Zobrazeno 1 - 6
of 6
pro vyhledávání: '"axion, oscillation"'
Publikováno v:
INSPIRE-HEP
A leading direction in the hunt for axion dark matter is to search for its influence on nuclear spins. The detection scheme involves polarizing a sample of nuclei within a strong static magnetic field and then looking for a spin precession induced by
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0860b6ae4b2355e9a3872a16ffb41cc
http://arxiv.org/abs/2210.06481
http://arxiv.org/abs/2210.06481
A leading direction in the hunt for axion dark-matter is to search for its influence on nuclear spins. The detection scheme involves polarizing a sample of nuclei within a strong static magnetic field and then looking for a spin precession induced by
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a006b45dc7f8411d186e09b5f73eb87a
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2021, 104 (11), pp.L111701. ⟨10.1103/PhysRevD.104.L111701⟩
Physical Review
Phys.Rev.D, 2021, 104 (11), pp.L111701. ⟨10.1103/PhysRevD.104.L111701⟩
Physical Review
We propose a new broadband search strategy for ultralight axion dark matter that interacts with electromagnetism. An oscillating axion field induces transitions between two quasi-degenerate resonant modes of a superconducting cavity. In two broadband
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2ad7ffcd0a6c60a3dc786e87fef3d89b
http://arxiv.org/abs/2007.15656
http://arxiv.org/abs/2007.15656
Publikováno v:
Physical Review D
Physical Review D, American Physical Society, 2018, 97 (8), pp.083502. ⟨10.1103/PhysRevD.97.083502⟩
Phys.Rev.D
Phys.Rev.D, 2018, 97 (8), pp.083502. ⟨10.1103/PhysRevD.97.083502⟩
Phys.Rev.D, 2018, 97 (8), pp.083502. 〈10.1103/PhysRevD.97.083502〉
Physical Review D, American Physical Society, 2018, 97 (8), pp.083502. ⟨10.1103/PhysRevD.97.083502⟩
Phys.Rev.D
Phys.Rev.D, 2018, 97 (8), pp.083502. ⟨10.1103/PhysRevD.97.083502⟩
Phys.Rev.D, 2018, 97 (8), pp.083502. 〈10.1103/PhysRevD.97.083502〉
If the symmetry breaking responsible for axion dark matter production occurs during the radiation-dominated epoch in the early Universe, then this produces large amplitude perturbations that collapse into dense objects known as axion miniclusters. Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d5513629ebf3c7a6d1c6587a0621408
https://hal.archives-ouvertes.fr/hal-01768113
https://hal.archives-ouvertes.fr/hal-01768113
Coherent oscillation of axions or axion-like particles may give rise to long-lived clumps, called axion stars, because of the attractive gravitational force or its self-interaction. Such a kind of configuration has been extensively studied in the con
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::416edf8cd3a439795ae0b0e2b8a1cd15
Publikováno v:
JCAP
JCAP, 2017, 12, pp.042. ⟨10.1088/1475-7516/2017/12/042⟩
JCAP, 2017, 12 (12), pp.042. 〈10.1088/1475-7516/2017/12/042〉
JCAP, 2017, 12, pp.042. ⟨10.1088/1475-7516/2017/12/042⟩
JCAP, 2017, 12 (12), pp.042. 〈10.1088/1475-7516/2017/12/042〉
We revisit the generation of dark matter isocurvature perturbations in the curvaton model in greater detail, both analytically and numerically. As concrete examples, we investigate the cases of thermally decoupled dark matter and axionic dark matter.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::16ca3f102bd34264f349b3f63ca227c1