and McDonnell Center for the Space Sciences, Washington University, St. Louis, MO 63130, USA 2Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA 3Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, USA 4School of Physics, Southeast University, Nanjing 211189, China There are broadly three channels to probe axion-like particles (ALPs) produced in the laboratory: through their subsequent decay to Standard Model (SM) particles, their scattering with SM particles, or their subsequent conversion to photons. Decay and scattering are the most commonly explored channels in beam-dump type experiments, while conversion has typically been utilized by light- shining-through-wall (LSW) experiments. A new class of experiments, dubbed PASSAT (Particle Accelerator helioScopes for Slim Axion-like-particle deTection), has been proposed to make use of the ALP-to-photon conversion in a novel way: ALPs, after being produced in a beam-dump setup, turn into photons in a magnetic field placed near the source. It has been shown that such hybrid beam-dump-helioscope experiments can probe regions of parameter space that have not been investigated by other laboratory-based experiments, hence providing complementary information; in particular, they probe a fundamentally different region than decay or LSW experiments. We propose the implementation of PASSAT in future neutrino experiments, taking a DUNE-like experiment as an example. -
Signal Processing in the PVLAS Experiment
Signal Processing in the PVLAS Experiment E. ZAVATTINI1, G. ZAVATTINI4, G. RUOSO2, E. POLACCO3, E. MILOTTI,1, M. KARUZA1, U. GASTALDI 2, G. DI DOMENICO4, F. DELLA VALLE1, R. CIMINO5, S. CARUSOTTO3, G. CANTATORE1, M. BREGANT1 1 - Università e I.N.F.N. Trieste, Via Valerio 2, 34127 Trieste, ITALY 2 - Lab. Naz.di Legnaro dell’I.N.F.N., Viale dell’Università 2, 35020 Legnaro, ITALY 3 - Università e I.N.F.N. Pisa, Via F. Buonarroti 2, 56100 Pisa, ITALY 4 - Università e I.N.F.N. Ferrara, Via del Paradiso 12, 44100 Ferrara, ITALY 5 - Lab. Naz.di Frascati dell’I.N.F.N., Via E. Fermi 40, 00044 Frascati, ITALY [email protected] http://www.ts.infn.it/experiments/pvlas/ Abstract: - Nonlinear interactions of light with light are well known in quantum electronics, and it is quite common to generate harmonic or subharmonic beams from a primary laser with photonic crystals. One suprising result of quantum electrodynamics is that because of the quantum fluctuations of charged fields, the same can happen in vacuum. The virtual charged particle pairs can be polarized by an external field and vacuum can thus become birefringent: the PVLAS experiment was originally meant to explore this strange quantum regime with optical methods. Since its inception PVLAS has found a new, additional goal: in fact vacuum can become a dichroic medium if we assume that it is filled with light neutral particles that couple to two photons, and thus PVLAS can search for exotic particles as well. PVLAS implements a complex signal processing scheme: here we describe the double data acquisition chain and the data analysis methods used to process the experimental data. -
Axions (A0) and Other Very Light Bosons, Searches for See the Related Review(S): Axions and Other Similar Particles
Citation: M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, 030001 (2018) Axions (A0) and Other Very Light Bosons, Searches for See the related review(s): Axions and Other Similar Particles A0 (Axion) MASS LIMITS from Astrophysics and Cosmology These bounds depend on model-dependent assumptions (i.e. — on a combination of axion parameters). VALUE (MeV) DOCUMENT ID TECN COMMENT We do not use the following data for averages, fits, limits, etc. ••• ••• >0.2 BARROSO 82 ASTR Standard Axion >0.25 1 RAFFELT 82 ASTR Standard Axion >0.2 2 DICUS 78C ASTR Standard Axion MIKAELIAN 78 ASTR Stellar emission >0.3 2 SATO 78 ASTR Standard Axion >0.2 VYSOTSKII 78 ASTR Standard Axion 1 Lower bound from 5.5 MeV γ-ray line from the sun. 2 