Search: onr:"swepub:oai:DiVA.org:kth-304299" > Axion quasiparticle...
Fältnamn | Indikatorer | Metadata |
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000 | 04974naa a2200565 4500 | |
001 | oai:DiVA.org:kth-304299 | |
003 | SwePub | |
008 | 211101s2021 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-199134 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3042992 URI |
024 | 7 | a https://doi.org/10.1088/1475-7516/2021/08/0662 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1991342 URI |
040 | a (SwePub)kthd (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Schuette-Engel, Janu Univ Illinois, Dept Phys, Urbana, IL 61801 USA.;Univ Illinois, Illinois Ctr Adv Studies Universe, Urbana, IL 61801 USA.;Hamburg Univ, D-22761 Hamburg, Germany.4 aut |
245 | 1 0 | a Axion quasiparticles for axion dark matter detection |
264 | c 2021-08-31 | |
264 | 1 | b IOP Publishing Ltd,c 2021 |
338 | a print2 rdacarrier | |
500 | a QC 20220615 | |
520 | a It has been suggested that certain antiferromagnetic topological insulators contain axion quasiparticles (AQs), and that such materials could be used to detect axion dark matter (DM). The AQ is a longitudinal antiferromagnetic spin fluctuation coupled to the electromagnetic Chern-Simons term, which, in the presence of an applied magnetic field, leads to mass mixing between the AQ and the electric field. The electromagnetic boundary conditions and transmission and reflection coefficients are computed. A model for including losses into this system is presented, and the resulting linewidth is computed. It is shown how transmission spectroscopy can be used to measure the resonant frequencies and damping coefficients of the material, and demonstrate conclusively the existence of the AQ. The dispersion relation and boundary conditions permit resonant conversion of axion DM into THz photons in a material volume that is independent of the resonant frequency, which is tuneable via an applied magnetic field. A parameter study for axion DM detection is performed, computing boost amplitudes and bandwidths using realistic material properties including loss. The proposal could allow for detection of axion DM in the mass range between 1 and 10 meV using current and near future technology. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysikx Subatomär fysik0 (SwePub)103012 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Subatomic Physics0 (SwePub)103012 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a axions | |
653 | a dark matter detectors | |
653 | a dark matter theory | |
653 | a dark matter experiments | |
700 | 1 | a Marsh, David J. E.u Georg August Univ Gottingen, Inst Astrophys, Friedrich Hund Pl 1, D-37077 Gottingen, Germany.4 aut |
700 | 1 | a Millar, Alexander J.u Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC),Nordiska institutet för teoretisk fysik (Nordita),Stockholm Univ, Oskar Klein Ctr Cosmoparticle Phys, Dept Phys, AlbaNova, S-10691 Stockholm, Sweden.Nordita SU4 aut0 (Swepub:su)almi8159 |
700 | 1 | a Sekine, Akihikou RIKEN, Ctr Emergent Matter Sci, Wako, Saitama 3510198, Japan.4 aut |
700 | 1 | a Chadha-Day, Francescau Univ Durham, Dept Phys, South Rd, Durham DH1 3LE, England.4 aut |
700 | 1 | a Hoof, Sebastianu Georg August Univ Gottingen, Inst Astrophys, Friedrich Hund Pl 1, D-37077 Gottingen, Germany.4 aut |
700 | 1 | a Ali, Mazhar N.u Max Planck Inst Microstruct Phys, Weinberg 2, D-06120 Halle, Germany.;Delft Univ Technol, Kavli Inst Nanosci, Delft, Netherlands.4 aut |
700 | 1 | a Fong, Kin Chungu Raytheon BBN Technol Quantum Engn & Comp, Cambridge, MA 02138 USA.4 aut |
700 | 1 | a Hardy, Edwardu Univ Liverpool, Math Sci, Liverpool L69 7ZL, Merseyside, England.4 aut |
700 | 1 | a Smejkal, Liboru Johannes Gutenberg Univ Mainz, Inst Phys, D-55128 Mainz, Germany.;Czech Acad Sci, Inst Phys, Cukrovarnicka 10, Prague 16200 6, Czech Republic.4 aut |
710 | 2 | a Univ Illinois, Dept Phys, Urbana, IL 61801 USA.;Univ Illinois, Illinois Ctr Adv Studies Universe, Urbana, IL 61801 USA.;Hamburg Univ, D-22761 Hamburg, Germany.b Georg August Univ Gottingen, Inst Astrophys, Friedrich Hund Pl 1, D-37077 Gottingen, Germany.4 org |
773 | 0 | t Journal of Cosmology and Astroparticle Physicsd : IOP Publishing Ltdg :8q :8x 1475-7516 |
856 | 4 | u http://arxiv.org/pdf/2102.05366 |
856 | 4 | u https://arxiv.org/abs/2102.05366y arXiv:2102.05366 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-304299 |
856 | 4 8 | u https://doi.org/10.1088/1475-7516/2021/08/066 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-199134 |
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