On Lithium Wall and Performance of Magnetic Fusion Device

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On Lithium Wall and Performance of Magnetic Fusion Device S. I. Krasheninnikov 1, L. E. Zakharov 2, and G. V. Pereverzev 3 1 University California San Diego, La Jolla, USA 2 Princeton Plasma Physics Laboratory, Princeton, USA 3 Max-Planck-Institut für Plasmaphysik, Garching bei München, Germany Abstract It is shon that lithium alls resulting in zero recycling conditions at the edge of magnetic fusion device can cause drastic reduction of heat conduction energy loss from the core and, therefore, can crucially alter the performance of magnetic fusion device.

During recent years the idea of potentially very strong impact of fully absorbing lithium alls on the performance of magnetic fusion devices have been reported by the authors many times on different meetings. Hoever, finding again and again the necessity to explain hy lithium all can crucially alter the performance of magnetic fusion devices e decided to publish the essence of our presentations on this particular topic along ith some preliminary modeling of the impact of lithium alls on next step device performance in this brief communication. The paper devoted to a much broader scope of the issues of applications of lithium to magnetic fusion ill be published elsehere. What makes lithium to be so special material for the first all of magnetic fusion devices is practically complete absorption of impinging protons (and other hydrogen isotopes) hich is associated ith the formation of lithium hydride. This feature results in zero recycling of the plasma on lithium surface hen practically there is no hydrogen comes back from the surface into the plasma. (We assume that lithium is not saturated ith hydrogen.) We ill sho that zero recycling conditions causes drastic reduction of heat conduction energy loss from the core and by that can crucially alter the performance of magnetic fusion devices. As an example e ill consider a tokamak, but the conclusions of our analysis can be applied to all magnetic fusion devices. follos The simplest form of the plasma energy transport equation in a tokamak can be ritten as Q Γ (ρ) + Q T (ρ) 5T Γ p (ρ) K(ρ) dt dρ = Q p (ρ), (1) here T is the plasma temperature (for simplicity e assume here T e = T i ), ρ is the effective coordinate going from the center of the machine all the ay to the all (0 ρ 1), Γ p (ρ) and Q p (ρ) are the plasma particle and energy flux, K(ρ) is the effective heat conduction coefficient. The first term on the left hand side of Eq. (1) describes convective part of the energy flux hile the second one is the simplest account for conduction part. To close the equation (1) e need to use the relation beteen plasma energy, Q p = Q p (ρ = 1), and particle, Γ p = Γp (ρ = 1), flux to neutralizing material all at tokamak edge (ρ = 1). For the case here the distribution function of plasma particles coming to the all is described 2

by only one parameter (e. g. effective temperature) e have (see for example Ref. 1 here the coupling of the edge and core plasmas is discussed in details) T = Q p γ Γ, (2) p here γ = γ e + γ i ~ 6 8 and γ e ~ γ i ~ 3 4 are so-called energy transmission coefficient, T is the averaged plasma temperature near the all, T = T(ρ =1). From the Eqs. (1) and (2) e find the contributions of conductive (Q Γ = QΓ (ρ = 1)) and conductive (Q T = Q T (ρ = 1)) parts of the energy flux at the edge are Q Γ Q p = 5 γ, (3a) Q T Q = γ 5 p γ. (3b) As e see from Eq. (3), at the vicinity of the all most of the energy flux is carried by convection. For knon profiles of Γ p (ρ) and Q p (ρ) e can solve the equations (1), (2). Qualitative solution of Eqs. (1), (2) is shon in Fig. 1 for constant Q p (ρ) and the plasma source localized at ρ ρ Γ. As one sees from Fig. 1, there are to distinctive regions of the temperature variation. In one of the regions,ρ < ρ Γ, the energy is transported by conduction causing a strong temperature gradient. In another one, ρ Γ < ρ 1, significant part of the energy is transported by convection hich results in rather flat temperature profile: T Γ < (γ /5)T. In conventional tokamaks flux Γ p is determined mainly by recycling processes including the plasma surface neutralization and volumetric recombination ith the folloing ionization of originated neutrals. The contributions of both gas puffing and pumping are small ( Γ p ) >> Γ conventional puf, Γ pump, (4) 3

here Γ puf (Γ pump ) is the puffing (pumping) particle flux (by puffing e assume here all sorts of hydrogen injection into tokamak). Therefore, the magnitude of plasma flux Γ p is governed by such hardly controlled recycling processes as plasma cross-field transport; reflection, absorption, and desorption of hydrogen at the all; and the transport of neutral hydrogen back to the plasma including neutral-plasma interactions and hydrogen ionization process. Moreover, due to relatively large plasma transport in the recycling region at the edge, the flux Γ p appears to be very large and, therefore, the temperature T is, correspondingly, small (T ~10 100 ev ) in comparison ith central temperature. As a result, large temperature gradient drives ion temperature gradient (ITG) instability resulting in large conductive energy losses and poor plasma performance (e. g. see Ref. 2). Hoever, the situation can be radically changed if the all completely absorbs incoming plasma flux like lithium all does. In this case ( Γ p ) = Γ puf = Γ absorb. (5) Li all Moreover, both magnitude and location of plasma source can be controlled by hydrogen injection. Then ith a proper choice of the location of hydrogen injection, for the same plasma density and energy flux, the magnitude of Γ p can be much smaller and T, correspondingly, much higher then in conventional tokamak (see Fig. 2). As a result, temperature gradient in the core can be reduced belo the level critical for ITG instability causing drastic improvement of plasma confinement. As an example of the impact of fully absorbing lithium all and zero recycling conditions on a tokamak performance e present here some results of the modeling of the performance of the ITER- FEAT [3] assuming fully absorbing boundary. For the modeling e use transport code ASTRA [4]. For the heat, χ e /i, and particle, D, diffusivities e use neo χ e = χ e + ITG χe + min T 11 { χbohm, χ e }, (6a) χ i = χ i neo + χi ITG, (6b) 4

