Matches in SemOpenAlex for { <https://semopenalex.org/work/W2740554105> ?p ?o ?g. }
- W2740554105 abstract "At second order in perturbation theory, the unstable r-mode of a rotating star includes growing differential rotation whose form and growth rate are determined by gravitational-radiation reaction. With no magnetic field, the angular velocity of a fluid element grows exponentially until the mode reaches its nonlinear saturation amplitude and remains nonzero after saturation. With a background magnetic field, the differential rotation winds up and amplifies the field, and previous work where large mode amplitudes were considered suggests that the amplification may damp out the instability. A background magnetic field, however, turns the saturated time-independent perturbations corresponding to adding differential rotation into perturbations whose characteristic frequencies are of order the Alfv'en frequency. As found in previous studies, we argue that magnetic- field growth is sharply limited by the saturation amplitude of an unstable mode. In contrast to previous work, however, we show that if the amplitude is small, i.e., of order 10^(-4), then the limit on the magnetic-field growth is stringent enough to prevent the loss of energy to the magnetic field from damping or significantly altering an unstable r-mode in nascent neutron stars with normal interiors and in cold stars whose interiors are type II superconductors. We show this result first for a toy model, and we then obtain an analogous upper limit on magnetic field growth using a more realistic model of a rotating neutron star. Our analysis depends on the assumption that there are no marginally unstable perturbations, and this may not hold when differential rotation leads to a magnetorotational instability." @default.
- W2740554105 created "2017-08-08" @default.
- W2740554105 creator A5007493982 @default.
- W2740554105 creator A5034731703 @default.
- W2740554105 creator A5052568385 @default.
- W2740554105 creator A5060564143 @default.
- W2740554105 date "2017-12-12" @default.
- W2740554105 modified "2023-10-17" @default.
- W2740554105 title "Limits on magnetic field amplification from the r -mode instability" @default.
- W2740554105 cites W1615681384 @default.
- W2740554105 cites W1844037262 @default.
- W2740554105 cites W1860224658 @default.
- W2740554105 cites W1970987695 @default.
- W2740554105 cites W1973052444 @default.
- W2740554105 cites W1986698473 @default.
- W2740554105 cites W1994857684 @default.
- W2740554105 cites W2011591061 @default.
- W2740554105 cites W2011606992 @default.
- W2740554105 cites W2015096308 @default.
- W2740554105 cites W2025016837 @default.
- W2740554105 cites W2025639957 @default.
- W2740554105 cites W2026494651 @default.
- W2740554105 cites W2033298480 @default.
- W2740554105 cites W2034809421 @default.
- W2740554105 cites W2043487112 @default.
- W2740554105 cites W2045694681 @default.
- W2740554105 cites W2047479827 @default.
- W2740554105 cites W2048273191 @default.
- W2740554105 cites W2052425458 @default.
- W2740554105 cites W2057348364 @default.
- W2740554105 cites W2059863168 @default.
- W2740554105 cites W2069651370 @default.
- W2740554105 cites W2081545524 @default.
- W2740554105 cites W2085339226 @default.
- W2740554105 cites W2093770362 @default.
- W2740554105 cites W2095437474 @default.
- W2740554105 cites W2097375932 @default.
- W2740554105 cites W2116961354 @default.
- W2740554105 cites W2130360506 @default.
- W2740554105 cites W2133668220 @default.
- W2740554105 cites W2189197678 @default.
- W2740554105 cites W2241183286 @default.
- W2740554105 cites W2256333104 @default.
- W2740554105 cites W2280022730 @default.
- W2740554105 cites W2536145767 @default.
- W2740554105 cites W2592733448 @default.
- W2740554105 cites W2594385597 @default.
- W2740554105 cites W2950667339 @default.
- W2740554105 cites W3100292491 @default.
- W2740554105 cites W3100430726 @default.
- W2740554105 cites W3100618079 @default.
- W2740554105 cites W3101727583 @default.
- W2740554105 cites W3102652932 @default.
- W2740554105 cites W3104550030 @default.
- W2740554105 cites W3122130680 @default.
- W2740554105 cites W3123942903 @default.
- W2740554105 cites W4205445407 @default.
- W2740554105 cites W4205483922 @default.
- W2740554105 cites W4241839635 @default.
- W2740554105 doi "https://doi.org/10.1103/physrevd.96.124008" @default.
- W2740554105 hasPublicationYear "2017" @default.
- W2740554105 type Work @default.
- W2740554105 sameAs 2740554105 @default.
- W2740554105 citedByCount "4" @default.
- W2740554105 countsByYear W27405541052017 @default.
- W2740554105 countsByYear W27405541052018 @default.
- W2740554105 countsByYear W27405541052019 @default.
- W2740554105 crossrefType "journal-article" @default.
- W2740554105 hasAuthorship W2740554105A5007493982 @default.
- W2740554105 hasAuthorship W2740554105A5034731703 @default.
- W2740554105 hasAuthorship W2740554105A5052568385 @default.
- W2740554105 hasAuthorship W2740554105A5060564143 @default.
- W2740554105 hasBestOaLocation W27405541051 @default.
- W2740554105 hasConcept C115260700 @default.
- W2740554105 hasConcept C121332964 @default.
- W2740554105 hasConcept C14257148 @default.
- W2740554105 hasConcept C190330329 @default.
- W2740554105 hasConcept C192887742 @default.
- W2740554105 hasConcept C207821765 @default.
- W2740554105 hasConcept C2776761751 @default.
- W2740554105 hasConcept C3079626 @default.
- W2740554105 hasConcept C44870925 @default.
- W2740554105 hasConcept C57879066 @default.
- W2740554105 hasConcept C62520636 @default.
- W2740554105 hasConcept C74650414 @default.
- W2740554105 hasConceptScore W2740554105C115260700 @default.
- W2740554105 hasConceptScore W2740554105C121332964 @default.
- W2740554105 hasConceptScore W2740554105C14257148 @default.
- W2740554105 hasConceptScore W2740554105C190330329 @default.
- W2740554105 hasConceptScore W2740554105C192887742 @default.
- W2740554105 hasConceptScore W2740554105C207821765 @default.
- W2740554105 hasConceptScore W2740554105C2776761751 @default.
- W2740554105 hasConceptScore W2740554105C3079626 @default.
- W2740554105 hasConceptScore W2740554105C44870925 @default.
- W2740554105 hasConceptScore W2740554105C57879066 @default.
- W2740554105 hasConceptScore W2740554105C62520636 @default.
- W2740554105 hasConceptScore W2740554105C74650414 @default.
- W2740554105 hasFunder F4320306076 @default.
- W2740554105 hasFunder F4320324099 @default.
- W2740554105 hasFunder F4320332999 @default.