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Your search keyword '"Tuev, P."' showing total 15 results
Start Over Author "Tuev, P." Publisher max planck inst phys & astrophys, d-80805 munich, germany.
15 results on '"Tuev, P."'

1. Filamentation of a relativistic proton bunch in plasma

Author

Verra, L., Amoedo, C., Torrado, N., Clairembaud, A., Mezger, J., Pannell, F., Pucek, J., van Gils, N., Bergamaschi, M., Della Porta, G. Zevi, Lopes, N., Sublet, A., Turner, M., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bencini, V., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. A., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Guzman, P. I. Morales, Moreira, M., Nechaeva, T., Okhotnikov, N., Pakuza, C., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Ranc, L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Swain, C., Topaloudis, A., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Walter, E., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., Zepp, M., Verra, L., Amoedo, C., Torrado, N., Clairembaud, A., Mezger, J., Pannell, F., Pucek, J., van Gils, N., Bergamaschi, M., Della Porta, G. Zevi, Lopes, N., Sublet, A., Turner, M., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bencini, V., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. A., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Guzman, P. I. Morales, Moreira, M., Nechaeva, T., Okhotnikov, N., Pakuza, C., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Ranc, L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Swain, C., Topaloudis, A., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Walter, E., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., and Zepp, M.

Abstract

We show in experiments that a long, underdense, relativistic proton bunch propagating in plasma undergoes the oblique instability, which we observe as filamentation. We determine a threshold value for the ratio between the bunch transverse size and plasma skin depth for the instability to occur. At the threshold, the outcome of the experiment alternates between filamentation and self-modulation instability (evidenced by longitudinal modulation into microbunches). Time-resolved images of the bunch density distribution reveal that filamentation grows to an observable level late along the bunch, confirming the spatiotemporal nature of the instability. We provide a rough estimate of the amplitude of the magnetic field generated in the plasma by the instability and show that the associated magnetic energy increases with plasma density.

Published
2024
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2. Filamentation of a relativistic proton bunch in plasma

Author

Verra, L., Amoedo, C., Torrado, N., Clairembaud, A., Mezger, J., Pannell, F., Pucek, J., van Gils, N., Bergamaschi, M., Della Porta, G. Zevi, Lopes, N., Sublet, A., Turner, M., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bencini, V., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. A., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Guzman, P. I. Morales, Moreira, M., Nechaeva, T., Okhotnikov, N., Pakuza, C., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Ranc, L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Swain, C., Topaloudis, A., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Walter, E., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., Zepp, M., Verra, L., Amoedo, C., Torrado, N., Clairembaud, A., Mezger, J., Pannell, F., Pucek, J., van Gils, N., Bergamaschi, M., Della Porta, G. Zevi, Lopes, N., Sublet, A., Turner, M., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bencini, V., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. A., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Guzman, P. I. Morales, Moreira, M., Nechaeva, T., Okhotnikov, N., Pakuza, C., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Ranc, L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Swain, C., Topaloudis, A., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Walter, E., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., and Zepp, M.

Abstract

We show in experiments that a long, underdense, relativistic proton bunch propagating in plasma undergoes the oblique instability, which we observe as filamentation. We determine a threshold value for the ratio between the bunch transverse size and plasma skin depth for the instability to occur. At the threshold, the outcome of the experiment alternates between filamentation and self-modulation instability (evidenced by longitudinal modulation into microbunches). Time-resolved images of the bunch density distribution reveal that filamentation grows to an observable level late along the bunch, confirming the spatiotemporal nature of the instability. We provide a rough estimate of the amplitude of the magnetic field generated in the plasma by the instability and show that the associated magnetic energy increases with plasma density.

Published
2024
Full Text
View/download PDF

3. Filamentation of a relativistic proton bunch in plasma

Author

Verra, L., Amoedo, C., Torrado, N., Clairembaud, A., Mezger, J., Pannell, F., Pucek, J., van Gils, N., Bergamaschi, M., Della Porta, G. Zevi, Lopes, N., Sublet, A., Turner, M., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bencini, V., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. A., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Guzman, P. I. Morales, Moreira, M., Nechaeva, T., Okhotnikov, N., Pakuza, C., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Ranc, L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Swain, C., Topaloudis, A., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Walter, E., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., Zepp, M., Verra, L., Amoedo, C., Torrado, N., Clairembaud, A., Mezger, J., Pannell, F., Pucek, J., van Gils, N., Bergamaschi, M., Della Porta, G. Zevi, Lopes, N., Sublet, A., Turner, M., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bencini, V., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. A., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Guzman, P. I. Morales, Moreira, M., Nechaeva, T., Okhotnikov, N., Pakuza, C., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Ranc, L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Swain, C., Topaloudis, A., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Walter, E., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., and Zepp, M.

