Neutron star cooling in modified gravity theories
国立国会図書館館内限定公開
収録元データベースで確認する
国立国会図書館デジタルコレクション
デジタルデータあり
公開元のウェブサイトで確認する
DOI[10.1093/ptep/ptab099]のデータに遷移します
全国の図書館の所蔵
国立国会図書館以外の全国の図書館の所蔵状況を表示します。
所蔵のある図書館から取寄せることが可能かなど、資料の利用方法は、ご自身が利用されるお近くの図書館へご相談ください
書誌情報
この資料の詳細や典拠（同じ主題の資料を指すキーワード、著者名）等を確認できます。
- 資料種別
- 記事
- 著者・編者
- Akira DohiRyotaro KaseRampei Kimura
- 出版年月日等
- 2021-09
- 出版年（W3CDTF）
- 2021-09
- タイトル（掲載誌）
- Progress of Theoretical and Experimental Physics : PTEP
- 巻号年月日等（掲載誌）
- 2021(9)
- 掲載巻
- 2021(9)
- ISSN（掲載誌）
- 2050-3911
- 本文の言語コード
- eng
- DOI
- 10.1093/ptep/ptab099
- 国立国会図書館永続的識別子
- info:ndljp/pid/11857324
- コレクション（共通）
- コレクション（障害者向け資料：レベル1）
- コレクション（個別）
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- 収集根拠
- オンライン資料収集制度
- 受理日（W3CDTF）
- 2021-10-29T15:30:40+09:00
- 保存日（W3CDTF）
- 2021-10-25
- 記録形式（IMT）
- application/pdf
- オンライン閲覧公開範囲
- 国立国会図書館内限定公開
- デジタル化資料送信
- 図書館・個人送信対象外
- 遠隔複写可否（NDL）
- 可
- 掲載誌（国立国会図書館永続的識別子）
- info:ndljp/pid/11857318
- 連携機関・データベース
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- 要約等
- コレクション : 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- DOI
- 10.1093/ptep/ptab09910.48550/arxiv.2003.12571
- 関連情報（URI）
- 参照
- Revisiting compact star in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>F</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:math> gravity: Roles of chameleon potential and energy conditionsRelativistic star perturbations in Horndeski theories with a gauge-ready formulationInvestigating the Time Evolution of the Thermal Emission from the Putative Neutron Star in SN 1987A for 50+ Years
- 参照
- COOLING OF COMPACT STARS WITH COLOR SUPERCONDUCTING PHASE IN QUARK-HADRON MIXED PHASESpontaneous scalarization with an extremely massive field and heavy neutron starsNeutron stars in<i>f</i>(<i>R</i>) gravity and scalar-tensor theoriesConstraints on perturbative<i>f</i>(<i>R</i>) gravity via neutron starsCooling neutron star in the Cassiopeia A supernova remnant: evidence for superfluidity in the coreStructure of neutron stars in $$R$$ -squared gravityAn X‐Ray Search for Compact Central Sources in Supernova Remnants. I. SNR<scp>s</scp>G093.3+6.9, G315.4−2.3, G084.2+0.8, and G127.1+0.5Structure of neutron star envelopesGravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817AElectromagnetism and hidden vector fields in modified gravity theories: Spontaneous and induced vectorizationLimit on the axion decay constant from the cooling neutron star in Cassiopeia ARelativistic stars in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>and scalar-tensor theoriesNeutron star structure with modern nucleonic three-body forcesNeutron Star CoolingTesting chameleon gravity with the Coma clusterGW170817: Observation of Gravitational Waves from a Binary Neutron Star InspiralConstraint on the cosmological<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>model from the multipole power spectrum of the SDSS luminous red galaxy sample and prospects for a future redshift surveyGas Density Profile in Dark Matter Halo in Chameleon CosmologyRelativistic stars in degenerate higher-order scalar-tensor theories after GW170817Relativistic stars in a cubic Galileon universeNeutron stars with a generalized Proca hair and spontaneous vectorizationModels of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>cosmic acceleration that evade solar system testsHot and cold, nuclear and neutron matterA Massive Pulsar in a Compact Relativistic BinaryRapid Cooling of the Neutron Star in Cassiopeia A Triggered by Neutron Superfluidity in Dense MatterDark Energy After GW170817: Dead Ends and the Road AheadThe Confrontation between General Relativity and ExperimentThe 1979 Nobel Prize in PhysicsTHE WEAK LENSING SIGNAL AND THE CLUSTERING OF BOSS GALAXIES. II. ASTROPHYSICAL AND COSMOLOGICAL CONSTRAINTSf(R) TheoriesRelativistic stars in vector-tensor theoriesGW170817: Measurements of Neutron Star Radii and Equation of StateNeutron stars in the Starobinsky modelConstraints on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:math> theories of gravity from GW170817Thermal Evolution of Neo-neutron Stars. I. Envelopes, Eddington Luminosity Phase, and Implications for GW170817Nuclear equation of state and neutron star coolingObservation of Gravitational Waves from a Binary