Bibliographies thématiques / Axion and axion like particles

Littérature scientifique sur le sujet « Axion and axion like particles »

Auteur : Grafiati
Publié le 11 mars 2023

Créez une référence correcte selon les styles APA, MLA, Chicago, Harvard et plusieurs autres

Choisissez une source :

Sommaire

Consultez les listes thématiques d’articles de revues, de livres, de thèses, de rapports de conférences et d’autres sources académiques sur le sujet « Axion and axion like particles ».

À côté de chaque source dans la liste de références il y a un bouton « Ajouter à la bibliographie ». Cliquez sur ce bouton, et nous générerons automatiquement la référence bibliographique pour la source choisie selon votre style de citation préféré : APA, MLA, Harvard, Vancouver, Chicago, etc.

Vous pouvez aussi télécharger le texte intégral de la publication scolaire au format pdf et consulter son résumé en ligne lorsque ces informations sont inclues dans les métadonnées.

Articles de revues sur le sujet "Axion and axion like particles"

1

Massó, Eduard. « Axions and axion-like particles ». Nuclear Physics B - Proceedings Supplements 114 (février 2003) : 67–73. http://dx.doi.org/10.1016/s0920-5632(02)01893-5.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
2

Stadnik, Yevgeny V., et Victor V. Flambaum. « New atomic probes for dark matter detection : Axions, axion-like particles and topological defects ». Modern Physics Letters A 29, no 37 (4 décembre 2014) : 1440007. http://dx.doi.org/10.1142/s0217732314400070.

Texte intégral
Résumé :
We present a brief overview of recently proposed detection schemes for axion, axion-like pseudoscalar particle and topological defect dark matter. We focus mainly on the possibility of using atomic and molecular systems for dark matter detection. For axions and axion-like particles, these methods are complementary probes to ongoing photon–axion interconversion experiments and astrophysical observations. For topological defects, these methods are complementary to conventional astrophysical search schemes based on gravitational signatures.
Styles APA, Harvard, Vancouver, ISO, etc.
3

Caloni, Luca, Martina Gerbino, Massimiliano Lattanzi et Luca Visinelli. « Novel cosmological bounds on thermally-produced axion-like particles ». Journal of Cosmology and Astroparticle Physics 2022, no 09 (1 septembre 2022) : 021. http://dx.doi.org/10.1088/1475-7516/2022/09/021.

Texte intégral
Résumé :
Abstract We constrain the coupling of thermally-produced axion-like particles (here axions) with photons and gluons, using data from the cosmic microwave background (CMB) spectra and baryon acoustic oscillations. The axion possesses an explicit soft breaking mass term and it is produced thermally in the early Universe from either axion-photon or axion-gluon processes, accounting for the recent progresses in the field. We derive the most stringent bounds on the axion-gluon coupling to date on the mass range considered 10-4 ≲ ma / eV ≲ 100, superseding the current bounds from SN1987A. The bounds on the axion-photon coupling are competitive with the results from the CAST collaboration for the axion mass ma ≳ 3eV. We comment on the forecast reaches that will be available given the sensitivity of future CMB-S4 missions.
Styles APA, Harvard, Vancouver, ISO, etc.
4

Flambaum, V. V., H. B. Tran Tan, I. B. Samsonov, Y. V. Stadnik et D. Budker. « Resonant detection and production of axions with atoms ». International Journal of Modern Physics A 33, no 31 (10 novembre 2018) : 1844030. http://dx.doi.org/10.1142/s0217751x1844030x.

Texte intégral
Résumé :
The axions and axion-like particles can be detected via a resonant atomic or molecular transition induced by axion absorption. The signal obtained in this process is second order in the axion-electron interaction constant and hence small. In this chapter, it is demonstrated that this signal may become first order in the axion-electron interaction constant if we allow the interference between the axion-induced transition amplitude and the transition amplitude induced by the electromagnetic radiation. Additionally, we show that the conventional scheme of producing axions from photons in a magnetic field may be improved if the field is replaced by an atomic medium in which photons scattering off the atoms in the forward direction are transformed into axions.
Styles APA, Harvard, Vancouver, ISO, etc.
5

Yang, Qiaoli. « Axions/Axion-like particles and the CMB asymmetric dipole ». International Journal of Modern Physics D 24, no 13 (novembre 2015) : 1545009. http://dx.doi.org/10.1142/s0218271815450091.