Lower bound from requiring the red giants’ stellar evolution not be disrupted by axion emission. A0 (Axion) and Other Light Boson (X 0) Searches in Hadron Decays Limits are for branching ratios. VALUE CL% DOCUMENT ID TECN COMMENT We do not use the following data for averages, fits, limits, etc. ••• ••• <2 10 10 95 1 AAIJ 17AQ LHCB B+ K+ X 0 (X 0 µ+ µ ) × − → → − <3.7 10 8 90 2 AHN 17 KOTO K0 π0 X 0, m = 135 MeV × − L → X 0 11 3 0 0 + <6 10− 90 BATLEY 17 NA48 K± π± X (X µ µ−) × 4 → 0 0 →+ WON 16 BELL η γ X (X π π−) 9 5 0→ 0 0 → 0 + <1 10− 95 AAIJ 15AZ LHCB B K∗ X (X µ µ−) × 6 6 0 → 0 0 →+ <1.5 10− 90 ADLARSON 13 WASA π γ X (X e e−), × m→ = 100 MeV→ X 0 <2 10 8 90 7 BABUSCI 13B KLOE φ η X0 (X 0 e+ e ) × − → → − 8 ARCHILLI 12 KLOE φ η X0, X 0 e+ e → → − <2 10 15 90 9 GNINENKO 12A BDMP π0 γ X 0 (X 0 e+ e ) × − → → − -
Dark Matter Vienna University of Technology V2.1
Dark Matter Vienna University of Technology V2.1 Jochen Schieck and Holger Kluck Institut f¨urHochenergiephysik Nikolsdorfer Gasse 18 1050 Wien Atominstitut derTechnischen Universit¨atWien Stadionallee 2 1020 Wien Wintersemester 2017/18 18.12.2017 2 Contents 1 Introduction 7 1.1 What is "Dark Matter" . .7 1.1.1 Dark . .7 1.1.2 Matter . .7 1.1.3 Cosmology . .7 1.1.4 Massive particles as origin of "Dark Matter" . .7 1.1.5 "Dark Matter" as contribution to the energy density of the universe in Cosmology . .7 1.2 First Indication of observing "Dark Matter" . 13 1.3 Brief Introduction to Cosmology . 15 1.3.1 Special Relativity . 16 1.3.2 Differential geometry . 16 1.3.3 General Relativity . 16 1.3.4 Cosmology . 17 1.3.5 Decoupling of matter and radiation . 18 1.4 The Standard Model of Particle Physics . 19 1.4.1 The matter content of the Standard Model . 19 1.4.2 Forces within the Standard Model . 19 1.4.3 Shortcoming of the Standard Model . 20 1.4.4 Microscopic Behaviour of Gravity . 21 2 Evidence 23 2.1 Dynamics of Galaxies . 23 2.2 Gravitational Lensing . 24 2.2.1 Bullet Cluster . 31 2.3 Cosmic Microwave Background . 33 2.4 Primordial Nucleosynthesis (Big Bang Nucleosynthesis - BBN) . 35 3 Structure Evolution 39 3.1 Structure Formation . 39 3.1.1 The Classic Picture . 39 3.1.2 Structure Formation and Cosmology . 41 3.2 Model of the Dark Matter Halo in our Galaxy . 45 3 4 Unsolved Questions and Open Issues 49 4.1 Core-Cusp Problem . -
Dark Matter in Nuclear Physics
Dark Matter in Nuclear Physics George Fuller (UCSD), Andrew Hime (LANL), Reyco Henning (UNC), Darin Kinion (LLNL), Spencer Klein (LBNL), Stefano Profumo (Caltech) Michael Ramsey-Musolf (Caltech/UW Madison), Robert Stokstad (LBNL) Introduction A transcendent accomplishment of nuclear physics and observational cosmology has been the definitive measurement of the baryon content of the universe. Big Bang Nucleosynthesis calculations, combined with measurements made with the largest new telescopes of the primordial deuterium abundance, have inferred the baryon density of the universe. This result has been confirmed by observations of the anisotropies in the Cosmic Microwave Background. The surprising upshot is that baryons account for only a small fraction of the observed mass and energy in the universe. It is now firmly established that most of the mass-energy in the Universe is comprised of non-luminous and unknown forms. One component of this is the so- called “dark energy”, believed to be responsible for the observed acceleration of the expansion rate of the universe. Another component appears to be composed of non-luminous material with non-relativistic kinematics at the current epoch. The relationship between the dark matter and the dark energy is unknown. Several national studies and task-force reports have found that the identification of the mysterious “dark matter” is one of the most important pursuits in modern science. It is now clear that an explanation for this phenomenon will require some sort of new physics, likely involving a new particle or particles, and in any case involving physics beyond the Standard Model. A large number of dark matter studies, from theory to direct dark matter particle detection, involve nuclear physics and nuclear physicists. -
