Klassik mexanikada Appell harakat tenglamasi (Gibbs-Appell harakat tenglamasi) 1879-yilda Josia Uillard Gibbs [1] va 1900-yilda Pol Emil Appell [2] tomonidan tasvirlangan klassik mexanikaning muqobil umumiy formulasidir.

Bayonot

Gibbs-Appell tenglamasi quyidagicha

Qr=∂S∂αr,{\displaystyle Q_{r} = \frac{\partial S}{\partial \alpha_{r}},}

bu yerda αr=qr¨{\displaystyle \alpha_r=\ddot{q_r}} ixtiyoriy umumlashtirilgan tezlanish yoki umumlashtirilgan koordinatalarning ikkinchi marta hosilasidir. qr{\displaystyle q_r}, va Qr{\displaystyle Q_r} uning tegishli umumlashgan kuchidir . Umumlashtirilgan kuch bajarilgan ishni beradi

dW=∑r=1DQrdqr,{\displaystyle dW = \sum_{r=1}^{D} Q_{r} dq_{r},}

indeks bu yerda r{\displaystyle r} ustidan yuguradi D{\displaystyle D} umumlashtirilgan koordinatalar qr{\displaystyle q_r}, bu odatda tizimning erkinlik darajalariga mos keladi. Funktsiya S{\displaystyle S} zarracha tezlanishlarining massaviy yigʻindisi kvadrati sifatida aniqlanadi,

S=12∑k=1Nmkak2,{\displaystyle S = \frac{1}{2} \sum_{k=1}^{N} m_{k} \mathbf{a}_{k}^{2}\,,}

indeks bu yerda k{\displaystyle k} ustidan yuguradi K{\displaystyle K} zarralar va

ak=r¨k=d2rkdt2{\displaystyle \mathbf{a}_k = \ddot{\mathbf{r}}_k = \frac{d^2 \mathbf{r}_k}{dt^2}}

ning tezlashishi hisoblanadi k{\displaystyle k} -chi zarra, uning pozitsiya vektorining ikkinchi marta hosilasi rk{\displaystyle \mathbf{r}_k} . Har biri rk{\displaystyle \mathbf{r}_k} umumlashtirilgan koordinatalar bilan ifodalanadi, va ak{\displaystyle \mathbf{a}_k} umumlashgan tezlanishlar bilan ifodalanadi.

Klassik mexanikaning boshqa formulalari bilan aloqalari

Appellning formulasi klassik mexanikaga hech qanday yangi fizikani kiritmaydi va shuning uchun Lagrang mexanikasi va Gamilton mexanikasi kabi klassik mexanikaning boshqa reformulalariga tengdir. Barcha klassik mexanika Nyutonning harakat qonunlarida mavjud. Baʼzi hollarda Appellning harakat tenglamasi odatda ishlatiladigan Lagranj mexanikasiga qaraganda qulayroq boʻlishi mumkin, ayniqsa golonomik boʻlmagan cheklovlar ishtirok etganda. Aslida, Appell tenglamasi toʻgʻridan-toʻgʻri Lagranjning harakat tenglamalariga olib keladi. [3] Bundan tashqari, u murakkab kosmik kemalarning harakatini tavsiflash uchun juda mos keladigan Keyn tenglamalarini olish uchun ishlatilishi mumkin. [4] Appell formulasi Gaussning eng kam cheklash printsipining qoʻllanilishidir. [5]

Chiqarish

D umumlashtirilgan koordinatalarining cheksiz kichik oʻzgarishi uchun zarrachalarning joylashuvi r k oʻzgarishi

drk=∑r=1Ddqr∂rk∂qr{\displaystyle d\mathbf{r}_{k} = \sum_{r=1}^{D} dq_{r} \frac{\partial \mathbf{r}_{k}}{\partial q_{r}}}

Vaqtga nisbatan ikkita hosila olish tezlashuvlar uchun ekvivalent tenglamani beradi.