Abstract

We show in experiments that a long, underdense, relativistic proton bunch propagating in plasma undergoes the oblique instability, which we observe as filamentation. We determine a threshold value for the ratio between the bunch transverse size and plasma skin depth for the instability to occur. At the threshold, the outcome of the experiment alternates between filamentation and self-modulation instability (evidenced by longitudinal modulation into microbunches). Time-resolved images of the bunch density distribution reveal that filamentation grows to an observable level late along the bunch, confirming the spatiotemporal nature of the instability. We provide a rough estimate of the amplitude of the magnetic field generated in the plasma by the instability and show that the associated magnetic energy increases with plasma density.

Published
2024
Full Text
View/download PDF

4. Filamentation of a relativistic proton bunch in plasma

Author

Verra, L., Amoedo, C., Torrado, N., Clairembaud, A., Mezger, J., Pannell, F., Pucek, J., van Gils, N., Bergamaschi, M., Della Porta, G. Zevi, Lopes, N., Sublet, A., Turner, M., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bencini, V., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. A., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Guzman, P. I. Morales, Moreira, M., Nechaeva, T., Okhotnikov, N., Pakuza, C., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Ranc, L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Swain, C., Topaloudis, A., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Walter, E., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., Zepp, M., Verra, L., Amoedo, C., Torrado, N., Clairembaud, A., Mezger, J., Pannell, F., Pucek, J., van Gils, N., Bergamaschi, M., Della Porta, G. Zevi, Lopes, N., Sublet, A., Turner, M., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bencini, V., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. A., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Guzman, P. I. Morales, Moreira, M., Nechaeva, T., Okhotnikov, N., Pakuza, C., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Ranc, L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Swain, C., Topaloudis, A., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Walter, E., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., and Zepp, M.

Abstract

We show in experiments that a long, underdense, relativistic proton bunch propagating in plasma undergoes the oblique instability, which we observe as filamentation. We determine a threshold value for the ratio between the bunch transverse size and plasma skin depth for the instability to occur. At the threshold, the outcome of the experiment alternates between filamentation and self-modulation instability (evidenced by longitudinal modulation into microbunches). Time-resolved images of the bunch density distribution reveal that filamentation grows to an observable level late along the bunch, confirming the spatiotemporal nature of the instability. We provide a rough estimate of the amplitude of the magnetic field generated in the plasma by the instability and show that the associated magnetic energy increases with plasma density.

Published
2024
Full Text
View/download PDF

5. Filamentation of a relativistic proton bunch in plasma

Author

Verra, L., Amoedo, C., Torrado, N., Clairembaud, A., Mezger, J., Pannell, F., Pucek, J., van Gils, N., Bergamaschi, M., Della Porta, G. Zevi, Lopes, N., Sublet, A., Turner, M., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bencini, V., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. A., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Guzman, P. I. Morales, Moreira, M., Nechaeva, T., Okhotnikov, N., Pakuza, C., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Ranc, L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Swain, C., Topaloudis, A., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Walter, E., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., Zepp, M., Verra, L., Amoedo, C., Torrado, N., Clairembaud, A., Mezger, J., Pannell, F., Pucek, J., van Gils, N., Bergamaschi, M., Della Porta, G. Zevi, Lopes, N., Sublet, A., Turner, M., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bencini, V., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. A., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Guzman, P. I. Morales, Moreira, M., Nechaeva, T., Okhotnikov, N., Pakuza, C., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Ranc, L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Swain, C., Topaloudis, A., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Walter, E., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., and Zepp, M.

Abstract

We show in experiments that a long, underdense, relativistic proton bunch propagating in plasma undergoes the oblique instability, which we observe as filamentation. We determine a threshold value for the ratio between the bunch transverse size and plasma skin depth for the instability to occur. At the threshold, the outcome of the experiment alternates between filamentation and self-modulation instability (evidenced by longitudinal modulation into microbunches). Time-resolved images of the bunch density distribution reveal that filamentation grows to an observable level late along the bunch, confirming the spatiotemporal nature of the instability. We provide a rough estimate of the amplitude of the magnetic field generated in the plasma by the instability and show that the associated magnetic energy increases with plasma density.

