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Objective Axial spondyloarthritis (axSpA) is often associated with persistent pain despite effective anti‐inflammatory treatment. Digital health applications (DHAs) provide innovative approaches to address multidimensional aspects of persistent pain through psychological and behavioral strategies. The aim of this study was to assess the impact of a DHA
David Kiefer +7 more
wiley +1 more source
Black Holes as Laboratories: Tests of General Relativity. [PDF]
Gregory R, Nissanke S.
europepmc +1 more source
Neutron capture measurements for s-process nucleosynthesis: A review about CERN n_TOF developments and contributions. [PDF]
Domingo-Pardo C +145 more
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The <sup>22</sup>Ne( α ,n)<sup>25</sup>Mg reaction - state of the art, astrophysics, and perspectives. [PDF]
Best A +13 more
europepmc +1 more source
Stellar occultations: a gateway to advances in planetary science. [PDF]
Souami D +3 more
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Fine-tunings in nucleosynthesis and the emergence of life: status and perspectives. [PDF]
Meißner UG, Metsch BC, Meyer H.
europepmc +1 more source
Terrestrial atmospheric ion implantation occurred in the nearside lunar regolith during the history of Earth's dynamo. [PDF]
Paramanick S +3 more
europepmc +1 more source
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Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures
Nature Astronomy, 2021While most of the compact-binary mergers detected by LIGO and Virgo are expected to consist of first-generation black holes formed from the collapse of stars, others might instead be of second (or higher) generation, containing the remnants of previous ...
D. Gerosa, M. Fishbach
semanticscholar +1 more source
Formation Channels of Single and Binary Stellar-Mass Black Holes
Handbook of Gravitational Wave Astronomy, 2021These are exciting times for binary black hole (BBH) research. LIGO and Virgo detections are progressively drawing a spectacular fresco of BBH masses, spins and merger rates.
M. Mapelli
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1989
We have seen that a careful analysis of a star’s spectrum reveals the chemical and physical characteristics of its atmosphere, but the spectrum tells us very little about its deep interior. It gives us only the total amount of radiation emitted per second by the star; it tells us nothing about the generation and transport of this radiation through the ...
Lloyd Motz, Jefferson Hane Weaver
openaire +1 more source
We have seen that a careful analysis of a star’s spectrum reveals the chemical and physical characteristics of its atmosphere, but the spectrum tells us very little about its deep interior. It gives us only the total amount of radiation emitted per second by the star; it tells us nothing about the generation and transport of this radiation through the ...
Lloyd Motz, Jefferson Hane Weaver
openaire +1 more source

