Results 101 to 110 of about 115,270 (322)

High‐Density Boron Nitride Nanotube Composites via Surfactant‐Stabilized Lyotropic Liquid Crystals for Enhanced Space Radiation Shielding

Advanced Functional Materials, EarlyView.
High‐density BNNT films, enabling mechanical robustness and high space radiation shielding effectiveness, are fabricated using surfactant‐stabilized BNNT liquid crystal. Simulations indicate that a 50 g cm−2 BNNT film can reduce radiation exposure by 56% compared to zero shielding, potentially doubling the duration of astronaut missions on the lunar ...
Young‐Kyeong Kim, Ik Jae Lim, Hongjin Lim, Yongbi Joo, Jueun Park, Md Monir Hossain, Hyunjin Cho, Nam‐Ho You, Seokhoon Ahn, Hunsu Lee, Sang Seok Lee, Yongho Joo, Se Youn Moon, Hee Il Yoo, Calista Lum, Cheol Park, Siyoung Q. Choi, Se Gyu Jang   +17 more
wiley   +1 more source

Isolated Neutron Stars

, 2023
Invited chapter for Handbook of X-ray and Gamma-ray Astrophysics (Section Eds. V. Doroshenko, A. Santangelo; Eds. C. Bambi and A. Santangelo, Springer Singapore, 2023)
Borghese, Alice, Esposito, Paolo
openaire   +2 more sources

Reaction rates and transport in neutron stars

, 2018
Understanding signals from neutron stars requires knowledge about the transport inside the star. We review the transport properties and the underlying reaction rates of dense hadronic and quark matter in the crust and the core of neutron stars and point ...
A Bransgrove, A Carbone, A Dehghan Niri, A Deibel, A Kurkela, A Passamonti, A Reisenegger, A Reisenegger, A Schmitt, A Schwenk, A Sedrakian, A Sedrakian, A. Akmal, AB Migdal, AB Migdal, AD Kaminker, AD Kaminker, AD Sedrakian, AI Chugunov, AI Chugunov, AI Chugunov, AI Chugunov, AJ Leggett, AJ Leggett, Alexander Haber, AM Beloborodov, AM Bykov, AM Rosenfeld, AMJ Schaeffer, AR Zhitnitsky, AY Potekhin, AY Potekhin, AY Potekhin, AY Potekhin, AY Potekhin, AY Potekhin, AY Potekhin, AY Potekhin, AY Potekhin, B Friman, B Haskell, B Haskell, B Posselt, BL Friman, BM Askerov, BP Abbott, Brynmor Haskell, C Eckart, C Manuel, C Manuel, C Petrovich, Christof Gattringer, CJ Horowitz, CJ Horowitz, CJ Pethick, CO Heinke, Cristina Manuel, D Bailin, D Blaschke, D Blaschke, D Burnett, D Burnett, D Jaccarino, D Mateos, D N Aguilera, D Page, D Page, D Page, D Page, D Viganò, D Vollhardt, DA Baiko, DA Baiko, DA Baiko, DA Baiko, DA Baiko, DA Shalybkov, DA Young, DD Ofengeim, DE Kharzeev, DG Ravenhall, DG Yakovlev, DG Yakovlev, DG Yakovlev, DG Yakovlev, DG Yakovlev, DG Yakovlev, DG Yakovlev, DG Yakovlev, DK Berry, DN Voskresensky, DT Son, DT Son, E Flowers, E Flowers, E Flowers, EE Kolomeitsev, EF Brown, EF Brown, EM Cackett, F Castillo, F Wilczek, FE Low, G Aarts, G Baym, G Baym, G Baym, G Chabrier, GA Brooker, GE Tauber, Gilberto Medeiros Kremer, GS Bisnovatyi-Kogan, GV Vereshchagin, H Heiselberg, H Heiselberg, H Højgård Jensen, H Reinholz, H Schatz, H Schatz, Igor A Shovkovy, IM Khalatnikov, J Boguta, J Carlson, J Chao, J Charbonneau, J Charbonneau, J Daligault, J Hoyos, J Madsen, J Madsen, J Sykes, J Wambach, JA Pons, JA Pons, JD Anand, JE Kim, JF Pérez-Azorín, JG Elfritz, JL Friedman, JM Dong, JM Lattimer, JM Ziman, JM Ziman, K Glampedakis, K Glampedakis, K Glampedakis, K Landsteiner, KG Balasi, KG Elshamouty, KS Thorne, L García-Colín, L Hernquist, L Landau, L Tisza, L Tolos, L Villain, LD Landau, LD Landau, LO Juri, M Delehaye, M Dine, M Greiter, M Hashimoto, M Iwasaki, M Iwasaki, M Kutschera, M Kutschera, M Kutschera, M Kutschera, M Mannarelli, M Wiescher, MA Shahzamanian, MA Shifman, MA Stephanov, MD Jones, ME Caplan, ME Gusakov, ME Gusakov, MG Alford, MG Alford, MG Alford, MG Alford, MG Alford, MG Alford, MG Alford, MG Alford, MG Alford, MV Beznogov, MV Beznogov, N Andersson, N Andersson, N Chamel, N Chamel, N Chamel, N Chamel, N Degenaar, N González-Jiménez, N Itoh, N Iwamoto, N Iwamoto, N Iwamoto, N Iwamoto, O Benhar, Omar Benhar, OV Maxwell, OY Gnedin, P Goldreich, P Haensel, P Haensel, P Haensel, P Haensel, P Haensel, P Haensel, P Haensel, P Kovtun, P Shternin, PAUL ROMATSCHKE, Pavel Kovtun, PB Jones, PI Arseev, PS Shternin, PS Shternin, PS Shternin, PS Shternin, PS Shternin, PS Shternin, Q D Wang, Q Li, R Anglani, R Mckinven, R Nandi, R Schmidt, R Turolla, RD Peccei, RF Sawyer, RF Sawyer, RG Timmermans, RH Anderson, RJ Donnelly, RN Manchester, Robert C Myers, S Cassisi, S Chapman, S Flores-Tulián, S Gupta, S Hannestad, S Weinberg, SC Huot, SH Lam, SI Braginskii, SL Adler, SL Shapiro, SS Gupta, T Hatsuda, T Noda, T Schäfer, TH Burnett, V Graber, V Zhdanov, Vanessa Graber, VP Silin, W Israel, W Zuo, W-B Ding, WA Harrison, WH Dickhoff, Wolfgang Keil, Y Li, Y Li, Y. Aoki   +269 more
core   +1 more source