Published
2024
Full Text
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6. Development of the self-modulation instability of a relativistic proton bunch in plasma

Author

Verra, L., Wyler, S., Nechaeva, T., Pucek, J., Bencini, V., Bergamaschi, M., Ranc, L., Zevi Della Porta, G., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Amoedo, C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. a., Kim, S. -y., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Morales Guzman, P. I., Moreira, M., Pakuza, C., Pannell, F., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Turner, M., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., Zepp, M., Verra, L., Wyler, S., Nechaeva, T., Pucek, J., Bencini, V., Bergamaschi, M., Ranc, L., Zevi Della Porta, G., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Amoedo, C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. a., Kim, S. -y., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Morales Guzman, P. I., Moreira, M., Pakuza, C., Pannell, F., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Turner, M., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., and Zepp, M.

Abstract

Self-modulation is a beam-plasma instability that is useful to drive large-amplitude wakefields with bunches much longer than the plasma skin depth. We present experimental results showing that, when increasing the ratio between the initial transverse size of the bunch and the plasma skin depth, the instability occurs later along the bunch, or not at all, over a fixed plasma length because the amplitude of the initial wakefields decreases. We show cases for which self-modulation does not develop, and we introduce a simple model discussing the conditions for which it would not occur after any plasma length. Changing bunch size and plasma electron density also changes the growth rate of the instability. We discuss the impact of these results on the design of a particle accelerator based on the self-modulation instability seeded by a relativistic ionization front, such as the future upgrade of the Advanced WAKefield Experiment.

Published
2023
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7. Development of the self-modulation instability of a relativistic proton bunch in plasma

Author

Verra, L., Wyler, S., Nechaeva, T., Pucek, J., Bencini, V., Bergamaschi, M., Ranc, L., Zevi Della Porta, G., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Amoedo, C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. a., Kim, S. -y., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Morales Guzman, P. I., Moreira, M., Pakuza, C., Pannell, F., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Turner, M., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., Zepp, M., Verra, L., Wyler, S., Nechaeva, T., Pucek, J., Bencini, V., Bergamaschi, M., Ranc, L., Zevi Della Porta, G., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Amoedo, C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. a., Kim, S. -y., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Morales Guzman, P. I., Moreira, M., Pakuza, C., Pannell, F., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Turner, M., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., and Zepp, M.

Abstract

Self-modulation is a beam-plasma instability that is useful to drive large-amplitude wakefields with bunches much longer than the plasma skin depth. We present experimental results showing that, when increasing the ratio between the initial transverse size of the bunch and the plasma skin depth, the instability occurs later along the bunch, or not at all, over a fixed plasma length because the amplitude of the initial wakefields decreases. We show cases for which self-modulation does not develop, and we introduce a simple model discussing the conditions for which it would not occur after any plasma length. Changing bunch size and plasma electron density also changes the growth rate of the instability. We discuss the impact of these results on the design of a particle accelerator based on the self-modulation instability seeded by a relativistic ionization front, such as the future upgrade of the Advanced WAKefield Experiment.

Published
2023
Full Text
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8. Development of the self-modulation instability of a relativistic proton bunch in plasma

Author

Verra, L., Wyler, S., Nechaeva, T., Pucek, J., Bencini, V., Bergamaschi, M., Ranc, L., Zevi Della Porta, G., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Amoedo, C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. a., Kim, S. -y., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Morales Guzman, P. I., Moreira, M., Pakuza, C., Pannell, F., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Turner, M., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., Zepp, M., Verra, L., Wyler, S., Nechaeva, T., Pucek, J., Bencini, V., Bergamaschi, M., Ranc, L., Zevi Della Porta, G., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Amoedo, C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. a., Kim, S. -y., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Morales Guzman, P. I., Moreira, M., Pakuza, C., Pannell, F., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Turner, M., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., and Zepp, M.

