Titlebook: Linear Pro-p-Groups of Finite Width; Gundel Klaas,Charles R. Leedham-Green,Wilhelm Ples Book 1997 Springer-Verlag Berlin Heidelberg 1997 L

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書(shū)目名稱(chēng)Linear Pro-p-Groups of Finite Width影響因子(影響力)




書(shū)目名稱(chēng)Linear Pro-p-Groups of Finite Width影響因子(影響力)學(xué)科排名




書(shū)目名稱(chēng)Linear Pro-p-Groups of Finite Width網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱(chēng)Linear Pro-p-Groups of Finite Width網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




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虛情假意

0075-8434 c .p. analogues are investigated. These groups have finite width, i.e. the indices of the sucessive terms of the lower central series are bounded since they become periodic. The richness of the lattice of normal subgroups is studied by the notion of obliquity. All just infinite maximal groups with L

增長(zhǎng)

Book 1997s up to dimension 14 and most Chevalley groups and classical groups in characteristic 0 and .p. are covered. The methods use computers in small cases and are purely theoretical for the infinite series using root systems or orders with involutions.

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Androgen

Gundel Klaas,Charles R. Leedham-Green,Wilhelm Pleskenible for its effective utilisation. In addition to the incentive of working for personal gain there is the attraction of being in sole control of the enterprise, with the right to take all business decisions. There are, however, some obvious disadvantages to this form of organisation. Successful tra

外科醫(yī)生

BRAWL

Commentary

Gundel Klaas,Charles R. Leedham-Green,Wilhelm Pleskenld at the undergraduate level. The reader is supposed to have only a high school training in physics and mathematics. In many respects this Introduction to Advanced Astrophysics could represent a volume of the Berkeley Physics Course. Thus, the primary audience for this work is composed of students

艦旗

Gundel Klaas,Charles R. Leedham-Green,Wilhelm Pleskenn this field at the undergraduate level. The reader is supposed to have only a high school training in physics and mathematics. In many respects this Introduction to Advanced Astrophysics could represent a volume of the Berkeley Physics Course. Thus, the primary audience for this work is composed of

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