Magnetic‐Field Tuning of the Spin Dynamics in the Quasi‐2D Van der Waals Antiferromagnet CuCrP2S6

Advanced Functional Materials, EarlyView.
This study reveals 2D character of the spin dynamics in CuCrP2S6, as well as complex field dependence of collective excitations in the antiferromagnetically ordered state. Their remarkable tuning from the antiferromagnetic to the ferromagnetic type with magnetic field, together with the non‐degeneracy of the magnon gaps favorable for the induction of ...
Joyal John Abraham, Yaqian Guo, Yuliia Shemerliuk, Sebastian Selter, Saicharan Aswartham, Kranthi Kumar Bestha, Laura T. Corredor, Anja U. B. Wolter, Olga Kataeva, Luka Rogić, Noah Somun, Damjan Pelc, Oleg Janson, Jeroen van den Brink, Bernd Büchner, Vladislav Kataev, Alexey Alfonsov   +16 more
wiley   +1 more source

Phases of Hadron-Quark Matter in (Proto) Neutron Stars

Universe, 2019
In the first part of this paper, we investigate the possible existence of a structured hadron-quark mixed phase in the cores of neutron stars. This phase, referred to as the hadron-quark pasta phase, consists of spherical blob, rod, and slab rare phase ...
Fridolin Weber, Delaney Farrell, William M. Spinella, Germán Malfatti, Milva G. Orsaria, Gustavo A. Contrera, Ian Maloney   +6 more
doaj   +1 more source

Neutron Star Matter and Neutron Star Models

Zeitschrift für Naturforschung A, 1974
Various methods to study the ground state of neutron star matter are compared and the corresponding neutron star models are contrasted with each other. In the low density region ρ < 1014gr cm-3 the nuclear gas is treated here by means of a Thomas Fermi method and the nuclei are described by the droplet model of Myers and Swiatecki.
H. Heintzmann, M. F. El Eid, Eberhard R. Hilf, W. Hillebrandt   +3 more
openaire   +2 more sources

Enhancing Mechanical Deformability of Rigid Conjugated Polymers through Functional Additive‐Induced Persistence Length Modulation

Advanced Functional Materials, EarlyView.
This study demonstrates a molecular strategy to enhance the stretchability of conjugated polymers by incorporating plasticizing molecular additives (PMAs). PMAs reduce the persistence length and promote chain entanglement, enabling deformable thin films with preserved electrical performance. A systematic analysis combining rheology, neutron scattering,
Sein Chung, Seung Hyun Kim, Sanghyo Kim, Eunsol Ok, Byeong Jin Kim, Jimin Kim, Jiyeong Shin, Taehun Chung, Jong Dae Jang, Siyoung Lee, Boseok Kang, Kilwon Cho   +11 more
wiley   +1 more source

Analysis of the Conformally Flat Approximation for Binary Neutron Star Initial Conditions

Advances in Astronomy, 2017
The spatially conformally flat approximation (CFA) is a viable method to deduce initial conditions for the subsequent evolution of binary neutron stars employing the full Einstein equations.
In-Saeng Suh, Grant J. Mathews, J. Reese Haywood, N. Q. Lan   +3 more
doaj   +1 more source

General Relativistic Decompression of Binary Neutron Stars During Dynamic Inspiral

, 2007
We investigate the dynamic stability of inspiraling neutron stars by performing multiple-orbit numerical relativity simulations of the binary neutron star inspiral process.
Miller, Mark
core   +1 more source

Direct Evidence of Topological Dirac Fermions in a Low Carrier Density Correlated 5d Oxide

Advanced Functional Materials, EarlyView.
The 5d oxide BiRe2O6 is discovered as a low‐carrier‐density topological semimetal hosting symmetry‐protected Dirac fermions stabilized by nonsymmorphic symmetries. Angle‐resolved photoemission spectroscopy, quantum oscillations, and magnetotransport measurements reveal gapless Dirac cones, quasi‐2D Fermi surfaces, high carrier mobility, and a field ...
Premakumar Yanda, Jorge Cardenas‐Gamboa, Ding Pei, François Bertran, Leila Noohinejad, Snehashish Chatterjee, Changjiang Yi, Iñigo Robredo, Horst Borrmann, Maia G. Vergniory, Chandra Shekhar, Claudia Felser   +11 more
wiley   +1 more source