∂ak∂αr=∂rk∂qr{\displaystyle \frac{\partial \mathbf{a}_{k}}{\partial \alpha_{r}} = \frac{\partial \mathbf{r}_{k}}{\partial q_{r}}}

Umumlashtirilgan koordinatalarda cheksiz kichik oʻzgarish dq r tomonidan bajarilgan ish

dW=∑r=1DQrdqr=∑k=1NFk⋅drk=∑k=1Nmkak⋅drk{\displaystyle dW = \sum_{r=1}^{D} Q_{r} dq_{r} = \sum_{k=1}^{N} \mathbf{F}_{k} \cdot d\mathbf{r}_{k} = \sum_{k=1}^{N} m_{k} \mathbf{a}_{k} \cdot d\mathbf{r}_{k}}

bu yerda k -chi zarra uchun Nyutonning ikkinchi qonuni

Fk=mkak{\displaystyle \mathbf{F}_k = m_k\mathbf{a}_k}

ishlatilgan. Formulani d r k oʻrniga qoʻyish va ikkita yigʻindining tartibini almashtirsak, formulalar hosil boʻladi.

dW=∑r=1DQrdqr=∑k=1Nmkak⋅∑r=1Ddqr(∂rk∂qr)=∑r=1Ddqr∑k=1Nmkak⋅(∂rk∂qr){\displaystyle dW = \sum_{r=1}^{D} Q_{r} dq_{r} = \sum_{k=1}^{N} m_{k} \mathbf{a}_{k} \cdot \sum_{r=1}^{D} dq_{r} \left( \frac{\partial \mathbf{r}_{k}}{\partial q_{r}} \right) = \sum_{r=1}^{D} dq_{r} \sum_{k=1}^{N} m_{k} \mathbf{a}_{k} \cdot \left( \frac{\partial \mathbf{r}_{k}}{\partial q_{r}} \right)}

Shuning uchun umumlashgan kuchlar

Qr=∑k=1Nmkak⋅(∂rk∂qr)=∑k=1Nmkak⋅(∂ak∂αr){\displaystyle Q_{r} = \sum_{k=1}^{N} m_{k} \mathbf{a}_{k} \cdot \left( \frac{\partial \mathbf{r}_{k}}{\partial q_{r}} \right) = \sum_{k=1}^{N} m_{k} \mathbf{a}_{k} \cdot \left( \frac{\partial \mathbf{a}_{k}}{\partial \alpha_{r}} \right)}

Bu umumlashtirilgan tezlanishlarga nisbatan S ning hosilasiga teng

∂S∂αr=∂∂αr12∑k=1Nmk|ak|2=∑k=1Nmkak⋅(∂ak∂αr){\displaystyle \frac{\partial S}{\partial \alpha_{r}} = \frac{\partial}{\partial \alpha_{r}} \frac{1}{2} \sum_{k=1}^{N} m_{k} \left| \mathbf{a}_{k} \right|^{2} = \sum_{k=1}^{N} m_{k} \mathbf{a}_{k} \cdot \left( \frac{\partial \mathbf{a}_{k}}{\partial \alpha_{r}} \right)}

Appellning harakat tenglamasi olinadi

∂S∂αr=Qr.{\displaystyle \frac{\partial S}{\partial \alpha_{r}} = Q_{r}.}

Misollar

Qattiq jismlar dinamikasining Eyler tenglamalari

Eyler tenglamalari Appell formulasining ajoyib tasvirini beradi.

Qattiq tayoqchalar bilan birlashtirilgan N zarrachaning qattiq tanasini koʻrib chiqaylik. Tananing aylanishini burchak tezligi vektori bilan tasvirlash mumkin ω{\displaystyle \boldsymbol\omega}, va mos keladigan burchak tezlanish vektori

