This Letter presents the first observation on how a strong, 500 kG, externally applied B field increases the mode-two asymmetry in shock-heated inertial fusion implosions. Using a direct-drive implosion with polar illumination and imposed field, we observed that magnetization produces a significant increase in the implosion oblateness (a 2.5× larger P2 amplitude in x-ray self-emission images) compared with reference experiments with identical drive but with no field applied. The implosions produce strongly magnetized electrons (ω_e τ_e ≫ 1) and ions (ω_i τ_i > 1) that, as shown using simulations, restrict the cross field heat flow necessary for lateral distribution of the laser and shock heating from the implosion pole to the waist, causing the enhanced mode-two shape.

Effect of strongly magnetized electrons and ions on heat flow and symmetry of inertial fusion implosions / Bose, A.; Peebles, J.; Walsh, C.  A.; Frenje, J.  A.; Kabadi, N.  V.; Adrian, P.  J.; Sutcliffe, G.  D.; Gatu Johnson, M.; Frank, C.  A.; Davies, J.  R.; Betti, R.; Glebov, V.  Yu.; Marshall, F.  J.; Regan, S.  P.; Stoeckl, C.; Campbell, E.  M.; Sio, H.; Moody, J.; Crilly, A.; Appelbe, B.  D.; Chittenden, J.  P.; Atzeni, S.; Barbato, F.; Forte, A.; Li, C.  K.; Seguin, F.  H.; Petrasso, R.  D.. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 128:19(2022). [10.1103/PhysRevLett.128.195002]

Effect of strongly magnetized electrons and ions on heat flow and symmetry of inertial fusion implosions

Atzeni, S.;Barbato, F.;
2022

Abstract

This Letter presents the first observation on how a strong, 500 kG, externally applied B field increases the mode-two asymmetry in shock-heated inertial fusion implosions. Using a direct-drive implosion with polar illumination and imposed field, we observed that magnetization produces a significant increase in the implosion oblateness (a 2.5× larger P2 amplitude in x-ray self-emission images) compared with reference experiments with identical drive but with no field applied. The implosions produce strongly magnetized electrons (ω_e τ_e ≫ 1) and ions (ω_i τ_i > 1) that, as shown using simulations, restrict the cross field heat flow necessary for lateral distribution of the laser and shock heating from the implosion pole to the waist, causing the enhanced mode-two shape.
2022
Plasma Physics, Inertial confinement fusion, shock-driven implosion, magnetized implosion
01 Pubblicazione su rivista::01a Articolo in rivista
Effect of strongly magnetized electrons and ions on heat flow and symmetry of inertial fusion implosions / Bose, A.; Peebles, J.; Walsh, C.  A.; Frenje, J.  A.; Kabadi, N.  V.; Adrian, P.  J.; Sutcliffe, G.  D.; Gatu Johnson, M.; Frank, C.  A.; Davies, J.  R.; Betti, R.; Glebov, V.  Yu.; Marshall, F.  J.; Regan, S.  P.; Stoeckl, C.; Campbell, E.  M.; Sio, H.; Moody, J.; Crilly, A.; Appelbe, B.  D.; Chittenden, J.  P.; Atzeni, S.; Barbato, F.; Forte, A.; Li, C.  K.; Seguin, F.  H.; Petrasso, R.  D.. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 128:19(2022). [10.1103/PhysRevLett.128.195002]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1633737
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