Abstract

Self-modulation is a beam-plasma instability that is useful to drive large-amplitude wakefields with bunches much longer than the plasma skin depth. We present experimental results showing that, when increasing the ratio between the initial transverse size of the bunch and the plasma skin depth, the instability occurs later along the bunch, or not at all, over a fixed plasma length because the amplitude of the initial wakefields decreases. We show cases for which self-modulation does not develop, and we introduce a simple model discussing the conditions for which it would not occur after any plasma length. Changing bunch size and plasma electron density also changes the growth rate of the instability. We discuss the impact of these results on the design of a particle accelerator based on the self-modulation instability seeded by a relativistic ionization front, such as the future upgrade of the Advanced WAKefield Experiment.

Published
2023
Full Text
View/download PDF

9. Development of the self-modulation instability of a relativistic proton bunch in plasma

Author

Verra, L., Wyler, S., Nechaeva, T., Pucek, J., Bencini, V., Bergamaschi, M., Ranc, L., Zevi Della Porta, G., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Amoedo, C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. a., Kim, S. -y., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Morales Guzman, P. I., Moreira, M., Pakuza, C., Pannell, F., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Turner, M., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., Zepp, M., Verra, L., Wyler, S., Nechaeva, T., Pucek, J., Bencini, V., Bergamaschi, M., Ranc, L., Zevi Della Porta, G., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Amoedo, C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. a., Kim, S. -y., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Morales Guzman, P. I., Moreira, M., Pakuza, C., Pannell, F., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Turner, M., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., and Zepp, M.

Abstract

Self-modulation is a beam-plasma instability that is useful to drive large-amplitude wakefields with bunches much longer than the plasma skin depth. We present experimental results showing that, when increasing the ratio between the initial transverse size of the bunch and the plasma skin depth, the instability occurs later along the bunch, or not at all, over a fixed plasma length because the amplitude of the initial wakefields decreases. We show cases for which self-modulation does not develop, and we introduce a simple model discussing the conditions for which it would not occur after any plasma length. Changing bunch size and plasma electron density also changes the growth rate of the instability. We discuss the impact of these results on the design of a particle accelerator based on the self-modulation instability seeded by a relativistic ionization front, such as the future upgrade of the Advanced WAKefield Experiment.

Published
2023
Full Text
View/download PDF

10. Development of the self-modulation instability of a relativistic proton bunch in plasma

Author

Verra, L., Wyler, S., Nechaeva, T., Pucek, J., Bencini, V., Bergamaschi, M., Ranc, L., Zevi Della Porta, G., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Amoedo, C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. a., Kim, S. -y., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Morales Guzman, P. I., Moreira, M., Pakuza, C., Pannell, F., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Turner, M., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., Zepp, M., Verra, L., Wyler, S., Nechaeva, T., Pucek, J., Bencini, V., Bergamaschi, M., Ranc, L., Zevi Della Porta, G., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Amoedo, C., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Blanchard, P., Burrows, P. N., Buttenschoen, B., Caldwell, A., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fonseca, R., Furno, I., Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Guran, E., Henderson, J., Kedves, M. a., Kim, S. -y., Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Moon, K., Morales Guzman, P. I., Moreira, M., Pakuza, C., Pannell, F., Pardons, A., Pepitone, Kevin, Poimendidou, E., Pukhov, A., Ramjiawan, R. L., Rey, S., Rossel, R., Saberi, H., Schmitz, O., Senes, E., Silva, F., Silva, L., Spear, B., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Turner, M., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V., and Zepp, M.

Abstract

Self-modulation is a beam-plasma instability that is useful to drive large-amplitude wakefields with bunches much longer than the plasma skin depth. We present experimental results showing that, when increasing the ratio between the initial transverse size of the bunch and the plasma skin depth, the instability occurs later along the bunch, or not at all, over a fixed plasma length because the amplitude of the initial wakefields decreases. We show cases for which self-modulation does not develop, and we introduce a simple model discussing the conditions for which it would not occur after any plasma length. Changing bunch size and plasma electron density also changes the growth rate of the instability. We discuss the impact of these results on the design of a particle accelerator based on the self-modulation instability seeded by a relativistic ionization front, such as the future upgrade of the Advanced WAKefield Experiment.

