Shock-Augmented Ignition Approach to Laser Inertial Fusion.


Journal

Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141

Informations de publication

Date de publication:
04 Nov 2022
Historique:
received: 23 06 2021
revised: 24 08 2022
accepted: 21 09 2022
entrez: 18 11 2022
pubmed: 19 11 2022
medline: 19 11 2022
Statut: ppublish

Résumé

Shock ignition enables high gain at low implosion velocity, reducing ablative Rayleigh-Taylor instability growth, which can degrade conventional direct drive. With this method, driving a strong shock requires high laser power and intensity, resulting in inefficiencies in the drive and the generation of hot electrons that can preheat the fuel. A new "shock-augmented ignition" pulse shape is described that, by preconditioning the ablation plasma before launching a strong shock, enables the shock ignition of thermonuclear fuel, but importantly, with substantially reduced laser power and intensity requirements. The reduced intensity requirement with respect to shock ignition limits laser-plasma instabilities, such as stimulated Raman and Brillouin scatter, reducing the risk of hot-electron preheat and restoring the laser coupling advantages of conventional direct drive. Simulations indicate that, due to the reduced power requirements, high gain (∼100) ignition of large-scale direct drive implosions (outer radius ∼1750  μm, deuterium-tritium ice thickness ∼165  μm) may be possible within the power and energy limits of existing facilities such as the National Ignition Facility. Moreover, this concept extends to indirect drive implosions, which exhibit substantial yield increases at reduced implosion velocity. Shock-augmented ignition expands the viable design space of laser inertial fusion.

Identifiants

pubmed: 36399760
doi: 10.1103/PhysRevLett.129.195001
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

195001

Auteurs

R H H Scott (RHH)

Central Laser Facility, STFC Rutherford Appleton Laboratory, Harwell Oxford, OX11 0QX, United Kingdom.

D Barlow (D)

Central Laser Facility, STFC Rutherford Appleton Laboratory, Harwell Oxford, OX11 0QX, United Kingdom.

W Trickey (W)

York Plasma Institute, School of Physics, Engineering and Technology, University of York, York, YO10 5DD, United Kingdom.

A Ruocco (A)

Central Laser Facility, STFC Rutherford Appleton Laboratory, Harwell Oxford, OX11 0QX, United Kingdom.

K Glize (K)

Central Laser Facility, STFC Rutherford Appleton Laboratory, Harwell Oxford, OX11 0QX, United Kingdom.

L Antonelli (L)

York Plasma Institute, School of Physics, Engineering and Technology, University of York, York, YO10 5DD, United Kingdom.

M Khan (M)

York Plasma Institute, School of Physics, Engineering and Technology, University of York, York, YO10 5DD, United Kingdom.

N C Woolsey (NC)

York Plasma Institute, School of Physics, Engineering and Technology, University of York, York, YO10 5DD, United Kingdom.

Classifications MeSH