D = D neo neo neo + 0.1 {( χ i χ i )+( χ e χ e )}, (6c) neo here χ e, neo χi, and D neo are the neoclassical heat and particle diffusivities, ITG χe and ITG χi are electron and ion heat diffusivities associated ith the ITG instability taken from [2], χ Bohm is the Bohm T 11 diffusion coefficient, and χ e is the Ohkaa type scaling from [5]. Neoclassical particle pinch is also accounted for in the plasma density transport equation. We assume 30 MW of the neutral beam and 10 MW of the ICRF auxiliary heating. We also adopt 5% dilution of the plasma due to helium and???5% due to beryllium. As the boundary conditions for the plasma density and both electron and ion temperatures at the all e used the model from Ref. 1 hich, in particular, relates the energy fluxes and temperatures in electron and ion components similar to that of Eq. (2). For the modeling presented here e choose γ e = γ i = 3. We apply bell shaped plasma particle source at ρ = 0.75 ith the magnitude varying to sustain constant volume averaged plasma density of 10 20 m 3. To model fully absorbing lithium all e assume no any other plasma particle source. We start ith nominal IETR-FEAT regime [3] and find that fusion poer runs aay. Time history of ion temperature in the center (T i (ρ = 0, t)) and at the all p (T i (ρ = 1, t)), fusion poer (P fus (t)), and plasma flux to the all (Γ (t)) are shon in Fig. 3. At these times β N does not exceed 2.5. As one sees from Fig. 3, in accordance ith Eq. (2) edge plasma temperatures naturally increase ith increasing fusion poer. As a result, temperature gradient in the core does not increase ith increasing fusion poer hich allos to avoid a fatal impact of the ITG instability. This is in a sharp contrast to conventional ITER here separatrix plasma temperature is negligibly small and the ITG instability limits the temperature gradient so that the performance of the machine is completely determined by the height of H-mode pedestal. The plasma density and electron and ion temperature profiles for t=1 sec are shon in Fig. 4. Notice that high edge plasma temperatures significantly increase fusion poer yield so that the ITER runs aay ith averaged energy confinement time ~ 2 s. 5

In sum, e sho that lithium alls resulting in zero recycling conditions at the edge of magnetic fusion device can cause drastic reduction of heat conduction energy loss from the core and, therefore, can crucially alter the performance of magnetic fusion device. As an example e model the ITER-FEAT performance ith lithium alls and sho that fusion poer runs aay due to natural increase edge plasma temperature ith increasing fusion poer hich eliminate strong core plasma gradient causing the ITG instability. Acknoledgments This research as supported by United States Department of Energy. 6

References [1] S. I. Krasheninnikov, P. N. Yushmanov, Sov. J. Plasma Phys., 16 (1990) 801; A. Yu. Dnestrovskij, S. I. Krasheninnikov, P. N. Yushmanov, Nucl. Fusion, 31 (1991) 647. [2] M. Kotschenreuther, W. Dorland, M. A. Beer, and G. W. Hammet, Phys. Plasmas 2 (1995) 2381. [3] Y. Shimomura, R. Aymar, V. Chuyanov, M. Huget, H. Matsumoto, T. Mizoguchi, Y. Murakami, A. Polevoi, M. Shimada and the ITER Joint Central Team and Home Teams, "ITER-FEAT Operation" 18th IAEA Fusion Energy Conference, Sorrento, Italy, 4-10 October 2000, Paper ITER/1. [4] G. Pereverzev and P. N. Yushmanov, ASTRA Automated System for Transport Analysis in a Tokamak, Max-Planck-Institut fur Plasmaphysik, IPP 5/98, February 2002. [5] A. G. Barsukov et al., 9th IAEA Conference on Plasma Physics and Controlled Nuclear Fusion Research, Baltimore, 1982 (IAEA, Vienna, V. 1 (1983) 83). 7

Figure Captions Fig. 1. Qualitative dependence T(ρ) of the solution of Eqs. (1), (2). Fig. 2. Schematic dependence of T(ρ) for both conventional and lithium all tokamaks. Fig. 3. Time history of ion central, T i (ρ = 0, t), and all, T i (ρ = 1, t), temperatures, fusion poer, p P fus (t), and plasma flux to the all, Γ (t). Fig. 4. The plasma density, n e (ρ), electron, T e (ρ), and ion, T i (ρ), temperature profiles for t=1 sec. On the top panel the shape of plasma particle source, S e (ρ), is also shon. 8

T(ρ) Q p (ρ) T Γ T Q p Γ p (ρ) Γ p ρ Γ 1 ρ Fig. 1. 9

Li all conventional T(ρ) Γ p (ρ) 1 ρ Fig. 2. 10

[kev] T i (ρ=0,t) T i (ρ=1,t) [GW] P fus (t) [10 22, s -1 ] Γ p (t) t, s Fig. 3. 11

1.5 1 0.5 [10 20, m -3 ] S e (ρ) n e (ρ) 0 0.25 0.5 0.75 1 20 T e (ρ) [kev] 10 T i (ρ) 0 0.25 0.5 0.75 1 ρ Fig. 4. 12

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