Texte intégral
Résumé :
Axions and axion-like particles (ALPs) are very attractive dark matter candidates. In this review, we briefly investigate how the cosmological observations reveal the existence of dark matter and some unique properties of axions/(ALPs) which make them more interesting.
Styles APA, Harvard, Vancouver, ISO, etc.
6

Li, Chuang, Nick Houston, Tianjun Li, Qiaoli Yang et Xin Zhang. « A detailed exploration of the EDGES 21cm absorption anomaly and axion-induced cooling ». International Journal of Modern Physics D 30, no 06 (22 mars 2021) : 2150041. http://dx.doi.org/10.1142/s0218271821500413.

Texte intégral
Résumé :
The EDGES collaboration’s observation of an anomalously strong 21 cm absorption feature around the cosmic dawn era has energised the cosmological community by suggesting a novel signature of dark matter in the cooling of cosmic hydrogen. In a recent paper, we have argued that by virtue of the ability to mediate cooling processes whilst in the condensed phase, a small amount of axion dark matter can explain these observations within the context of Standard Models of axions and axion-like particles. These axions and axion-like particles (ALPs) can thermalise through gravitational self-interactions and so eventually form a Bose–Einstein condensate (BEC), whereupon large-scale long-range correlation can produce experimentally observable signals such as these. In this context, the EDGES best-fit result favours an ALP mass in the (6, 400) meV range. Future experiments and galaxy surveys, particularly the International Axion Observatory (IAXO) and EUCLID, should have the capability to directly test this scenario. In this paper, we will explore this mechanism in detail and give more thorough computational details of certain key points.
Styles APA, Harvard, Vancouver, ISO, etc.
7

Zhang, Hong. « Axion Stars ». Symmetry 12, no 1 (20 décembre 2019) : 25. http://dx.doi.org/10.3390/sym12010025.

Texte intégral
Résumé :
The dark matter particle can be a QCD axion or axion-like particle. A locally over-densed distribution of axions can condense into a bound Bose–Einstein condensate called an axion star, which can be bound by self-gravity or bound by self-interactions. It is possible that a significant fraction of the dark matter axion is in the form of axion stars. This would make some efforts searching for the axion as the dark matter particle more challenging, but at the same time it would also open up new possibilities. Some of the properties of axion stars, including their emission rates and their interactions with other astrophysical objects, are not yet completely understood.
Styles APA, Harvard, Vancouver, ISO, etc.
8

Avgoustidis, Anastasios. « New Cosmological Constraints on Axions and Axion-Like Particles ». Journal of Physics : Conference Series 283 (1 février 2011) : 012003. http://dx.doi.org/10.1088/1742-6596/283/1/012003.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
9

STEFFEN, JASON H., et AMOL UPADHYE. « THE GammeV SUITE OF EXPERIMENTAL SEARCHES FOR AXION-LIKE PARTICLES ». Modern Physics Letters A 24, no 26 (30 août 2009) : 2053–68. http://dx.doi.org/10.1142/s0217732309031727.

Texte intégral
Résumé :
We report on the design and results of the GammeV search for axion-like particles and for chameleon particles. We also discuss plans for an improved experiment to search for chameleon particles, one which is sensitive to both cosmological and power-law chameleon models. Plans for an improved axion-like particle search using coupled resonant cavities are also presented. This experiment will be more sensitive to axion-like particles than stellar astrophysical models or current helioscope experiments.
Styles APA, Harvard, Vancouver, ISO, etc.
10

Graham, Peter W., Igor G. Irastorza, Steven K. Lamoreaux, Axel Lindner et Karl A. van Bibber. « Experimental Searches for the Axion and Axion-Like Particles ». Annual Review of Nuclear and Particle Science 65, no 1 (19 octobre 2015) : 485–514. http://dx.doi.org/10.1146/annurev-nucl-102014-022120.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
Plus de sources

Thèses sur le sujet "Axion and axion like particles"

1

Cadamuro, Davide. « Cosmological limits on axions and axion-like particles ». Diss., lmu, 2012. http://nbn-resolving.de/urn:nbn:de:bvb:19-149191.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
2

Day, Francesca. « Astrophysical signatures of axion-like particles ». Thesis, University of Oxford, 2017. https://ora.ox.ac.uk/objects/uuid:215f6432-6dbb-4a16-80d8-3ad0bc76ec2d.