Published
2023
Full Text
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11. Controlled Growth of the Self-Modulation of a Relativistic Proton Bunch in Plasma

Author

Verra, L., Della Porta, G. Zevi, Pucek, J., Nechaeva, T., Wyler, S., Bergamaschi, M., Senes, E., Guran, E., Moody, J. T., Kedves, M. A., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Goncalves, M. C. A., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bachmann, A-M, Barrientos, D., Batsch, F., Bencini, V, Blanchard, P., Burrows, P. N., Buttenschon, B., Caldwell, A., Chappell, J., Chevallay, E., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fedosseev, V, Fonseca, R., Furno, I, Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Hafych, V, Henderson, J., Huether, M., Khudiakov, V, Kim, S-Y, Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Godoy, D. Medina, Moon, K., Guzman, P. I. Morales, Moreira, M., Nowak, E., Pakuza, C., Panuganti, H., Pardons, A., Pepitone, Kevin, Perera, A., Pukhov, A., Ramjiawan, R. L., Rey, S., Schmitz, O., Silva, F., Silva, L., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V, Zepp, M., Verra, L., Della Porta, G. Zevi, Pucek, J., Nechaeva, T., Wyler, S., Bergamaschi, M., Senes, E., Guran, E., Moody, J. T., Kedves, M. A., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Goncalves, M. C. A., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bachmann, A-M, Barrientos, D., Batsch, F., Bencini, V, Blanchard, P., Burrows, P. N., Buttenschon, B., Caldwell, A., Chappell, J., Chevallay, E., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fedosseev, V, Fonseca, R., Furno, I, Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Hafych, V, Henderson, J., Huether, M., Khudiakov, V, Kim, S-Y, Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Godoy, D. Medina, Moon, K., Guzman, P. I. Morales, Moreira, M., Nowak, E., Pakuza, C., Panuganti, H., Pardons, A., Pepitone, Kevin, Perera, A., Pukhov, A., Ramjiawan, R. L., Rey, S., Schmitz, O., Silva, F., Silva, L., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V, and Zepp, M.

Abstract

A long, narrow, relativistic charged particle bunch propagating in plasma is subject to the self -modulation (SM) instability. We show that SM of a proton bunch can be seeded by the wakefields driven by a preceding electron bunch. SM timing reproducibility and control are at the level of a small fraction of the modulation period. With this seeding method, we independently control the amplitude of the seed wakefields with the charge of the electron bunch and the growth rate of SM with the charge of the proton bunch. Seeding leads to larger growth of the wakefields than in the instability case.

Published
2022
Full Text
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12. Controlled Growth of the Self-Modulation of a Relativistic Proton Bunch in Plasma

Author

Verra, L., Della Porta, G. Zevi, Pucek, J., Nechaeva, T., Wyler, S., Bergamaschi, M., Senes, E., Guran, E., Moody, J. T., Kedves, M. A., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Goncalves, M. C. A., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bachmann, A-M, Barrientos, D., Batsch, F., Bencini, V, Blanchard, P., Burrows, P. N., Buttenschon, B., Caldwell, A., Chappell, J., Chevallay, E., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fedosseev, V, Fonseca, R., Furno, I, Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Hafych, V, Henderson, J., Huether, M., Khudiakov, V, Kim, S-Y, Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Godoy, D. Medina, Moon, K., Guzman, P. I. Morales, Moreira, M., Nowak, E., Pakuza, C., Panuganti, H., Pardons, A., Pepitone, Kevin, Perera, A., Pukhov, A., Ramjiawan, R. L., Rey, S., Schmitz, O., Silva, F., Silva, L., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V, Zepp, M., Verra, L., Della Porta, G. Zevi, Pucek, J., Nechaeva, T., Wyler, S., Bergamaschi, M., Senes, E., Guran, E., Moody, J. T., Kedves, M. A., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Goncalves, M. C. A., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bachmann, A-M, Barrientos, D., Batsch, F., Bencini, V, Blanchard, P., Burrows, P. N., Buttenschon, B., Caldwell, A., Chappell, J., Chevallay, E., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fedosseev, V, Fonseca, R., Furno, I, Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Hafych, V, Henderson, J., Huether, M., Khudiakov, V, Kim, S-Y, Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Godoy, D. Medina, Moon, K., Guzman, P. I. Morales, Moreira, M., Nowak, E., Pakuza, C., Panuganti, H., Pardons, A., Pepitone, Kevin, Perera, A., Pukhov, A., Ramjiawan, R. L., Rey, S., Schmitz, O., Silva, F., Silva, L., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V, and Zepp, M.

