文章第一次在基于新的OFDMA框架结构和新的隧道传输技术(tunnel)的基础上评估802.16j的MAC层性能。尽管利用隧道传输已经在802.16j标准中定义了,但是我们找到了一个方法使得隧道的利用能够满足每个业务的QoS要求并且获得更高的MAC效率...文章第一次在基于新的OFDMA框架结构和新的隧道传输技术(tunnel)的基础上评估802.16j的MAC层性能。尽管利用隧道传输已经在802.16j标准中定义了,但是我们找到了一个方法使得隧道的利用能够满足每个业务的QoS要求并且获得更高的MAC效率。不同参数之间的影响,例如MAC的帧大小,MAC协议数据单元(MPDU)的大小,QoS和业务数都在文章分析的范围中。文章的实验结果表明,如要提升效率,标准定义的5种QoS应分为5个不同业务组,并包括在每个中继站(RS)的5个隧道中。文章的结果还表明,逐跳(hop by hop)的隧道比端到端(end to end)的隧道有更好的性能。展开更多
We obtain preliminary limits on a logarithmic correction to the Newtonian gravitational potential by using five binary pulsars： PSR J0737-3039, PSR B 1534＋12, PSR J 1756-2251, PSR B 1913＋ 16 and PSR B2127＋ 11C. Th...We obtain preliminary limits on a logarithmic correction to the Newtonian gravitational potential by using five binary pulsars： PSR J0737-3039, PSR B 1534＋12, PSR J 1756-2251, PSR B 1913＋ 16 and PSR B2127＋ 11C. This kind of correction may originate from fundamental frameworks, like string theories, effective models of grav- ity due to quantum effects and the non-local gravity scheme. We estimate the upper limit of the Tohline-Kuhn-Kruglyak parameter A and the lower limit of the Fabris- Campos parameter α, which parameterize the correction and are connected to each other by αλ = -1. By analyzing the advances of periastron of these binary pulsars, we find that the preliminary upper limit of a is 0.19 ± 0.14 kpc^-1 and the prelimi- nary lower limit of ）, is -5.2 4± 3.8 kpc. They are compatible with the bounds based on dynamics of spiral galaxies but quite different from those given by solar system dynamics. These results indicate that this logarithmic correction might be more ob- servable in current timings of binary pulsars than in motions of the solar system.展开更多
文摘文章第一次在基于新的OFDMA框架结构和新的隧道传输技术(tunnel)的基础上评估802.16j的MAC层性能。尽管利用隧道传输已经在802.16j标准中定义了,但是我们找到了一个方法使得隧道的利用能够满足每个业务的QoS要求并且获得更高的MAC效率。不同参数之间的影响,例如MAC的帧大小,MAC协议数据单元(MPDU)的大小,QoS和业务数都在文章分析的范围中。文章的实验结果表明,如要提升效率,标准定义的5种QoS应分为5个不同业务组,并包括在每个中继站(RS)的5个隧道中。文章的结果还表明,逐跳(hop by hop)的隧道比端到端(end to end)的隧道有更好的性能。
基金Supported by the National Natural Science Foundation of China
文摘We obtain preliminary limits on a logarithmic correction to the Newtonian gravitational potential by using five binary pulsars： PSR J0737-3039, PSR B 1534＋12, PSR J 1756-2251, PSR B 1913＋ 16 and PSR B2127＋ 11C. This kind of correction may originate from fundamental frameworks, like string theories, effective models of grav- ity due to quantum effects and the non-local gravity scheme. We estimate the upper limit of the Tohline-Kuhn-Kruglyak parameter A and the lower limit of the Fabris- Campos parameter α, which parameterize the correction and are connected to each other by αλ = -1. By analyzing the advances of periastron of these binary pulsars, we find that the preliminary upper limit of a is 0.19 ± 0.14 kpc^-1 and the prelimi- nary lower limit of ）, is -5.2 4± 3.8 kpc. They are compatible with the bounds based on dynamics of spiral galaxies but quite different from those given by solar system dynamics. These results indicate that this logarithmic correction might be more ob- servable in current timings of binary pulsars than in motions of the solar system.