Texte intégral
Résumé :
The Standard Model of particle physics has enjoyed unprecedented success in predicting experimental results. However, evidence from astrophysical observations points to the existence of a dark sector of particles that interact only very weakly with the Standard Model. In this work, we search for dark sector signatures in X-ray telescope data. Much of this work concerns a class of hypothetical particles, the axion-like particle (ALP). ALPs are a theoretically well-motivated extension of the Standard Model. If ALPs exist, they may lead to intriguing astrophysical signatures: in the presence of a background magnetic field, ALPs and photons can interconvert. We could detect ALPs by searching for photon to ALP conversion. For example, photons produced by point sources in or behind galaxy clusters may convert to ALPs in the cluster's magnetic field. This could lead to observable spectral anomalies. Using this strategy, we place world leading bounds on the ALP-photon coupling. One potential signal of dark matter is an anomalous line in the spectra of galaxies and galaxy clusters. In 2014, an anomalous line was found at an energy of 3.5 keV. The nature and cause of this line is still under discussion. We analyse a scenario in which the 3.5 keV line arises from dark matter decay to ALPs, which interconvert with 3.5 keV photons in astrophysical magnetic fields. We further report an anomalous deficit at 3.5 keV in the spectrum of the Active Galactic Nucleus at the centre of the Perseus galaxy cluster. This motivates the study of a new model in which both features are caused by “fluorescent dark matter” which resonantly interacts with 3.5 keV photons. We analyse observations of Perseus at 3.5 keV to date, and show that they are well explained by this model. Further theoretical and experimental work is needed to discover or exclude fundamental physics effects in X-ray spectra.
Styles APA, Harvard, Vancouver, ISO, etc.
3

Shaul, Diana Naomi April. « Searching for WIMPs and axion-like particles ». Thesis, Imperial College London, 1996. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.244125.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
4

Cadamuro, Davide [Verfasser], et Georg [Akademischer Betreuer] Raffelt. « Cosmological limits on axions and axion-like particles / Davide Cadamuro. Betreuer : Georg Raffelt ». München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2012. http://d-nb.info/1027669298/34.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
5

Powell, Andrew James. « The cosmology and astrophysics of axion-like particles ». Thesis, University of Oxford, 2016. https://ora.ox.ac.uk/objects/uuid:bbbb3cbc-a0ba-4024-86b0-c720d8104270.

Texte intégral
Résumé :
In this thesis I study astrophysical and cosmological effects of axion-like particles (ALPs). ALPs are pseudo-scalar particles, which are generally very weakly-interacting, with a coupling α/M E · B to electromagnetism. They are predicted by many theories which extend the standard model (SM) of particle physics, most notably string theory. String theory compactifications also predict many scalar fields called moduli which describe the size and shape of the extra, compact dimensions. In string theory models generically the moduli fields are responsible for reheating the universe after inflation. Being gravitationally-coupled, they will also decay to any other particles or sectors of the theory, including any light ALPs, of which there are usually many. The ALPs produced by moduli decay will contribute to dark radiation, additional relativistic energy density. The amount of dark radiation is tightly constrained by observations, this bounds the branching fraction of moduli decays into ALPs, which constrains the string theory model itself. I calculate the amount of dark radiation produced in a model with one light modulus, solely responsible for reheating, called the Large Volume Scenario. I study a minimal version of this model with one ALP and a visible sector comprised of the minimal supersymmetric SM. The dominant visible sector decay mode is to two Higgses, I include radiative corrections to this decay and find that ALP dark radiation is over-produced in this minimal version of the model, effectively ruling it out. The production of ALPs from moduli decay at reheating seems to be a generic feature of string theory models. These ALPs would exist today as a homogeneous cosmic ALP background (CAB). The coupling of ALPs to electromagnetism allows ALPs to convert to photons and vice versa in a magnetic field, leading to potential observable astrophysical signals of this CAB. Observations have shown an excess in soft X-ray emission from many galaxy clusters. I use detailed simulations of galaxy cluster magnetic fields to show that a CAB can explain these observations by conversion of ALPs into X-ray photons. I simulate ALP-photon conversion in four galaxy clusters and compare to soft X-ray observations. I show the excesses (or lack thereof) can be fit consistently across the clusters for a CAB with ALP-photon inverse coupling of M = 6 - 12 x 10¹² GeV, if the CAB spectrum has energy ~ 200 eV. I also study the possibility of using galaxy clusters to search for and constrain the ALP coupling to photons using cluster X-ray emission. Conversion of X-ray photons into ALPs will cause spectral distortions to the thermal X-ray spectrum emitted by galaxy clusters. I show that the non-observation of these distortions is able to produce the strongest constraints to date on the ALP-photon inverse coupling, M ≳ 7 x 10¹¹ GeV.
Styles APA, Harvard, Vancouver, ISO, etc.
6