Abstract

A long, narrow, relativistic charged particle bunch propagating in plasma is subject to the self -modulation (SM) instability. We show that SM of a proton bunch can be seeded by the wakefields driven by a preceding electron bunch. SM timing reproducibility and control are at the level of a small fraction of the modulation period. With this seeding method, we independently control the amplitude of the seed wakefields with the charge of the electron bunch and the growth rate of SM with the charge of the proton bunch. Seeding leads to larger growth of the wakefields than in the instability case.

Published
2022
Full Text
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13. Controlled Growth of the Self-Modulation of a Relativistic Proton Bunch in Plasma

Author

Verra, L., Della Porta, G. Zevi, Pucek, J., Nechaeva, T., Wyler, S., Bergamaschi, M., Senes, E., Guran, E., Moody, J. T., Kedves, M. A., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Goncalves, M. C. A., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bachmann, A-M, Barrientos, D., Batsch, F., Bencini, V, Blanchard, P., Burrows, P. N., Buttenschon, B., Caldwell, A., Chappell, J., Chevallay, E., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fedosseev, V, Fonseca, R., Furno, I, Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Hafych, V, Henderson, J., Huether, M., Khudiakov, V, Kim, S-Y, Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Godoy, D. Medina, Moon, K., Guzman, P. I. Morales, Moreira, M., Nowak, E., Pakuza, C., Panuganti, H., Pardons, A., Pepitone, Kevin, Perera, A., Pukhov, A., Ramjiawan, R. L., Rey, S., Schmitz, O., Silva, F., Silva, L., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V, Zepp, M., Verra, L., Della Porta, G. Zevi, Pucek, J., Nechaeva, T., Wyler, S., Bergamaschi, M., Senes, E., Guran, E., Moody, J. T., Kedves, M. A., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Goncalves, M. C. A., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bachmann, A-M, Barrientos, D., Batsch, F., Bencini, V, Blanchard, P., Burrows, P. N., Buttenschon, B., Caldwell, A., Chappell, J., Chevallay, E., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fedosseev, V, Fonseca, R., Furno, I, Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Hafych, V, Henderson, J., Huether, M., Khudiakov, V, Kim, S-Y, Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Godoy, D. Medina, Moon, K., Guzman, P. I. Morales, Moreira, M., Nowak, E., Pakuza, C., Panuganti, H., Pardons, A., Pepitone, Kevin, Perera, A., Pukhov, A., Ramjiawan, R. L., Rey, S., Schmitz, O., Silva, F., Silva, L., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V, and Zepp, M.

Abstract

A long, narrow, relativistic charged particle bunch propagating in plasma is subject to the self -modulation (SM) instability. We show that SM of a proton bunch can be seeded by the wakefields driven by a preceding electron bunch. SM timing reproducibility and control are at the level of a small fraction of the modulation period. With this seeding method, we independently control the amplitude of the seed wakefields with the charge of the electron bunch and the growth rate of SM with the charge of the proton bunch. Seeding leads to larger growth of the wakefields than in the instability case.

Published
2022
Full Text
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14. Controlled Growth of the Self-Modulation of a Relativistic Proton Bunch in Plasma

Author

Verra, L., Della Porta, G. Zevi, Pucek, J., Nechaeva, T., Wyler, S., Bergamaschi, M., Senes, E., Guran, E., Moody, J. T., Kedves, M. A., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Goncalves, M. C. A., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bachmann, A-M, Barrientos, D., Batsch, F., Bencini, V, Blanchard, P., Burrows, P. N., Buttenschon, B., Caldwell, A., Chappell, J., Chevallay, E., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fedosseev, V, Fonseca, R., Furno, I, Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Hafych, V, Henderson, J., Huether, M., Khudiakov, V, Kim, S-Y, Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Godoy, D. Medina, Moon, K., Guzman, P. I. Morales, Moreira, M., Nowak, E., Pakuza, C., Panuganti, H., Pardons, A., Pepitone, Kevin, Perera, A., Pukhov, A., Ramjiawan, R. L., Rey, S., Schmitz, O., Silva, F., Silva, L., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V, Zepp, M., Verra, L., Della Porta, G. Zevi, Pucek, J., Nechaeva, T., Wyler, S., Bergamaschi, M., Senes, E., Guran, E., Moody, J. T., Kedves, M. A., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Goncalves, M. C. A., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bachmann, A-M, Barrientos, D., Batsch, F., Bencini, V, Blanchard, P., Burrows, P. N., Buttenschon, B., Caldwell, A., Chappell, J., Chevallay, E., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fedosseev, V, Fonseca, R., Furno, I, Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Hafych, V, Henderson, J., Huether, M., Khudiakov, V, Kim, S-Y, Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Godoy, D. Medina, Moon, K., Guzman, P. I. Morales, Moreira, M., Nowak, E., Pakuza, C., Panuganti, H., Pardons, A., Pepitone, Kevin, Perera, A., Pukhov, A., Ramjiawan, R. L., Rey, S., Schmitz, O., Silva, F., Silva, L., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V, and Zepp, M.