Gammev: Fermilab Axion-Like Particle Photon Regeneration Results
GammeV: Fermilab Axion-like Particle Photon Regeneration Results William Wester Fermilab, MS222, Batavia IL, USA presented on behalf of the GammeV Collaboration DOI: http://dx.doi.org/10.3204/DESY-PROC-2008-02/wester william GammeV is an axion-like particle photon regeneration experiment conducted at Fermilab that employs the light shining through a wall technique. We obtain limits on the cou- pling of a photon to an axion-like particle that extend previous limits for both scalar and pseudoscalar axion-like particles in the milli-eV mass range. We are able to exclude the axion-like particle interpretation of the anomalous PVLAS 2006 result by more than 5 standard deviations. 1 Introduction The question, What are the particles that make up the dark matter of the universe?, is one of the most fundamental scientific questions today. Besides weakly interacting massive particles (WIMPs) such as neutralinos, axion-like particles or other weakly interacting sub-eV particles (WISPs) are highly motivated dark matter particle candidates since they have properties that might explain the cosmic abundance of dark matter. The milli-eV mass scale is of particular interest in modern particle physics since that mass scale may be constructed with a see-saw between the Planck and TeV mass scales, and may be related to neutrino mass differences, the dark energy density expressed in (milli-eV)4, and known dark matter candidates such as gravitinos and axion-like particles. In 2006, the PVLAS experiment reported [1] anomalous polarization effects in the presence of a magnetic field including polarization rotation and el- lipticity generation that could be interpreted as being mediated by an axion-like particle in the milli-eV mass range with a unexpectedly strong coupling to photons. -
Doubly Fed Induction Motor
© 2018 JETIR April 2018, Volume 5, Issue 4 www.jetir.org (ISSN-2349-5162) Doubly fed induction motor For speed control of motor 1 2 3 4 Rushikesh pandya , Hingrajiya jaydeep , Goswami rajan , Nandaniya hiral Sarvaiya kinjal5, 1 Assistant Professor 2, 3, 4, 5, students 1, 2, 3, 4, 5, Department of Electrical engineering Dr Subhash technical campus, junagadh, Gujarat, India Abstract—Doubly-fed electric machines are electric motors or electric generators where both the field magnet windings and armature windings are separately connected to equipment outside the machine. This is useful, for instance, for generators used in wind turbines. By feeding adjustable frequency AC power to the field windings, the magnetic field can be made to rotate, allowing variation in motor or generator speed. Index Terms—doubly fed induction motor, speed control, different regulator _____________________________________________________________________________________________________ I. INTRODUCTION a three-phase wound-rotor induction machine operates as a synchronous speed nS obtained during normal singly-fed synchronous machine when ac currents are fed into one set of operation. This is illustrated in Figure 8a. In this case, the windings and dc current is fed into the other set of windings. When resulting synchronous speed of the doubly-fed induction motor ac currents are fed into both the stator and rotor windings of a is equal to: three-phase wound-rotor induction machine, the machine also operates as a synchronous machine. In this situation, when the nS (DF) 120 × (fStator — fRotor) wound-rotor induction machine operates as a synchronous motor, it = is referred to as a doubly-fed induction motor since electrical NPoSe power from the power network is converted into mechanical power available at the machine shaft via both the stator and rotor Where nS (DF) is the synchronous speed of the windings of the machine.