Guidetti, Veronica <1991&gt. « Axion-like particles and inflation from String Theory ». Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amsdottorato.unibo.it/9586/1/guidetti_veronica_tesi.pdf.

Texte intégral
Résumé :
This thesis is focused on cosmological applications of the 4D Effective Field Theory (EFT) coming from type IIB string theory. We focus in particular on model building in inflation, dark matter and dark radiation using Kaehler moduli and axion-like fields which are ubiquitous features of type IIB flux compactifications. These fields enjoy effective approximate symmetries which can protect their potential against quantum corrections. This property makes both of them good inflaton candidates and implies that axion-like particles from string theory tend naturally to be very light with intriguing applications to dark radiation and dark matter. We first consider a class of type IIB inflationary models called "Fibre Inflation" where the inflaton is a Kaehler modulus. We provide a consistent global embedding of these models into Calabi-Yau orientifolds with D-branes, fluxes and a chiral visible sector. We also analyse the multi-field dynamics of this class of models, including both Kaehler moduli and axion-like particles which give rise to isocurvature perturbations. We then focus on different applications of axion-like particles coming from string theory. Depending on the value of their mass and decay constant, together with their production mechanism, these particles can drive inflation or can represent a non-negligible component of dark matter and dark radiation. We provide a string embedding of a model that explains the 3.5 keV line recently detected from galaxy clusters by exploting axion-photon conversion in astrophysical magnetic fields. Finally, we analyse the mechanisms of electro-magnetic dissipation in models where the inflaton is an axion, finding a new resonant behaviour in the gauge field production that affects the shape of the cosmological parameters.
Styles APA, Harvard, Vancouver, ISO, etc.
7

Lu, Bin. « Search for axion-like particles in the slac beam dump ». Diss., Virginia Polytechnic Institute and State University, 1987. http://hdl.handle.net/10919/49852.

Texte intégral
Résumé :
A search for axion-like particles was made at the Stanford Linear Accelerator Center (SLAC) by dumping 30 Coulombs of 20 GeV electrons into a beam absorption facility. After 179 meters of earth shielding the in-flight decay of the particle into two photons or an electron-positron pair, in a decay volume of 204 meters in length, was searched for with a fine-grained electromagnetic calorimeter. No positive signals were identified. Experimental limits were obtained for axions of mass up to ~ 200 MeV/c², and photinos of mass up to ~ 65 MeV/c².
Ph. D.
incomplete_metadata
Styles APA, Harvard, Vancouver, ISO, etc.
8

Guidetti, Veronica. « Axion-like particles and the 3.5 keV line in 4D string models ». Master's thesis, Alma Mater Studiorum - Università di Bologna, 2016. http://amslaurea.unibo.it/10346/.

