Results 321 to 330 of about 3,828,801 (363)

Digital Behavioral Therapy Improves Outcome in Patients With Axial Spondyloarthritis and Persistent Pain: A Randomized Controlled Trial

open access: yesArthritis Care &Research, EarlyView.
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

Neutron capture measurements for s-process nucleosynthesis: A review about CERN n_TOF developments and contributions. [PDF]

open access: yesEur Phys J A Hadron Nucl
Domingo-Pardo C   +145 more
europepmc   +1 more source

The <sup>22</sup>Ne( α ,n)<sup>25</sup>Mg reaction - state of the art, astrophysics, and perspectives. [PDF]

open access: yesEur Phys J A Hadron Nucl
Best A   +13 more
europepmc   +1 more source

Stellar occultations: a gateway to advances in planetary science. [PDF]

open access: yesPhilos Trans A Math Phys Eng Sci
Souami D   +3 more
europepmc   +1 more source

Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures

Nature Astronomy, 2021
While 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, 2021
These 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
semanticscholar   +1 more source

Stellar Masses and Radii

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

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