Abstract

A long, narrow, relativistic charged particle bunch propagating in plasma is subject to the self -modulation (SM) instability. We show that SM of a proton bunch can be seeded by the wakefields driven by a preceding electron bunch. SM timing reproducibility and control are at the level of a small fraction of the modulation period. With this seeding method, we independently control the amplitude of the seed wakefields with the charge of the electron bunch and the growth rate of SM with the charge of the proton bunch. Seeding leads to larger growth of the wakefields than in the instability case.

Published
2022
Full Text
View/download PDF

15. Controlled Growth of the Self-Modulation of a Relativistic Proton Bunch in Plasma

Author

Verra, L., Della Porta, G. Zevi, Pucek, J., Nechaeva, T., Wyler, S., Bergamaschi, M., Senes, E., Guran, E., Moody, J. T., Kedves, M. A., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Goncalves, M. C. A., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bachmann, A-M, Barrientos, D., Batsch, F., Bencini, V, Blanchard, P., Burrows, P. N., Buttenschon, B., Caldwell, A., Chappell, J., Chevallay, E., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fedosseev, V, Fonseca, R., Furno, I, Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Hafych, V, Henderson, J., Huether, M., Khudiakov, V, Kim, S-Y, Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Godoy, D. Medina, Moon, K., Guzman, P. I. Morales, Moreira, M., Nowak, E., Pakuza, C., Panuganti, H., Pardons, A., Pepitone, Kevin, Perera, A., Pukhov, A., Ramjiawan, R. L., Rey, S., Schmitz, O., Silva, F., Silva, L., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V, Zepp, M., Verra, L., Della Porta, G. Zevi, Pucek, J., Nechaeva, T., Wyler, S., Bergamaschi, M., Senes, E., Guran, E., Moody, J. T., Kedves, M. A., Gschwendtner, E., Muggli, P., Agnello, R., Ahdida, C. C., Goncalves, M. C. A., Andrebe, Y., Apsimon, O., Apsimon, R., Arnesano, J. M., Bachmann, A-M, Barrientos, D., Batsch, F., Bencini, V, Blanchard, P., Burrows, P. N., Buttenschon, B., Caldwell, A., Chappell, J., Chevallay, E., Chung, M., Cooke, D. A., Davut, C., Demeter, G., Dexter, A. C., Doebert, S., Elverson, F. A., Farmer, J., Fasoli, A., Fedosseev, V, Fonseca, R., Furno, I, Gorn, A., Granados, E., Granetzny, M., Graubner, T., Grulke, O., Hafych, V, Henderson, J., Huether, M., Khudiakov, V, Kim, S-Y, Kraus, F., Krupa, M., Lefevre, T., Liang, L., Liu, S., Lopes, N., Lotov, K., Calderon, M. Martinez, Mazzoni, S., Godoy, D. Medina, Moon, K., Guzman, P. I. Morales, Moreira, M., Nowak, E., Pakuza, C., Panuganti, H., Pardons, A., Pepitone, Kevin, Perera, A., Pukhov, A., Ramjiawan, R. L., Rey, S., Schmitz, O., Silva, F., Silva, L., Stollberg, C., Sublet, A., Swain, C., Topaloudis, A., Torrado, N., Tuev, P., Velotti, F., Verzilov, V., Vieira, J., Weidl, M., Welsch, C., Wendt, M., Wing, M., Wolfenden, J., Woolley, B., Xia, G., Yarygova, V, and Zepp, M.

Abstract

A long, narrow, relativistic charged particle bunch propagating in plasma is subject to the self -modulation (SM) instability. We show that SM of a proton bunch can be seeded by the wakefields driven by a preceding electron bunch. SM timing reproducibility and control are at the level of a small fraction of the modulation period. With this seeding method, we independently control the amplitude of the seed wakefields with the charge of the electron bunch and the growth rate of SM with the charge of the proton bunch. Seeding leads to larger growth of the wakefields than in the instability case.

Published
2022
Full Text
View/download PDF

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