Texte intégral
Résumé :
This work is focused on axions and axion like particles (ALPs) and their possible relation with the 3.55 keV photon line detected, in recent years, from galaxy clusters and other astrophysical objects. We focus on axions that come from string compactification and we study the vacuum structure of the resulting low energy 4D N=1 supergravity effective field theory. We then provide a model which might explain the 3.55 keV line through the following processes. A 7.1 keV dark matter axion decays in two light axions, which, in turn, are transformed into photons thanks to the Primakoff effect and the existence of a kinetic mixing between two U(1)s gauge symmetries belonging respectively to the hidden and the visible sector. We present two models, the first one gives an outcome inconsistent with experimental data, while the second can yield the desired result.
Styles APA, Harvard, Vancouver, ISO, etc.
9

Almeida, Raquel Malta Nunes de. « Study of axion-like particles signals at the Cherenkov Telescope Array ». reponame:Repositório Institucional da UFABC, 2018.

Trouver le texte intégral
Résumé :
Orientador: Prof. Dr. Marcelo Augusto Leigui de Oliveira
Dissertação (mestrado) - Universidade Federal do ABC, Programa de Pós-Graduação em Física, Santo André, 2018.
O objetivo deste trabalho é discutir a distorção do fluxo de raios gama de altas energias (250 GeV ¿ 25 TeV) devido a processos de atenuação desde a fonte até sua chegada na Via Lactea. Entre esses processos estão a produção de pares pela interação com a radiação cósmica de fundo, principalmente EBL, e a oscilação de fótons em bosons pseudoescalares leves, chamados de partículas tipo áxion (ALPs). Também é discutido como será o sinal do fluxo detectado pelo Cherenkov Telescope Array, explicitando suas especificações técnicas e principais melhorias em relação aos detectores atuais, o que nos levará a uma nova geração de telescópios de raios gama.
The purpose of this research is to discuss the distortion of VHE gamma-ray flux (250 GeV - 25 TeV) due to attenuation processes along its path from the source to our galaxy, namely: pair production as a result of the interaction with the background cosmic radiation, especially EBL, and gamma-ray mix with a light pseudoescalar fundamental boson called axion-like particle (ALP). It is also discussed how this signal should appear at Cherenkov Telescope Array, emphasizing its technical specifications and major improvements over current IACTs, which will lead us to a new generation of gamma-ray telescopes.
Styles APA, Harvard, Vancouver, ISO, etc.
10

Eby, Joshua. « Phenomenology and Astrophysics of Gravitationally-Bound Condensates of Axion-Like Particles ». University of Cincinnati / OhioLINK, 2017. http://rave.ohiolink.edu/etdc/view?acc_num=ucin1504868633515325.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
Plus de sources

Chapitres de livres sur le sujet "Axion and axion like particles"

1

Fortin, Jean-François, et Kuver Sinha. « Axion-Like Particles, Magnetars, and X-ray Astronomy ». Dans Quantum Theory and Symmetries, 569–75. Cham : Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-55777-5_53.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
2

Chudasama, Ruchi. « Observation of Light-by-Light Scattering and Search for Axion-Like Particles with CMS Experiment ». Dans Springer Proceedings in Physics, 473–77. Singapore : Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-19-2354-8_87.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
3

Jackson Kimball, Derek F., Leanne D. Duffy et David J. E. Marsh. « Ultralight Bosonic Dark Matter Theory ». Dans The Search for Ultralight Bosonic Dark Matter, 31–72. Cham : Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-95852-7_2.

Texte intégral
Résumé :
AbstractThe basic theoretical concepts motivating the hypothesis that dark matter may consist of ultralight spin-0 or spin-1 bosons are explored. The origin of bosons with masses ≪ 1 eV from spontaneous and explicit symmetry breaking is illustrated with examples. The origins and characteristics of nongravitational couplings or “portals” between ultralight bosons and Standard Model particles and fields are considered, with particular attention paid to the cases of the axion-photon and axion-fermion interactions. Theoretical motivations for the existence of ultralight bosons, besides as an explanation of dark matter, are examined, with particular focus on the Peccei-Quinn solution to the strong CP problem (resulting in the QCD axion) and a dynamical solution to the hierarchy problem (the “relaxion” hypothesis, based on a particular axion-Higgs coupling in the early universe). Mechanisms for non-thermal production of ultralight bosonic dark matter are examined.
Styles APA, Harvard, Vancouver, ISO, etc.
4

Dienes, Keith R. « Particles in the Bulk : A Higher-Dimensional Approach to Neutrino and Axion Phenomenology ». Dans Dark Matter in Astro- and Particle Physics, 234–46. Berlin, Heidelberg : Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-642-56643-1_22.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
5

Geraci, Andrew A., et Yun Chang Shin. « Laboratory Searches for Exotic Spin-Dependent Interactions ». Dans The Search for Ultralight Bosonic Dark Matter, 219–53. Cham : Springer International Publishing, 2012. http://dx.doi.org/10.1007/978-3-030-95852-7_8.

