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Sản Xuất Tia Cosmi Trong Các Siêu Nova
Tóm tắt
Chúng tôi đưa ra một cái nhìn tổng quan ngắn gọn về nguồn gốc và sự gia tốc của tia cosmi (CRs), nhấn mạnh việc sản xuất tia CR tại các giai đoạn khác nhau của sự tiến hóa siêu nova thông qua cơ chế gia tốc sốc Fermi cấp một. Chúng tôi gợi ý rằng các siêu nova với luồng khí siêu tốc, mặc dù khá hiếm, có thể gia tốc tia CR đến năng lượng vượt quá $10^{18}\mbox{ eV}$ trong năm đầu tiên của sự tiến hóa của chúng. Các siêu nova trong các cụm sao trẻ và chặt chẽ, cũng như siêu nova siêu sáng do tương tác cung cấp năng lượng, có thể gia tốc tia CR lên trên chế độ PeV. Chúng tôi thảo luận về sự gia tốc của phần lớn các tia CR thiên văn trong các tàn dư siêu nova cô lập và sự tái gia tốc của các tia CR đã thoát ra bởi nhiều sốc có mặt trong các siêu bóng do các hiệp hội sao OB tạo ra. Các hiệu ứng của việc khuếch đại từ trường do những bất ổn được điều khiển bởi tia CR, cũng như sự vận chuyển tia CR siêu khuếch tán, được thảo luận cho bức xạ phi nhiệt do các sốc phi tuyến với mọi tốc độ, bao gồm cả những sốc siêu tốc.
Từ khóa
#Tia Cosmi #Siêu nova #Gia tốc #Nguồn gốc #Tương tác #Siêu sángTài liệu tham khảo
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