Black Hole MergerMinimal Cooling of Neutron Stars: A New ParadigmDirect URCA process in neutron starsUpper Limits on the Rapid Cooling of the Central Compact Object in Cas ATheory of SuperconductivityIs cosmic speed-up due to new gravitational physics?Superfluidity of neutron matterA New Method of Automatic Computation of Stellar Evolution.A compendium of chameleon constraintsChameleon cosmologyBlack holes and neutron stars in vector GalileonsTests of chameleon gravitySecond-order scalar-tensor field equations in a four-dimensional spaceA no-hair theorem for black holes in <i>f</i> ( <i>R</i> ) gravityMeasurements of Ω and Λ from 42 High‐Redshift SupernovaeOn neutron stars in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" display="inline" overflow="scroll"> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>R</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:math> theories: Small radii, large masses and large energy emitted in a merger<i>Planck</i>2015 resultsMach's Principle and a Relativistic Theory of GravitationPSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star MatterStrong Constraints on Cosmological Gravity from GW170817 and GRB 170817ANeutron stars in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity with perturbative constraintsRelativistic Shapiro delay measurements of an extremely massive millisecond pulsarNon-perturbative and self-consistent models of neutron stars in<i>R</i>-squared gravityImplications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor TheoriesRelativistic stars in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity, and absence thereofPairing gaps in nucleonic superfluidsTo the problem of nonvanishing gravitation massA NICER View of PSR J0030+0451: Millisecond Pulsar Parameter EstimationScreening Long-Range Forces through Local Symmetry RestorationDark energy fifth forces in torsion pendulum experimentsConstraints on scalar-tensor models of dark energy from observational and local gravity testsBlack Holes, White Dwarfs, and Neutron StarsTHE EQUATION OF STATE FROM OBSERVED MASSES AND RADII OF NEUTRON STARSDiffusive nuclear burning in cooling simulations and application to new temperature data of the Cassiopeia A neutron starBreaking a dark degeneracy with gravitational wavesAn X‐Ray Search for Compact Central Sources in Supernova Remnants. II. Six Large‐Diameter SNRsA no-hair theorem for spherically symmetric black holes in $$R^2$$ R 2 gravityNeutrino emission from neutron starsSpontaneous growth of vector fields in gravityDark Energy after GW170817 and GRB170817AMEASURING THE COOLING OF THE NEUTRON STAR IN CASSIOPEIA A WITH ALL<i>CHANDRA X-RAY OBSERVATORY</i>DETECTORSChameleon Fields: Awaiting Surprises for Tests of Gravity in SpaceThe power spectrum and bispectrum of SDSS DR11 BOSS galaxies – I. Bias and gravityA two-solar-mass neutron star measured using Shapiro delayEquation of state of nucleon matter and neutron star structureThe relativistic equations of stellar structure and evolutionFURTHER CONSTRAINTS ON THERMAL QUIESCENT X-RAY EMISSION FROM SAX J1808.4-3658Proton and neutron superfluidity in neutron star matterAnalytical representations of unified equations of state for neutron-star matterFurther stable neutron star models from<i>f</i>(<i>R</i>) gravityDIRECT OBSERVATION OF THE COOLING OF THE CASSIOPEIA A NEUTRON STARFurther explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII. Stiffness and stability of neutron-star matterImperfect dark energy from kinetic gravity braidingDisappearing cosmological constant in f(R) gravityChallenges to self-acceleration in modified gravity from gravitational waves and large-scale structureNeutron stars in a perturbative<i>f</i>(<i>R</i>) gravity model with strong magnetic fieldsNeutrino emissivities of neutron starsCosmological tests of modified gravityObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological ConstantBaryon Superfluidity and Neutrino Emissivity of Neutron StarsEnergy gap in neutron-star matterEnergy Gaps in Crust-Phase of Neutron StarsPossibility of rapid neutron star cooling with a realistic equation of state
- 連携機関・データベース
- 国立情報学研究所 : CiNii Research
- 提供元機関・データベース
- 雑誌記事索引データベースCrossref科学研究費助成事業データベースCrossrefCrossrefCrossref
- 書誌ID（NDLBibID）
- 11857324