Texte intégral
Résumé :
AbstractThe possible existence of exotic spin-dependent interactions with ranges from the subatomic scale to astrophysical scales has been of great theoretical interest for the last few decades. Typically, these exotic interactions are mediated by ultralight bosons with very weak coupling strength. If they indeed exist, such long-range interactions would indicate new physics beyond the Standard Model. A wide variety of experimental tests have been made to search for novel long-range spin-dependent interactions. Most experimental searches have focused on monopole-dipole or dipole-dipole interactions that could be induced by the exchange of ultralight bosons such as axions or axionlike particles. These ultralight bosons could also provide an answer to some of the most challenging problems in modern particle physics and astronomy: for example, the strong-CP problem in quantum chromodynamics (QCD), where C represents the charge conjugate symmetry and P represents the parity symmetry, and the explanation of dark matter and dark energy. In this chapter, we discuss the theoretical motivations as well as experimental searches for exotic spin-dependent interactions mediated by ultralight bosons in recent decades. We also introduce ongoing experimental efforts, such as Axion Resonant InterAction DetectioN Experiment (ARIADNE) and the QUest for AXion (QUAX)-gsgp experiment. The high sensitivities of these tests will allow vast expansion of the discovery potential for exotic spin-dependent interactions.
Styles APA, Harvard, Vancouver, ISO, etc.
6

Marsh, David J. E., et Sebastian Hoof. « Astrophysical Searches and Constraints ». Dans The Search for Ultralight Bosonic Dark Matter, 73–122. Cham : Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-95852-7_3.

Texte intégral
Résumé :
AbstractStarting from the evidence that dark matter (DM) indeed exists and permeates the entire cosmos, various bounds on its properties can be estimated. Beginning with the cosmic microwave background and large-scale structure, we summarize bounds on the ultralight bosonic dark matter (UBDM) mass and cosmic density. These bounds are extended to larger masses by considering galaxy formation and evolution and the phenomenon of black hole superradiance. We then discuss the formation of different classes of UBDM compact objects including solitons/axion stars and miniclusters. Next, we consider astrophysical constraints on the couplings of UBDM to Standard Model particles, from stellar cooling (production of UBDM) and indirect searches (decays or conversion of UBDM). Throughout, there are short discussions of “hints and opportunities” in searching for UBDM in each area.
Styles APA, Harvard, Vancouver, ISO, etc.
7

« Axions and Axion-like Particles as Dark Matter ». Dans An Introduction to Particle Dark Matter, 147–66. WORLD SCIENTIFIC (EUROPE), 2017. http://dx.doi.org/10.1142/9781786340023_0007.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
8

CHU, P. H. « LABORATORY SEARCH FOR SPIN-DEPENDENT SHORT-RANGE FORCE FROM AXION-LIKE PARTICLES USING OPTICALLY POLARIZED 3HE GAS ». Dans CPT and Lorentz Symmetry, 232–35. WORLD SCIENTIFIC, 2014. http://dx.doi.org/10.1142/9789814566438_0058.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
9

De Rújula, Alvaro. « Today’s Standard Models of Particles and Gravity ». Dans Enjoy Our Universe, 129–31. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198817802.003.0023.

Texte intégral
Résumé :
The missing particle of the standard model: the “axion.” Our considerable ignorance concerning dark matter and the dark energy density of the Universe. No decent theory of quantum gravity. How all this sends us back to the drawing board, and to return to observations of the Universe, starting with Hubble’s law of its expansion.
Styles APA, Harvard, Vancouver, ISO, etc.
10

De Rújula, Alvaro. « Limitations and Peculiarities of the Standard Models ». Dans Enjoy Our Universe, 160–61. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198817802.003.0030.

