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Nature
Resumen/Descripción – provisto por la editorial en inglés
Nature is a weekly international journal publishing the finest peer-reviewed research in all fields of science and technology on the basis of its originality, importance, interdisciplinary interest, timeliness, accessibility, elegance and surprising conclusions. Nature also provides rapid, authoritative, insightful and arresting news and interpretation of topical and coming trends affecting science, scientists and the wider public.Palabras clave – provistas por la editorial
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Disponibilidad
Institución detectada | Período | Navegá | Descargá | Solicitá |
---|---|---|---|---|
No detectada | desde jul. 2012 / hasta dic. 2023 | Nature.com | ||
No detectada | desde jul. 2006 / hasta ago. 2012 | Ovid |
Información
Tipo de recurso:
revistas
ISSN impreso
0028-0836
ISSN electrónico
1476-4687
Editor responsable
Springer Nature
País de edición
Reino Unido
Fecha de publicación
1869-
Tabla de contenidos
Early-career satisfaction: industry beats academia
Shusheng Geng
Palabras clave: Multidisciplinary.
Pp. 33-33
COVID-19: LMICs need antivirals as well as vaccines
Simar Singh Bajaj; Fatima Cody Stanford
Palabras clave: Multidisciplinary.
Pp. 33-33
A subset of immune-system T cells branded as seeds for type 1 diabetes
Stephen J. Turner; Nicole L. La Gruta
Palabras clave: Multidisciplinary.
Pp. 35-36
Lost magnetism pinned on atomic rotations
Georg Woltersdorf
Palabras clave: Multidisciplinary.
Pp. 36-38
Important genomic regions mutate less often than do other regions
Jianzhi Zhang
Palabras clave: Multidisciplinary.
Pp. 38-39
Search for single magnetic charges in the largest of fields
Sonia Kabana
Palabras clave: Multidisciplinary.
Pp. 39-40
Reproducibility in the fabrication and physics of moiré materials
Chun Ning Lau; Marc W. Bockrath; Kin Fai Mak; Fan Zhang
Palabras clave: Multidisciplinary.
Pp. 41-50
An open science study of ageing in companion dogs
Kate E. Creevy; Joshua M. Akey; Matt Kaeberlein; Daniel E. L. Promislow; Brian G. Barnett; Brooke Benton; Elhanan Borenstein; Marta G. Castelhano; Lucy Chou; Devin Collins; Amanda E. Coleman; Kyle Crowder; Matthew D. Dunbar; Jeremy Evans; Virginia R. Fajt; Annette L. Fitzpatrick; Unity Jeffery; Erica C. Jonlin; Elinor K. Karlsson; Kathleen F. Kerr; Hannah Lee; Jonathan M. Levine; Jing Ma; Robyn L. McClelland; Kellyn E. McNulty; Kathleen Morrill; Yunbi Nam; Audrey Ruple; Stephen M. Schwartz; Sandi Shrager; Noah Snyder-Mackler; William Thistlethwaite; Amanda K. Tinkle; M. Katherine Tolbert; Silvan R. Urfer; Benjamin S. Wilfond;
Palabras clave: Multidisciplinary.
Pp. 51-57
Microwave background temperature at a redshift of 6.34 from H2O absorption
Dominik A. Riechers; Axel Weiss; Fabian Walter; Christopher L. Carilli; Pierre Cox; Roberto Decarli; Roberto Neri
<jats:title>Abstract</jats:title><jats:p>Distortions of the observed cosmic microwave background provide a direct measurement of the microwave background temperature at redshifts from 0 to 1 (refs. <jats:sup>1,2</jats:sup>). Some additional background temperature estimates exist at redshifts from 1.8 to 3.3 based on molecular and atomic line-excitation temperatures in quasar absorption-line systems, but are model dependent<jats:sup>3</jats:sup>. No deviations from the expected (1 + <jats:italic>z</jats:italic>) scaling behaviour of the microwave background temperature have been seen<jats:sup>4</jats:sup>, but the measurements have not extended deeply into the matter-dominated era of the Universe at redshifts <jats:italic>z</jats:italic> > 3.3. Here we report observations of submillimetre line absorption from the water molecule against the cosmic microwave background at <jats:italic>z</jats:italic> = 6.34 in a massive starburst galaxy, corresponding to a lookback time of 12.8 billion years (ref. <jats:sup>5</jats:sup>). Radiative pumping of the upper level of the ground-state ortho-H<jats:sub>2</jats:sub>O(1<jats:sub>10</jats:sub>–1<jats:sub>01</jats:sub>) line due to starburst activity in the dusty galaxy HFLS3 results in a cooling to below the redshifted microwave background temperature, after the transition is initially excited by the microwave background. This implies a microwave background temperature of 16.4–30.2 K (1<jats:italic>σ</jats:italic> range) at <jats:italic>z</jats:italic> = 6.34, which is consistent with a background temperature increase with redshift as expected from the standard ΛCDM cosmology<jats:sup>4</jats:sup>.</jats:p>
Palabras clave: Multidisciplinary.
Pp. 58-62
Search for magnetic monopoles produced via the Schwinger mechanism
B. Acharya; J. Alexandre; P. Benes; B. Bergmann; S. Bertolucci; A. Bevan; H. Branzas; P. Burian; M. Campbell; Y. M. Cho; M. de Montigny; A. De Roeck; J. R. Ellis; M. El Sawy; M. Fairbairn; D. Felea; M. Frank; O. Gould; J. Hays; A. M. Hirt; D. L.-J. Ho; P. Q. Hung; J. Janecek; M. Kalliokoski; A. Korzenev; D. H. Lacarrère; C. Leroy; G. Levi; A. Lionti; A. Maulik; A. Margiotta; N. Mauri; N. E. Mavromatos; P. Mermod; L. Millward; V. A. Mitsou; I. Ostrovskiy; P.-P. Ouimet; J. Papavassiliou; B. Parker; L. Patrizii; G. E. Păvălaş; J. L. Pinfold; L. A. Popa; V. Popa; M. Pozzato; S. Pospisil; A. Rajantie; R. Ruiz de Austri; Z. Sahnoun; M. Sakellariadou; A. Santra; S. Sarkar; G. Semenoff; A. Shaa; G. Sirri; K. Sliwa; R. Soluk; M. Spurio; M. Staelens; M. Suk; M. Tenti; V. Togo; J. A. Tuszyn’ski; A. Upreti; V. Vento; O. Vives
Palabras clave: Multidisciplinary.
Pp. 63-67