α=dωdt{\displaystyle \boldsymbol\alpha = \frac{d\boldsymbol\omega}{dt}}

Aylanish uchun umumlashtirilgan kuch moment hisoblanadi N{\displaystyle \textbf{N}}, cheksiz kichik aylanish uchun bajarilgan ish beri δϕ{\displaystyle \delta \boldsymbol\phi} hisoblanadi dW=N⋅δϕ{\displaystyle dW = \mathbf{N} \cdot \delta \boldsymbol\phi} . ning tezligi k{\displaystyle k} -chi zarracha tomonidan berilgan

vk=ω×rk{\displaystyle \mathbf{v}_{k} = \boldsymbol\omega \times \mathbf{r}_{k}}

bu yerda rk{\displaystyle \mathbf{r}_{k}} zarrachaning Dekart koordinatalaridagi holati; uning mos keladigan tezlanishi

ak=dvkdt=α×rk+ω×vk{\displaystyle \mathbf{a}_{k} = \frac{d\mathbf{v}_{k}}{dt} = \boldsymbol\alpha \times \mathbf{r}_{k} + \boldsymbol\omega \times \mathbf{v}_{k}}

Shuning uchun, funktsiya S{\displaystyle S} sifatida yozilishi mumkin

S=12∑k=1Nmk(ak⋅ak)=12∑k=1Nmk{(α×rk)2+(ω×vk)2+2(α×rk)⋅(ω×vk)}{\displaystyle S = \frac{1}{2} \sum_{k=1}^{N} m_{k} \left( \mathbf{a}_{k} \cdot \mathbf{a}_{k} \right) = \frac{1}{2} \sum_{k=1}^{N} m_{k} \left\{ \left(\boldsymbol\alpha \times \mathbf{r}_{k} \right)^{2} + \left( \boldsymbol\omega \times \mathbf{v}_{k} \right)^{2} + 2 \left( \boldsymbol\alpha \times \mathbf{r}_{k} \right) \cdot \left(\boldsymbol\omega \times \mathbf{v}_{k}\right) \right\}}

ga nisbatan S ning hosilasini belgilash α{\displaystyle \boldsymbol\alpha} momentga teng Eyler tenglamalarini beradi

Ixxαx−(Iyy−Izz)ωyωz=Nx{\displaystyle I_{xx} \alpha_{x} - \left( I_{yy} - I_{zz} \right)\omega_{y} \omega_{z} = N_{x}}
Iyyαy−(Izz−Ixx)ωzωx=Ny{\displaystyle I_{yy} \alpha_{y} - \left( I_{zz} - I_{xx} \right)\omega_{z} \omega_{x} = N_{y}}
Izzαz−(Ixx−Iyy)ωxωy=Nz{\displaystyle I_{zz} \alpha_{z} - \left( I_{xx} - I_{yy} \right)\omega_{x} \omega_{y} = N_{z}}

Manbalar

Qoʻshimcha adabiyotlar

  1. ↑ Gibbs, JW (1879). "On the Fundamental Formulae of Dynamics.". American Journal of Mathematics 2 (1): 49–64. doi:10.2307/2369196. 
  2. ↑ Appell, P (1900). "Sur une forme générale des équations de la dynamique.". Journal für die reine und angewandte Mathematik 121: 310–?. 
  3. ↑ Deslodge, Edward A. (1988). "The Gibbs–Appell equations of motion". American Journal of Physics 56 (9): 841–46. doi:10.1119/1.15463. https://hal.archives-ouvertes.fr/hal-01399766/file/EAD.pdf. 
  4. ↑ Deslodge, Edward A. (1987). "Relationship between Kane's equations and the Gibbs-Appell equations". Journal of Guidance, Control, and Dynamics (American Institute of Aeronautics and Astronautics) 10 (1): 120–22. doi:10.2514/3.20192. https://archive.org/details/sim_journal-of-guidance-control-and-dynamics_january-february-1987_10_1/page/120. 
  5. ↑ Lewis, Andrew D. (August 1996). "The geometry of the Gibbs-Appell equations and Gauss' principle of least constraint". Reports on Mathematical Physics 38 (1): 11–28. doi:10.1016/0034-4877(96)87675-0. https://hal.archives-ouvertes.fr/hal-01401930/file/ADL.pdf.