Texte intégral
Résumé :
Back to how peculiar the recipe to cook an inflationary universe is, with its mysterious cosmological constant and dark matter components. The arbitrary parameters of the Standard Model of particles are also many, and one of its predictions (the axion particle) still escapes detection. CERN’s CAST experiment, looking for—with no success—axions that the Sun could be emitting.
Styles APA, Harvard, Vancouver, ISO, etc.

Actes de conférences sur le sujet "Axion and axion like particles"

1

Di Vecchia, Paolo, Maurizio Giannotti, Massimiliano Lattanzi et Axel Lindner. « Round Table on Axions and Axion-like Particles ». Dans XIII Quark Confinement and the Hadron Spectrum. Trieste, Italy : Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.336.0034.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
2

Kowalczyk, Elizabeth, et Nikita Blinov. « Simulation of Axion-like Particles at DarkQuest ». Dans Simulation of Axion-like Particles at DarkQuest. US DOE, 2020. http://dx.doi.org/10.2172/1648542.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
3

ZIOUTAS, K., Y. SEMERTZIDIS et TH PAPAEVANGELOU. « OVERLOOKED ASTROPHYSICAL SIGNATURES OF AXION(-LIKE) PARTICLES ». Dans Proceedings of the Sixth International Workshop. WORLD SCIENTIFIC, 2007. http://dx.doi.org/10.1142/9789812770288_0050.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
4

Laha, Ranjan. « Diffuse axion-like particle searches ». Dans Neutrino Oscillation Workshop. Trieste, Italy : Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.337.0091.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
5

Schmieden, Kristof. « Searches for Axion Like Particles at the LHC ». Dans The Ninth Annual Conference on Large Hadron Collider Physics. Trieste, Italy : Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.397.0005.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
6

Papoulias, Dimitrios, D. Aristizabal Sierra, V. De Romeri et L. J. Flores. « Probing axion-like particles with reactor neutrino experiments ». Dans The 22nd International Workshop on Neutrinos from Accelerators. Trieste, Italy : Sissa Medialab, 2022. http://dx.doi.org/10.22323/1.402.0090.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
7

Meyer, Manuel, et Dieter Horns. « Impact of axion-like particles on observations with IACTs ». Dans The European Physical Society Conference on High Energy Physics. Trieste, Italy : Sissa Medialab, 2014. http://dx.doi.org/10.22323/1.180.0406.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
8

MANOUSOS, Athanasios, A. Liolios et C. Eleftheriadis. « Energetic axion-like particle production in galaxies ». Dans Identification of Dark Matter 2010. Trieste, Italy : Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.110.0034.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
9

Nguyen, Federico, Mariano Carpanese, Giuseppe Dattoli et Alberto Petralia. « PROPOSAL TO SEARCH FOR AXION-LIKE PARTICLES WITH FEL OSCILLATORS ». Dans Nineteenth Lomonosov Conference on Elementary Particle Physics. WORLD SCIENTIFIC, 2021. http://dx.doi.org/10.1142/9789811233913_0052.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
10

YOO, JONGHEE. « The FIRST RESULTS OF THE GammeV AXION-LIKE PARTICLES SEARCH EXPERIMENT ». Dans Proceedings of the 6th International Heidelberg Conference. WORLD SCIENTIFIC, 2008. http://dx.doi.org/10.1142/9789812814357_0050.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.

Rapports d'organisations sur le sujet "Axion and axion like particles"

1

Eby, Joshua Armstrong. Phenomenology and Astrophysics of Gravitationally-Bound Condensates of Axion-Like Particles. Office of Scientific and Technical Information (OSTI), janvier 2017. http://dx.doi.org/10.2172/1408206.

Texte intégral
Styles APA, Harvard, Vancouver, ISO, etc.
Vous pouvez également être intéressé par les bibliographies sur le sujet « Axion and axion like particles » pour d’autres types de sources :
Articles de revues Thèses
Nous offrons des réductions sur tous les plans premium pour les auteurs dont les œuvres sont incluses dans des sélections littéraires thématiques. Contactez-nous pour obtenir un code promo unique!

Vers la bibliographie